BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Date iCal//NONSGML kigkonsult.se iCalcreator 2.18// METHOD:PUBLISH X-WR-CALNAME;VALUE=TEXT:KIAA Events Calendar X-WR-TIMEZONE:Asia/Shanghai BEGIN:VTIMEZONE TZID:Asia/Shanghai X-LIC-LOCATION:Asia/Shangha BEGIN:STANDARD DTSTART:19791021T033000 TZOFFSETFROM:+0800 TZOFFSETTO:+0800 TZNAME:CST END:STANDARD END:VTIMEZONE BEGIN:VEVENT UID:6657@kiaa.pku.edu.cn DTSTAMP:20120221T203847Z CREATED:20120221T203847Z DESCRIPTION:The 2nd Telescope Access Program Workshop DTSTART;TZID=Asia/Shanghai:20120316T000000 DTEND;TZID=Asia/Shanghai:20120317T000000 LAST-MODIFIED:20120221T203847Z LOCATION:National Astronomical Observatories, Chinese Academy of Sciences (NAOC) Beijing, China SUMMARY:The 2nd Telescope Access Program Workshop URL;TYPE=URI:/info/1089/6657.htm END:VEVENT BEGIN:VEVENT UID:4837@kiaa.pku.edu.cn DTSTAMP:20120320T211433Z CREATED:20120320T211433Z DESCRIPTION:Special Lunch Discussion: Recent Sofia Results on PDRs DTSTART;TZID=Asia/Shanghai:20120321T120000 DTEND;TZID=Asia/Shanghai:20120321T120000 LAST-MODIFIED:20120320T211433Z LOCATION: SUMMARY:Special Lunch Discussion: Recent Sofia Results on PDRs URL;TYPE=URI:/info/1025/4837.htm END:VEVENT BEGIN:VEVENT UID:3890@kiaa.pku.edu.cn DTSTAMP:20120320T212555Z CREATED:20120320T212555Z DESCRIPTION:Fundamental physics from astronomical observations DTSTART;TZID=Asia/Shanghai:20120322T160000 DTEND;TZID=Asia/Shanghai:20120322T160000 LAST-MODIFIED:20120320T212555Z LOCATION:KIAA SUMMARY:Fundamental physics from astronomical observations URL;TYPE=URI:/info/1030/3890.htm END:VEVENT BEGIN:VEVENT UID:3891@kiaa.pku.edu.cn DTSTAMP:20120320T212801Z CREATED:20120320T212801Z DESCRIPTION:Galaxy Clusters from Inside to Out: Thermal Instability and Non-thermal Pressure Support DTSTART;TZID=Asia/Shanghai:20120329T160000 DTEND;TZID=Asia/Shanghai:20120329T160000 LAST-MODIFIED:20120320T212801Z LOCATION:KIAA SUMMARY:Galaxy Clusters from Inside to Out: Thermal Instability and Non-thermal Pressure Support URL;TYPE=URI:/info/1030/3891.htm END:VEVENT BEGIN:VEVENT UID:4432@kiaa.pku.edu.cn DTSTAMP:20120320T210128Z CREATED:20120320T210128Z DESCRIPTION:Star Formation in Galaxy Clusters over the Past 10 Billion Years DTSTART;TZID=Asia/Shanghai:20120406T160000 DTEND;TZID=Asia/Shanghai:20120406T160000 LAST-MODIFIED:20120320T210128Z LOCATION:KIAA-PKU SUMMARY:Star Formation in Galaxy Clusters over the Past 10 Billion Years URL;TYPE=URI:/info/1024/4432.htm END:VEVENT BEGIN:VEVENT UID:4433@kiaa.pku.edu.cn DTSTAMP:20120320T210255Z CREATED:20120320T210255Z DESCRIPTION:A golden age in gamma-ray pulsar astrophysics DTSTART;TZID=Asia/Shanghai:20120412T160000 DTEND;TZID=Asia/Shanghai:20120412T160000 LAST-MODIFIED:20120320T210255Z LOCATION:KIAA 1st floor seminar room SUMMARY:A golden age in gamma-ray pulsar astrophysics URL;TYPE=URI:/info/1024/4433.htm END:VEVENT BEGIN:VEVENT UID:4434@kiaa.pku.edu.cn DTSTAMP:20120320T210419Z CREATED:20120320T210419Z DESCRIPTION:The Coevolution of Black Holes and Galaxies DTSTART;TZID=Asia/Shanghai:20120503T160000 DTEND;TZID=Asia/Shanghai:20120503T160000 LAST-MODIFIED:20120320T210419Z LOCATION:KIAA Seminar Room SUMMARY:The Coevolution of Black Holes and Galaxies URL;TYPE=URI:/info/1024/4434.htm END:VEVENT BEGIN:VEVENT UID:4435@kiaa.pku.edu.cn DTSTAMP:20120320T210524Z CREATED:20120320T210524Z DESCRIPTION:A Synthesis of the Cosmic X-ray and Infrared Backgrounds DTSTART;TZID=Asia/Shanghai:20120517T160000 DTEND;TZID=Asia/Shanghai:20120517T160000 LAST-MODIFIED:20120320T210524Z LOCATION:KIAA-PKU SUMMARY:A Synthesis of the Cosmic X-ray and Infrared Backgrounds URL;TYPE=URI:/info/1024/4435.htm END:VEVENT BEGIN:VEVENT UID:4436@kiaa.pku.edu.cn DTSTAMP:20120320T210640Z CREATED:20120320T210640Z DESCRIPTION:Testing the Copernican Principle DTSTART;TZID=Asia/Shanghai:20120524T160000 DTEND;TZID=Asia/Shanghai:20120524T160000 LAST-MODIFIED:20120320T210640Z LOCATION:KIAA-PKU SUMMARY:Testing the Copernican Principle URL;TYPE=URI:/info/1024/4436.htm END:VEVENT BEGIN:VEVENT UID:4838@kiaa.pku.edu.cn DTSTAMP:20120618T151518Z CREATED:20120618T151518Z DESCRIPTION:Observe a Simulated Disk Galaxy DTSTART;TZID=Asia/Shanghai:20120611T120000 DTEND;TZID=Asia/Shanghai:20120611T120000 LAST-MODIFIED:20120618T151518Z LOCATION:DoA, Rm 2907 SUMMARY:Observe a Simulated Disk Galaxy URL;TYPE=URI:/info/1025/4838.htm END:VEVENT BEGIN:VEVENT UID:4437@kiaa.pku.edu.cn DTSTAMP:20120320T210748Z CREATED:20120320T210748Z DESCRIPTION:Unified equations of state of neutron stars DTSTART;TZID=Asia/Shanghai:20120621T160000 DTEND;TZID=Asia/Shanghai:20120621T160000 LAST-MODIFIED:20120320T210748Z LOCATION:KIAA Seminar Room SUMMARY:Unified equations of state of neutron stars URL;TYPE=URI:/info/1024/4437.htm END:VEVENT BEGIN:VEVENT UID:6658@kiaa.pku.edu.cn DTSTAMP:20120617T180307Z CREATED:20120617T180307Z DESCRIPTION:Quasar Science with Large Surveys DTSTART;TZID=Asia/Shanghai:20120625T000000 DTEND;TZID=Asia/Shanghai:20120627T000000 LAST-MODIFIED:20120617T180307Z LOCATION:KIAA-PKU SUMMARY:Quasar Science with Large Surveys URL;TYPE=URI:/info/1089/6658.htm END:VEVENT BEGIN:VEVENT UID:4438@kiaa.pku.edu.cn DTSTAMP:20120618T171104Z CREATED:20120618T171104Z DESCRIPTION:Microlensing Planets: A controlled Scientific Experiment Drawn From Absolute Chaos DTSTART;TZID=Asia/Shanghai:20120628T160000 DTEND;TZID=Asia/Shanghai:20120628T160000 LAST-MODIFIED:20120618T171104Z LOCATION:KIAA Seminar Room SUMMARY:Microlensing Planets: A controlled Scientific Experiment Drawn From Absolute Chaos URL;TYPE=URI:/info/1024/4438.htm END:VEVENT BEGIN:VEVENT UID:6659@kiaa.pku.edu.cn DTSTAMP:20120617T180605Z CREATED:20120617T180605Z DESCRIPTION:A Workshop on Magnetohydrodynamics and Energetic Particles in Laboratory, Space and Astrophysical Plasmas DTSTART;TZID=Asia/Shanghai:20120704T000000 DTEND;TZID=Asia/Shanghai:20120706T000000 LAST-MODIFIED:20120617T180605Z LOCATION:KIAA-PKU SUMMARY:A Workshop on Magnetohydrodynamics and Energetic Particles in Laboratory, Space and Astrophysical Plasmas URL;TYPE=URI:/info/1089/6659.htm END:VEVENT BEGIN:VEVENT UID:4439@kiaa.pku.edu.cn DTSTAMP:20120703T181709Z CREATED:20120703T181709Z DESCRIPTION:Growth of Supermassive Black Holes and Their Environment at z=6-7 DTSTART;TZID=Asia/Shanghai:20120705T160000 DTEND;TZID=Asia/Shanghai:20120705T160000 LAST-MODIFIED:20120703T181709Z LOCATION:KIAA-PKU Auditorium. SUMMARY:Growth of Supermassive Black Holes and Their Environment at z=6-7 URL;TYPE=URI:/info/1024/4439.htm END:VEVENT BEGIN:VEVENT UID:4840@kiaa.pku.edu.cn DTSTAMP:20120711T104155Z CREATED:20120711T104155Z DESCRIPTION:125GeV Higgs-like boson discovery: Recent results on Higgs search at the LHC! DTSTART;TZID=Asia/Shanghai:20120709T121500 DTEND;TZID=Asia/Shanghai:20120709T131500 LAST-MODIFIED:20120711T104155Z LOCATION:KIAA Seminar Room SUMMARY:125GeV Higgs-like boson discovery: Recent results on Higgs search at the LHC! URL;TYPE=URI:/info/1025/4840.htm END:VEVENT BEGIN:VEVENT UID:6660@kiaa.pku.edu.cn DTSTAMP:20120711T104706Z CREATED:20120711T104706Z DESCRIPTION:Lunch Science Discussions DTSTART;TZID=Asia/Shanghai:20120710T121500 DTEND;TZID=Asia/Shanghai:20120710T131500 LAST-MODIFIED:20120711T104706Z LOCATION:KIAA 2nd floor coffee area SUMMARY:Lunch Science Discussions URL;TYPE=URI:/info/1089/6660.htm END:VEVENT BEGIN:VEVENT UID:6661@kiaa.pku.edu.cn DTSTAMP:20120711T104846Z CREATED:20120711T104846Z DESCRIPTION:Science Coffee DTSTART;TZID=Asia/Shanghai:20120712T100000 DTEND;TZID=Asia/Shanghai:20120712T104500 LAST-MODIFIED:20120711T104846Z LOCATION:KIAA 2nd floor coffee area SUMMARY:Science Coffee URL;TYPE=URI:/info/1089/6661.htm END:VEVENT BEGIN:VEVENT UID:6662@kiaa.pku.edu.cn DTSTAMP:20120713T040351Z CREATED:20120713T040351Z DESCRIPTION:Astronomy Summer Camp 2012 DTSTART;TZID=Asia/Shanghai:20120719T090000 DTEND;TZID=Asia/Shanghai:20120722T170000 LAST-MODIFIED:20120713T040351Z LOCATION:KIAA-PKU SUMMARY:Astronomy Summer Camp 2012 URL;TYPE=URI:/info/1089/6662.htm END:VEVENT BEGIN:VEVENT UID:4839@kiaa.pku.edu.cn DTSTAMP:20120703T181933Z CREATED:20120703T181933Z DESCRIPTION:Where are the Obscured AGNs? - Resolving the 6-8 keV X-ray Background DTSTART;TZID=Asia/Shanghai:20120806T120000 DTEND;TZID=Asia/Shanghai:20120806T120000 LAST-MODIFIED:20120703T181933Z LOCATION:DoA, Rm 2907 SUMMARY:Where are the Obscured AGNs? - Resolving the 6-8 keV X-ray Background URL;TYPE=URI:/info/1025/4839.htm END:VEVENT BEGIN:VEVENT UID:6663@kiaa.pku.edu.cn DTSTAMP:20120802T144137Z CREATED:20120802T144137Z DESCRIPTION:Workshop on Fermi Data Analysis DTSTART;TZID=Asia/Shanghai:20120816T090000 DTEND;TZID=Asia/Shanghai:20120817T170000 LAST-MODIFIED:20120802T144137Z LOCATION:KIAA-PKU, Beijing SUMMARY:Workshop on Fermi Data Analysis URL;TYPE=URI:/info/1089/6663.htm END:VEVENT BEGIN:VEVENT UID:4440@kiaa.pku.edu.cn DTSTAMP:20120814T121839Z CREATED:20120814T121839Z DESCRIPTION:Water in space: from interstellar clouds to planet-forming disks DTSTART;TZID=Asia/Shanghai:20120816T160000 DTEND;TZID=Asia/Shanghai:20120816T170000 LAST-MODIFIED:20120814T121839Z LOCATION:KIAA-PKU SUMMARY:Water in space: from interstellar clouds to planet-forming disks URL;TYPE=URI:/info/1024/4440.htm END:VEVENT BEGIN:VEVENT UID:6665@kiaa.pku.edu.cn DTSTAMP:20120816T171349Z CREATED:20120816T171349Z DESCRIPTION:IAU Public Forum DTSTART;TZID=Asia/Shanghai:20120827T200000 DTEND;TZID=Asia/Shanghai:20120827T220000 LAST-MODIFIED:20120816T171349Z LOCATION:KIAA Auditorium SUMMARY:IAU Public Forum URL;TYPE=URI:/info/1089/6665.htm END:VEVENT BEGIN:VEVENT UID:6664@kiaa.pku.edu.cn DTSTAMP:20120814T122306Z CREATED:20120814T122306Z DESCRIPTION:Mini-School of Observations of High-Redshift Galaxies DTSTART;TZID=Asia/Shanghai:20120903T090000 DTEND;TZID=Asia/Shanghai:20120904T170000 LAST-MODIFIED:20120814T122306Z LOCATION:KIAA-PKU, Beijing SUMMARY:Mini-School of Observations of High-Redshift Galaxies URL;TYPE=URI:/info/1089/6664.htm END:VEVENT BEGIN:VEVENT UID:4441@kiaa.pku.edu.cn DTSTAMP:20120913T194126Z CREATED:20120913T194126Z DESCRIPTION:Evolution of massive galaxies: the role of galaxy mergers DTSTART;TZID=Asia/Shanghai:20120913T160000 DTEND;TZID=Asia/Shanghai:20120913T170000 LAST-MODIFIED:20120913T194126Z LOCATION:KIAA-PKU SUMMARY:Evolution of massive galaxies: the role of galaxy mergers URL;TYPE=URI:/info/1024/4441.htm END:VEVENT BEGIN:VEVENT UID:5157@kiaa.pku.edu.cn DTSTAMP:20140722T232255Z CREATED:20140722T232255Z DESCRIPTION:2013 Multi-Messenger Transient Astrophysics Workshop DTSTART;TZID=Asia/Shanghai:20130505T080000 DTEND;TZID=Asia/Shanghai:20130510T080000 LAST-MODIFIED:20140722T232255Z LOCATION:KIAA, Peking University SUMMARY:2013 Multi-Messenger Transient Astrophysics Workshop URL;TYPE=URI:/info/1026/5157.htm END:VEVENT BEGIN:VEVENT UID:4442@kiaa.pku.edu.cn DTSTAMP:20130902T104201Z CREATED:20130902T104201Z DESCRIPTION:Variations of Fundamental Constants with Cosmic History – Pushing the Limits with Radio and (Sub)millimeter Interferometry DTSTART;TZID=Asia/Shanghai:20130905T160000 DTEND;TZID=Asia/Shanghai:20130905T170000 LAST-MODIFIED:20130902T104201Z LOCATION:KIAA-PKU SUMMARY:Variations of Fundamental Constants with Cosmic History – Pushing the Limits with Radio and (Sub)millimeter Interferometry URL;TYPE=URI:/info/1024/4442.htm END:VEVENT BEGIN:VEVENT UID:4443@kiaa.pku.edu.cn DTSTAMP:20130902T104251Z CREATED:20130902T104251Z DESCRIPTION:SUBARU Weak-Lensing Survey of Dark Matter Subhalos in Coma Cluster DTSTART;TZID=Asia/Shanghai:20130926T160000 DTEND;TZID=Asia/Shanghai:20130926T170000 LAST-MODIFIED:20130902T104251Z LOCATION:KIAA-PKU SUMMARY:SUBARU Weak-Lensing Survey of Dark Matter Subhalos in Coma Cluster URL;TYPE=URI:/info/1024/4443.htm END:VEVENT BEGIN:VEVENT UID:4445@kiaa.pku.edu.cn DTSTAMP:20130902T104357Z CREATED:20130902T104357Z DESCRIPTION:Outflow from hot accretion flows DTSTART;TZID=Asia/Shanghai:20131010T104500 DTEND;TZID=Asia/Shanghai:20131010T170000 LAST-MODIFIED:20130902T104357Z LOCATION:KIAA-PKU SUMMARY:Outflow from hot accretion flows URL;TYPE=URI:/info/1024/4445.htm END:VEVENT BEGIN:VEVENT UID:4444@kiaa.pku.edu.cn DTSTAMP:20130902T104357Z CREATED:20130902T104357Z DESCRIPTION:Outflow from hot accretion flows DTSTART;TZID=Asia/Shanghai:20131010T104500 DTEND;TZID=Asia/Shanghai:20131010T170000 LAST-MODIFIED:20130902T104357Z LOCATION:KIAA-PKU SUMMARY:Outflow from hot accretion flows URL;TYPE=URI:/info/1024/4444.htm END:VEVENT BEGIN:VEVENT UID:4446@kiaa.pku.edu.cn DTSTAMP:20131022T141114Z CREATED:20131022T141114Z DESCRIPTION:Why Are AGN So Similar? DTSTART;TZID=Asia/Shanghai:20131024T160000 DTEND;TZID=Asia/Shanghai:20131024T170000 LAST-MODIFIED:20131022T141114Z LOCATION:KIAA-PKU SUMMARY:Why Are AGN So Similar? URL;TYPE=URI:/info/1024/4446.htm END:VEVENT BEGIN:VEVENT UID:4447@kiaa.pku.edu.cn DTSTAMP:20131022T141442Z CREATED:20131022T141442Z DESCRIPTION:Testing Foundations of Modern Cosmology DTSTART;TZID=Asia/Shanghai:20131114T160000 DTEND;TZID=Asia/Shanghai:20131114T170000 LAST-MODIFIED:20131022T141442Z LOCATION:KIAA-PKU SUMMARY:Testing Foundations of Modern Cosmology URL;TYPE=URI:/info/1024/4447.htm END:VEVENT BEGIN:VEVENT UID:4448@kiaa.pku.edu.cn DTSTAMP:20131211T001801Z CREATED:20131211T001801Z DESCRIPTION:The ultra-high energy cosmic rays and their astrophysical sources DTSTART;TZID=Asia/Shanghai:20131212T160000 DTEND;TZID=Asia/Shanghai:20131212T170000 LAST-MODIFIED:20131211T001801Z LOCATION:KIAA-PKU Auditorium SUMMARY:The ultra-high energy cosmic rays and their astrophysical sources URL;TYPE=URI:/info/1024/4448.htm END:VEVENT BEGIN:VEVENT UID:4841@kiaa.pku.edu.cn DTSTAMP:20131211T000212Z CREATED:20131211T000212Z DESCRIPTION:Flowtube dynamics with Athena DTSTART;TZID=Asia/Shanghai:20131216T120000 DTEND;TZID=Asia/Shanghai:20131216T130000 LAST-MODIFIED:20131211T000212Z LOCATION:DoA, Rm 2907 SUMMARY:Flowtube dynamics with Athena URL;TYPE=URI:/info/1025/4841.htm END:VEVENT BEGIN:VEVENT UID:4451@kiaa.pku.edu.cn DTSTAMP:20131212T163035Z CREATED:20131212T163035Z DESCRIPTION:Puzzling accretion onto a black hole in M101 ULX-1 DTSTART;TZID=Asia/Shanghai:20131219T160000 DTEND;TZID=Asia/Shanghai:20131219T170000 LAST-MODIFIED:20131212T163035Z LOCATION:KIAA-PKU Auditorium SUMMARY:Puzzling accretion onto a black hole in M101 ULX-1 URL;TYPE=URI:/info/1024/4451.htm END:VEVENT BEGIN:VEVENT UID:4842@kiaa.pku.edu.cn DTSTAMP:20131211T000313Z CREATED:20131211T000313Z DESCRIPTION:Anti-glitch of magnetar 1E 2259+586 in the wind braking scenario DTSTART;TZID=Asia/Shanghai:20131223T120000 DTEND;TZID=Asia/Shanghai:20131223T130000 LAST-MODIFIED:20131211T000313Z LOCATION:DoA, Rm 2907 SUMMARY:Anti-glitch of magnetar 1E 2259+586 in the wind braking scenario URL;TYPE=URI:/info/1025/4842.htm END:VEVENT BEGIN:VEVENT UID:4843@kiaa.pku.edu.cn DTSTAMP:20131211T000419Z CREATED:20131211T000419Z DESCRIPTION:Mass-radius relations of neutron stars and strange stars DTSTART;TZID=Asia/Shanghai:20131230T120000 DTEND;TZID=Asia/Shanghai:20131230T130000 LAST-MODIFIED:20131211T000419Z LOCATION:DoA, Rm 2907 SUMMARY:Mass-radius relations of neutron stars and strange stars URL;TYPE=URI:/info/1025/4843.htm END:VEVENT BEGIN:VEVENT UID:4449@kiaa.pku.edu.cn DTSTAMP:20131212T162807Z CREATED:20131212T162807Z DESCRIPTION:Implications of the AMS-02 results DTSTART;TZID=Asia/Shanghai:20140102T160000 DTEND;TZID=Asia/Shanghai:20140102T170000 LAST-MODIFIED:20131212T162807Z LOCATION:KIAA-PKU Auditorium SUMMARY:Implications of the AMS-02 results URL;TYPE=URI:/info/1024/4449.htm END:VEVENT BEGIN:VEVENT UID:4844@kiaa.pku.edu.cn DTSTAMP:20131211T000508Z CREATED:20131211T000508Z DESCRIPTION:How much cosmological information can be measured? DTSTART;TZID=Asia/Shanghai:20140106T120000 DTEND;TZID=Asia/Shanghai:20140106T130000 LAST-MODIFIED:20131211T000508Z LOCATION:DoA, Rm 2907 SUMMARY:How much cosmological information can be measured? URL;TYPE=URI:/info/1025/4844.htm END:VEVENT BEGIN:VEVENT UID:4450@kiaa.pku.edu.cn DTSTAMP:20131212T162902Z CREATED:20131212T162902Z DESCRIPTION:Finding Transiting Exoplanets and Characterizing their Atmospheres: HATSouth and ACCESS DTSTART;TZID=Asia/Shanghai:20140109T160000 DTEND;TZID=Asia/Shanghai:20140109T170000 LAST-MODIFIED:20131212T162902Z LOCATION:KIAA-PKU Auditorium SUMMARY:Finding Transiting Exoplanets and Characterizing their Atmospheres: HATSouth and ACCESS URL;TYPE=URI:/info/1024/4450.htm END:VEVENT BEGIN:VEVENT UID:4452@kiaa.pku.edu.cn DTSTAMP:20140111T144926Z CREATED:20140111T144926Z DESCRIPTION:New frontiers in wide-field time-domain X-ray astronomy DTSTART;TZID=Asia/Shanghai:20140116T153000 DTEND;TZID=Asia/Shanghai:20140116T163000 LAST-MODIFIED:20140111T144926Z LOCATION:KIAA-PKU SUMMARY:New frontiers in wide-field time-domain X-ray astronomy URL;TYPE=URI:/info/1024/4452.htm END:VEVENT BEGIN:VEVENT UID:4453@kiaa.pku.edu.cn DTSTAMP:20140218T112823Z CREATED:20140218T112823Z DESCRIPTION:Not-so-simple stellar populations in Local Group star clusters DTSTART;TZID=Asia/Shanghai:20140220T160000 DTEND;TZID=Asia/Shanghai:20140220T170000 LAST-MODIFIED:20140218T112823Z LOCATION:KIAA-PKU Auditorium SUMMARY:Not-so-simple stellar populations in Local Group star clusters URL;TYPE=URI:/info/1024/4453.htm END:VEVENT BEGIN:VEVENT UID:4454@kiaa.pku.edu.cn DTSTAMP:20140218T113007Z CREATED:20140218T113007Z DESCRIPTION:High-Redshift Quasars and Galaxies at the Epoch of Cosmic Reionization DTSTART;TZID=Asia/Shanghai:20140228T160000 DTEND;TZID=Asia/Shanghai:20140228T170000 LAST-MODIFIED:20140218T113007Z LOCATION:KIAA-PKU Auditorium SUMMARY:High-Redshift Quasars and Galaxies at the Epoch of Cosmic Reionization URL;TYPE=URI:/info/1024/4454.htm END:VEVENT BEGIN:VEVENT UID:4845@kiaa.pku.edu.cn DTSTAMP:20140218T173822Z CREATED:20140218T173822Z DESCRIPTION:The major merger impact on the evolution of the spiral and dwarf galaxies DTSTART;TZID=Asia/Shanghai:20140303T120000 DTEND;TZID=Asia/Shanghai:20140303T130000 LAST-MODIFIED:20140218T173822Z LOCATION:DoA, Rm 2907 SUMMARY:The major merger impact on the evolution of the spiral and dwarf galaxies URL;TYPE=URI:/info/1025/4845.htm END:VEVENT BEGIN:VEVENT UID:4455@kiaa.pku.edu.cn DTSTAMP:20140218T113112Z CREATED:20140218T113112Z DESCRIPTION:The Varied Fates of Galaxies in the Young Universe DTSTART;TZID=Asia/Shanghai:20140304T160000 DTEND;TZID=Asia/Shanghai:20140304T170000 LAST-MODIFIED:20140218T113112Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Varied Fates of Galaxies in the Young Universe URL;TYPE=URI:/info/1024/4455.htm END:VEVENT BEGIN:VEVENT UID:4465@kiaa.pku.edu.cn DTSTAMP:20140301T214651Z CREATED:20140301T214651Z DESCRIPTION:All Sky dust modelling with Planck, IRAS and WISE Observations DTSTART;TZID=Asia/Shanghai:20140306T160000 DTEND;TZID=Asia/Shanghai:20140306T170000 LAST-MODIFIED:20140301T214651Z LOCATION:KIAA-PKU Auditorium SUMMARY:All Sky dust modelling with Planck, IRAS and WISE Observations URL;TYPE=URI:/info/1024/4465.htm END:VEVENT BEGIN:VEVENT UID:4456@kiaa.pku.edu.cn DTSTAMP:20140218T114608Z CREATED:20140218T114608Z DESCRIPTION:Active Galactic Nuclei at the Highest Gamma-Ray Energies DTSTART;TZID=Asia/Shanghai:20140313T160000 DTEND;TZID=Asia/Shanghai:20140313T170000 LAST-MODIFIED:20140218T114608Z LOCATION:KIAA-PKU Auditorium SUMMARY:Active Galactic Nuclei at the Highest Gamma-Ray Energies URL;TYPE=URI:/info/1024/4456.htm END:VEVENT BEGIN:VEVENT UID:4846@kiaa.pku.edu.cn DTSTAMP:20140218T181111Z CREATED:20140218T181111Z DESCRIPTION:Planetary crash: New insight into why hot Jupiters are so diverse DTSTART;TZID=Asia/Shanghai:20140317T120000 DTEND;TZID=Asia/Shanghai:20140317T130000 LAST-MODIFIED:20140218T181111Z LOCATION:DoA, Rm 2907 SUMMARY:Planetary crash: New insight into why hot Jupiters are so diverse URL;TYPE=URI:/info/1025/4846.htm END:VEVENT BEGIN:VEVENT UID:4466@kiaa.pku.edu.cn DTSTAMP:20140301T215653Z CREATED:20140301T215653Z DESCRIPTION:Stars in adolescence: wild accretion, manic depression, fits of irrational outbursts, and pimply spots DTSTART;TZID=Asia/Shanghai:20140320T160000 DTEND;TZID=Asia/Shanghai:20140320T170000 LAST-MODIFIED:20140301T215653Z LOCATION:KIAA-PKU Auditorium SUMMARY:Stars in adolescence: wild accretion, manic depression, fits of irrational outbursts, and pimply spots URL;TYPE=URI:/info/1024/4466.htm END:VEVENT BEGIN:VEVENT UID:4847@kiaa.pku.edu.cn DTSTAMP:20140218T182256Z CREATED:20140218T182256Z DESCRIPTION:Characterizing hot-Jupiter atmospheres with Palomar/Hale transit spectroscopy DTSTART;TZID=Asia/Shanghai:20140324T120000 DTEND;TZID=Asia/Shanghai:20140324T130000 LAST-MODIFIED:20140218T182256Z LOCATION:DoA, Rm 2907 SUMMARY:Characterizing hot-Jupiter atmospheres with Palomar/Hale transit spectroscopy URL;TYPE=URI:/info/1025/4847.htm END:VEVENT BEGIN:VEVENT UID:4851@kiaa.pku.edu.cn DTSTAMP:20140304T210146Z CREATED:20140304T210146Z DESCRIPTION:Gas Outflows and Accretion from Distant Star Forming Galaxies DTSTART;TZID=Asia/Shanghai:20140325T120000 DTEND;TZID=Asia/Shanghai:20140325T130000 LAST-MODIFIED:20140304T210146Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Gas Outflows and Accretion from Distant Star Forming Galaxies URL;TYPE=URI:/info/1025/4851.htm END:VEVENT BEGIN:VEVENT UID:4457@kiaa.pku.edu.cn DTSTAMP:20140218T115257Z CREATED:20140218T115257Z DESCRIPTION:Spin-Orbit Interactions for Exoplanetary Systems DTSTART;TZID=Asia/Shanghai:20140327T160000 DTEND;TZID=Asia/Shanghai:20140327T170000 LAST-MODIFIED:20140218T115257Z LOCATION:KIAA-PKU Auditorium SUMMARY:Spin-Orbit Interactions for Exoplanetary Systems URL;TYPE=URI:/info/1024/4457.htm END:VEVENT BEGIN:VEVENT UID:4852@kiaa.pku.edu.cn DTSTAMP:20140313T090616Z CREATED:20140313T090616Z DESCRIPTION:On the lifetime of binary star clusters DTSTART;TZID=Asia/Shanghai:20140331T120000 DTEND;TZID=Asia/Shanghai:20140331T130000 LAST-MODIFIED:20140313T090616Z LOCATION:DoA, Rm 2907 SUMMARY:On the lifetime of binary star clusters URL;TYPE=URI:/info/1025/4852.htm END:VEVENT BEGIN:VEVENT UID:4458@kiaa.pku.edu.cn DTSTAMP:20140218T115403Z CREATED:20140218T115403Z DESCRIPTION:Formation of planetary architecture and the detection of exoplanets in Antarctic DTSTART;TZID=Asia/Shanghai:20140403T160000 DTEND;TZID=Asia/Shanghai:20140403T170000 LAST-MODIFIED:20140218T115403Z LOCATION:KIAA-PKU Auditorium SUMMARY:Formation of planetary architecture and the detection of exoplanets in Antarctic URL;TYPE=URI:/info/1024/4458.htm END:VEVENT BEGIN:VEVENT UID:4459@kiaa.pku.edu.cn DTSTAMP:20140218T115458Z CREATED:20140218T115458Z DESCRIPTION:Multi-scale Outflows in Active Galactic Nuclei DTSTART;TZID=Asia/Shanghai:20140410T160000 DTEND;TZID=Asia/Shanghai:20140410T170000 LAST-MODIFIED:20140218T115458Z LOCATION:KIAA-PKU Auditorium SUMMARY:Multi-scale Outflows in Active Galactic Nuclei URL;TYPE=URI:/info/1024/4459.htm END:VEVENT BEGIN:VEVENT UID:4853@kiaa.pku.edu.cn DTSTAMP:20140313T175621Z CREATED:20140313T175621Z DESCRIPTION:Sculpting the Central Parsec of our Galaxy DTSTART;TZID=Asia/Shanghai:20140414T120000 DTEND;TZID=Asia/Shanghai:20140414T130000 LAST-MODIFIED:20140313T175621Z LOCATION:DoA, Rm 2907 SUMMARY:Sculpting the Central Parsec of our Galaxy URL;TYPE=URI:/info/1025/4853.htm END:VEVENT BEGIN:VEVENT UID:4848@kiaa.pku.edu.cn DTSTAMP:20140218T182334Z CREATED:20140218T182334Z DESCRIPTION:3D Global radiation MHD simulations of Black Hole Accretion Disks DTSTART;TZID=Asia/Shanghai:20140415T120000 DTEND;TZID=Asia/Shanghai:20140415T130000 LAST-MODIFIED:20140218T182334Z LOCATION:KIAA, 1st floor seminar room SUMMARY:3D Global radiation MHD simulations of Black Hole Accretion Disks URL;TYPE=URI:/info/1025/4848.htm END:VEVENT BEGIN:VEVENT UID:4858@kiaa.pku.edu.cn DTSTAMP:20140405T063019Z CREATED:20140405T063019Z DESCRIPTION:How to Make Massive Stars: the First Steps DTSTART;TZID=Asia/Shanghai:20140416T120000 DTEND;TZID=Asia/Shanghai:20140416T130000 LAST-MODIFIED:20140405T063019Z LOCATION:KIAA, 1st floor seminar room SUMMARY:How to Make Massive Stars: the First Steps URL;TYPE=URI:/info/1025/4858.htm END:VEVENT BEGIN:VEVENT UID:4460@kiaa.pku.edu.cn DTSTAMP:20140218T115538Z CREATED:20140218T115538Z DESCRIPTION:A Parsec-scale Jet from The Galactic Center Black Hole: Interaction with Local Gas DTSTART;TZID=Asia/Shanghai:20140417T160000 DTEND;TZID=Asia/Shanghai:20140417T170000 LAST-MODIFIED:20140218T115538Z LOCATION:KIAA-PKU Auditorium SUMMARY:A Parsec-scale Jet from The Galactic Center Black Hole: Interaction with Local Gas URL;TYPE=URI:/info/1024/4460.htm END:VEVENT BEGIN:VEVENT UID:4849@kiaa.pku.edu.cn DTSTAMP:20140218T182422Z CREATED:20140218T182422Z DESCRIPTION:From Red-Nuggets to Giant Ellipticals: Structural Evolution of Massive Galaxies DTSTART;TZID=Asia/Shanghai:20140421T120000 DTEND;TZID=Asia/Shanghai:20140421T130000 LAST-MODIFIED:20140218T182422Z LOCATION:DaO, Rm 2907 SUMMARY:From Red-Nuggets to Giant Ellipticals: Structural Evolution of Massive Galaxies URL;TYPE=URI:/info/1025/4849.htm END:VEVENT BEGIN:VEVENT UID:4461@kiaa.pku.edu.cn DTSTAMP:20140218T115630Z CREATED:20140218T115630Z DESCRIPTION:The Clustered Universe DTSTART;TZID=Asia/Shanghai:20140424T160000 DTEND;TZID=Asia/Shanghai:20140424T170000 LAST-MODIFIED:20140218T115630Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Clustered Universe URL;TYPE=URI:/info/1024/4461.htm END:VEVENT BEGIN:VEVENT UID:4859@kiaa.pku.edu.cn DTSTAMP:20140408T102310Z CREATED:20140408T102310Z DESCRIPTION:Magellanic Clouds: How much do we understand these neighbouring galaxies? DTSTART;TZID=Asia/Shanghai:20140425T120000 DTEND;TZID=Asia/Shanghai:20140425T130000 LAST-MODIFIED:20140408T102310Z LOCATION:KIAA, first floor seminar room SUMMARY:Magellanic Clouds: How much do we understand these neighbouring galaxies? URL;TYPE=URI:/info/1025/4859.htm END:VEVENT BEGIN:VEVENT UID:4862@kiaa.pku.edu.cn DTSTAMP:20140415T185530Z CREATED:20140415T185530Z DESCRIPTION:The earliest stages of black hole and stellar mass growth: news from the 1.2Gyr old Universe DTSTART;TZID=Asia/Shanghai:20140428T120000 DTEND;TZID=Asia/Shanghai:20140428T130000 LAST-MODIFIED:20140415T185530Z LOCATION:DoA, Rm 2907 SUMMARY:The earliest stages of black hole and stellar mass growth: news from the 1.2Gyr old Universe URL;TYPE=URI:/info/1025/4862.htm END:VEVENT BEGIN:VEVENT UID:4856@kiaa.pku.edu.cn DTSTAMP:20140329T235116Z CREATED:20140329T235116Z DESCRIPTION:Detections of supermassive black hole binaries in galactic nuclei DTSTART;TZID=Asia/Shanghai:20140429T120000 DTEND;TZID=Asia/Shanghai:20140429T130000 LAST-MODIFIED:20140329T235116Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Detections of supermassive black hole binaries in galactic nuclei URL;TYPE=URI:/info/1025/4856.htm END:VEVENT BEGIN:VEVENT UID:4863@kiaa.pku.edu.cn DTSTAMP:20140422T150558Z CREATED:20140422T150558Z DESCRIPTION:Nonparametric reconstruction of dark energy Equation of State DTSTART;TZID=Asia/Shanghai:20140505T120000 DTEND;TZID=Asia/Shanghai:20140505T130000 LAST-MODIFIED:20140422T150558Z LOCATION:DoA, Rm 2907 SUMMARY:Nonparametric reconstruction of dark energy Equation of State URL;TYPE=URI:/info/1025/4863.htm END:VEVENT BEGIN:VEVENT UID:4855@kiaa.pku.edu.cn DTSTAMP:20140318T205248Z CREATED:20140318T205248Z DESCRIPTION:Observations of Short Gamma-Ray Bursts and future prospects DTSTART;TZID=Asia/Shanghai:20140508T120000 DTEND;TZID=Asia/Shanghai:20140508T130000 LAST-MODIFIED:20140318T205248Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Observations of Short Gamma-Ray Bursts and future prospects URL;TYPE=URI:/info/1025/4855.htm END:VEVENT BEGIN:VEVENT UID:4463@kiaa.pku.edu.cn DTSTAMP:20140218T115802Z CREATED:20140218T115802Z DESCRIPTION:Microlensing's New Frontier: Parallax DTSTART;TZID=Asia/Shanghai:20140508T160000 DTEND;TZID=Asia/Shanghai:20140508T170000 LAST-MODIFIED:20140218T115802Z LOCATION:KIAA-PKU Auditorium SUMMARY:Microlensing's New Frontier: Parallax URL;TYPE=URI:/info/1024/4463.htm END:VEVENT BEGIN:VEVENT UID:4867@kiaa.pku.edu.cn DTSTAMP:20140505T144840Z CREATED:20140505T144840Z DESCRIPTION:The role of turbulent reconnection diffusion during star formation DTSTART;TZID=Asia/Shanghai:20140509T120000 DTEND;TZID=Asia/Shanghai:20140509T130000 LAST-MODIFIED:20140505T144840Z LOCATION:1st floor seminar room, KIAA SUMMARY:The role of turbulent reconnection diffusion during star formation URL;TYPE=URI:/info/1025/4867.htm END:VEVENT BEGIN:VEVENT UID:4854@kiaa.pku.edu.cn DTSTAMP:20140318T144537Z CREATED:20140318T144537Z DESCRIPTION:White dwarf-main sequence binaries from LAMOST DTSTART;TZID=Asia/Shanghai:20140512T120000 DTEND;TZID=Asia/Shanghai:20140512T130000 LAST-MODIFIED:20140318T144537Z LOCATION:DoA, Rm 2907 SUMMARY:White dwarf-main sequence binaries from LAMOST URL;TYPE=URI:/info/1025/4854.htm END:VEVENT BEGIN:VEVENT UID:4693@kiaa.pku.edu.cn DTSTAMP:20140514T233149Z CREATED:20140514T233149Z DESCRIPTION:Millisecond pulsars as the source of gamma-ray excess in the Galactic Center - no dark matter needed DTSTART;TZID=Asia/Shanghai:20140513T121500 DTEND;TZID=Asia/Shanghai:20140513T131500 LAST-MODIFIED:20140514T233149Z LOCATION:KIAA-PKU SUMMARY:Millisecond pulsars as the source of gamma-ray excess in the Galactic Center - no dark matter needed URL;TYPE=URI:/info/1028/4693.htm END:VEVENT BEGIN:VEVENT UID:4462@kiaa.pku.edu.cn DTSTAMP:20140218T115725Z CREATED:20140218T115725Z DESCRIPTION:Cosmology and its large scale probes DTSTART;TZID=Asia/Shanghai:20140515T160000 DTEND;TZID=Asia/Shanghai:20140515T170000 LAST-MODIFIED:20140218T115725Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmology and its large scale probes URL;TYPE=URI:/info/1024/4462.htm END:VEVENT BEGIN:VEVENT UID:4860@kiaa.pku.edu.cn DTSTAMP:20140408T155631Z CREATED:20140408T155631Z DESCRIPTION:Transitional Disks: Signatures of Gap Opening by Young Planets? DTSTART;TZID=Asia/Shanghai:20140516T120000 DTEND;TZID=Asia/Shanghai:20140516T130000 LAST-MODIFIED:20140408T155631Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Transitional Disks: Signatures of Gap Opening by Young Planets? URL;TYPE=URI:/info/1025/4860.htm END:VEVENT BEGIN:VEVENT UID:4467@kiaa.pku.edu.cn DTSTAMP:20140312T095139Z CREATED:20140312T095139Z DESCRIPTION:Unavoidable spectral distortions of the Cosmic Background Radiation DTSTART;TZID=Asia/Shanghai:20140516T160000 DTEND;TZID=Asia/Shanghai:20140516T170000 LAST-MODIFIED:20140312T095139Z LOCATION:KIAA-PKU Auditorium SUMMARY:Unavoidable spectral distortions of the Cosmic Background Radiation URL;TYPE=URI:/info/1024/4467.htm END:VEVENT BEGIN:VEVENT UID:4857@kiaa.pku.edu.cn DTSTAMP:20140404T124027Z CREATED:20140404T124027Z DESCRIPTION:Testing the nature of astrophysical black hole candidates DTSTART;TZID=Asia/Shanghai:20140519T120000 DTEND;TZID=Asia/Shanghai:20140519T130000 LAST-MODIFIED:20140404T124027Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Testing the nature of astrophysical black hole candidates URL;TYPE=URI:/info/1025/4857.htm END:VEVENT BEGIN:VEVENT UID:4468@kiaa.pku.edu.cn DTSTAMP:20140411T214234Z CREATED:20140411T214234Z DESCRIPTION:Asteroseismology for Galactic Archaeology: bridging two fields DTSTART;TZID=Asia/Shanghai:20140522T160000 DTEND;TZID=Asia/Shanghai:20140522T170000 LAST-MODIFIED:20140411T214234Z LOCATION:KIAA-PKU Auditorium SUMMARY:Asteroseismology for Galactic Archaeology: bridging two fields URL;TYPE=URI:/info/1024/4468.htm END:VEVENT BEGIN:VEVENT UID:4866@kiaa.pku.edu.cn DTSTAMP:20140505T103102Z CREATED:20140505T103102Z DESCRIPTION:A Method for Identifying M dwarfs with Ultra Cool Companions in 2MASS and WISE DTSTART;TZID=Asia/Shanghai:20140523T120000 DTEND;TZID=Asia/Shanghai:20140523T130000 LAST-MODIFIED:20140505T103102Z LOCATION:KIAA, 1st floor seminar room SUMMARY:A Method for Identifying M dwarfs with Ultra Cool Companions in 2MASS and WISE URL;TYPE=URI:/info/1025/4866.htm END:VEVENT BEGIN:VEVENT UID:4850@kiaa.pku.edu.cn DTSTAMP:20140227T135045Z CREATED:20140227T135045Z DESCRIPTION:Gas Accretion, Galactic Winds and the Circumgalactic Medium in Cosmological Galaxy Formation Simulations DTSTART;TZID=Asia/Shanghai:20140526T120000 DTEND;TZID=Asia/Shanghai:20140526T130000 LAST-MODIFIED:20140227T135045Z LOCATION:Room 2907, the Department of Astronomy SUMMARY:Gas Accretion, Galactic Winds and the Circumgalactic Medium in Cosmological Galaxy Formation Simulations URL;TYPE=URI:/info/1025/4850.htm END:VEVENT BEGIN:VEVENT UID:4464@kiaa.pku.edu.cn DTSTAMP:20140218T115846Z CREATED:20140218T115846Z DESCRIPTION:Satellite galaxies in Milky Way DTSTART;TZID=Asia/Shanghai:20140529T160000 DTEND;TZID=Asia/Shanghai:20140529T170000 LAST-MODIFIED:20140218T115846Z LOCATION:KIAA-PKU Auditorium SUMMARY:Satellite galaxies in Milky Way URL;TYPE=URI:/info/1024/4464.htm END:VEVENT BEGIN:VEVENT UID:4865@kiaa.pku.edu.cn DTSTAMP:20140429T185500Z CREATED:20140429T185500Z DESCRIPTION:Dynamical evolution of globular cluster systems and their cosmological origin DTSTART;TZID=Asia/Shanghai:20140606T120000 DTEND;TZID=Asia/Shanghai:20140606T130000 LAST-MODIFIED:20140429T185500Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Dynamical evolution of globular cluster systems and their cosmological origin URL;TYPE=URI:/info/1025/4865.htm END:VEVENT BEGIN:VEVENT UID:4869@kiaa.pku.edu.cn DTSTAMP:20140524T192046Z CREATED:20140524T192046Z DESCRIPTION:Low luminosity GRBs: A different class, shock breakout and afterglow DTSTART;TZID=Asia/Shanghai:20140609T120000 DTEND;TZID=Asia/Shanghai:20140609T130000 LAST-MODIFIED:20140524T192046Z LOCATION:DoA, Rm 2907 SUMMARY:Low luminosity GRBs: A different class, shock breakout and afterglow URL;TYPE=URI:/info/1025/4869.htm END:VEVENT BEGIN:VEVENT UID:4472@kiaa.pku.edu.cn DTSTAMP:20140520T104757Z CREATED:20140520T104757Z DESCRIPTION:Astronomical X-ray polarimetry: a new window about to open DTSTART;TZID=Asia/Shanghai:20140612T160000 DTEND;TZID=Asia/Shanghai:20140612T160000 LAST-MODIFIED:20140520T104757Z LOCATION:KIAA-PKU Auditorium SUMMARY:Astronomical X-ray polarimetry: a new window about to open URL;TYPE=URI:/info/1024/4472.htm END:VEVENT BEGIN:VEVENT UID:4864@kiaa.pku.edu.cn DTSTAMP:20140425T081818Z CREATED:20140425T081818Z DESCRIPTION:The effects of metallicity on the Galactic disk white dwarf population DTSTART;TZID=Asia/Shanghai:20140613T120000 DTEND;TZID=Asia/Shanghai:20140613T130000 LAST-MODIFIED:20140425T081818Z LOCATION:KIAA, 1st floor seminar room SUMMARY:The effects of metallicity on the Galactic disk white dwarf population URL;TYPE=URI:/info/1025/4864.htm END:VEVENT BEGIN:VEVENT UID:4694@kiaa.pku.edu.cn DTSTAMP:20140613T142911Z CREATED:20140613T142911Z DESCRIPTION:SDSSJ001153.08-064739.2, a cataclysmic variable with an evolved donor in the period gap DTSTART;TZID=Asia/Shanghai:20140617T120000 DTEND;TZID=Asia/Shanghai:20140617T120000 LAST-MODIFIED:20140613T142911Z LOCATION:KIAA-PKU SUMMARY:SDSSJ001153.08-064739.2, a cataclysmic variable with an evolved donor in the period gap URL;TYPE=URI:/info/1028/4694.htm END:VEVENT BEGIN:VEVENT UID:4469@kiaa.pku.edu.cn DTSTAMP:20140424T170041Z CREATED:20140424T170041Z DESCRIPTION:An Enterprise with Two Purposes: Measurement of Longitude in 17th and 18th Century China DTSTART;TZID=Asia/Shanghai:20140619T160000 DTEND;TZID=Asia/Shanghai:20140619T170000 LAST-MODIFIED:20140424T170041Z LOCATION:KIAA-PKU Auditorium SUMMARY:An Enterprise with Two Purposes: Measurement of Longitude in 17th and 18th Century China URL;TYPE=URI:/info/1024/4469.htm END:VEVENT BEGIN:VEVENT UID:4470@kiaa.pku.edu.cn DTSTAMP:20140424T170041Z CREATED:20140424T170041Z DESCRIPTION:An Enterprise with Two Purposes: Measurement of Longitude in 17th and 18th Century China DTSTART;TZID=Asia/Shanghai:20140619T160000 DTEND;TZID=Asia/Shanghai:20140619T170000 LAST-MODIFIED:20140424T170041Z LOCATION:KIAA-PKU Auditorium SUMMARY:An Enterprise with Two Purposes: Measurement of Longitude in 17th and 18th Century China URL;TYPE=URI:/info/1024/4470.htm END:VEVENT BEGIN:VEVENT UID:4868@kiaa.pku.edu.cn DTSTAMP:20140514T110602Z CREATED:20140514T110602Z DESCRIPTION:International Year of Light 2015, Public Naming of Exoplanets and IAU Office for Astronomy Outreach DTSTART;TZID=Asia/Shanghai:20140620T120000 DTEND;TZID=Asia/Shanghai:20140620T130000 LAST-MODIFIED:20140514T110602Z LOCATION:KIAA, 1st floor seminar room SUMMARY:International Year of Light 2015, Public Naming of Exoplanets and IAU Office for Astronomy Outreach URL;TYPE=URI:/info/1025/4868.htm END:VEVENT BEGIN:VEVENT UID:4695@kiaa.pku.edu.cn DTSTAMP:20140620T212726Z CREATED:20140620T212726Z DESCRIPTION:Resonant Clumping and Substructure in Galactic Discs DTSTART;TZID=Asia/Shanghai:20140624T120000 DTEND;TZID=Asia/Shanghai:20140624T130000 LAST-MODIFIED:20140620T212726Z LOCATION:KIAA-PKU SUMMARY:Resonant Clumping and Substructure in Galactic Discs URL;TYPE=URI:/info/1028/4695.htm END:VEVENT BEGIN:VEVENT UID:4473@kiaa.pku.edu.cn DTSTAMP:20140612T205205Z CREATED:20140612T205205Z DESCRIPTION:What can we learn from X-ray Spectroscopy? DTSTART;TZID=Asia/Shanghai:20140626T160000 DTEND;TZID=Asia/Shanghai:20140626T170000 LAST-MODIFIED:20140612T205205Z LOCATION:KIAA-PKU Auditorium SUMMARY:What can we learn from X-ray Spectroscopy? URL;TYPE=URI:/info/1024/4473.htm END:VEVENT BEGIN:VEVENT UID:4696@kiaa.pku.edu.cn DTSTAMP:20140624T132137Z CREATED:20140624T132137Z DESCRIPTION:Historical trends in LMC distance moduli: Publication bias or not? DTSTART;TZID=Asia/Shanghai:20140708T120000 DTEND;TZID=Asia/Shanghai:20140708T120000 LAST-MODIFIED:20140624T132137Z LOCATION:KIAA-PKU SUMMARY:Historical trends in LMC distance moduli: Publication bias or not? URL;TYPE=URI:/info/1028/4696.htm END:VEVENT BEGIN:VEVENT UID:4474@kiaa.pku.edu.cn DTSTAMP:20140707T101721Z CREATED:20140707T101721Z DESCRIPTION:The European-Chinese MESSIER satellite: lifting the veil on galaxy formation DTSTART;TZID=Asia/Shanghai:20140717T160000 DTEND;TZID=Asia/Shanghai:20140717T170000 LAST-MODIFIED:20140707T101721Z LOCATION:KIAA-PKU Auditorium SUMMARY:The European-Chinese MESSIER satellite: lifting the veil on galaxy formation URL;TYPE=URI:/info/1024/4474.htm END:VEVENT BEGIN:VEVENT UID:4697@kiaa.pku.edu.cn DTSTAMP:20140703T134030Z CREATED:20140703T134030Z DESCRIPTION:The XSL X-shooter Spectral Library project: a focus on carbon stars DTSTART;TZID=Asia/Shanghai:20140722T120000 DTEND;TZID=Asia/Shanghai:20140722T120000 LAST-MODIFIED:20140703T134030Z LOCATION:KIAA-PKU SUMMARY:The XSL X-shooter Spectral Library project: a focus on carbon stars URL;TYPE=URI:/info/1028/4697.htm END:VEVENT BEGIN:VEVENT UID:4471@kiaa.pku.edu.cn DTSTAMP:20140505T155416Z CREATED:20140505T155416Z DESCRIPTION:Asymmetries in Protoplanetary Transition Disks DTSTART;TZID=Asia/Shanghai:20140724T160000 DTEND;TZID=Asia/Shanghai:20140724T160000 LAST-MODIFIED:20140505T155416Z LOCATION:KIAA-PKU Auditorium SUMMARY:Asymmetries in Protoplanetary Transition Disks URL;TYPE=URI:/info/1024/4471.htm END:VEVENT BEGIN:VEVENT UID:4870@kiaa.pku.edu.cn DTSTAMP:20140526T150440Z CREATED:20140526T150440Z DESCRIPTION:The Galactic rotation curve DTSTART;TZID=Asia/Shanghai:20140808T120000 DTEND;TZID=Asia/Shanghai:20140808T120000 LAST-MODIFIED:20140526T150440Z LOCATION:KIAA, 1st floor seminar room SUMMARY:The Galactic rotation curve URL;TYPE=URI:/info/1025/4870.htm END:VEVENT BEGIN:VEVENT UID:4872@kiaa.pku.edu.cn DTSTAMP:20140721T073233Z CREATED:20140721T073233Z DESCRIPTION:Asteroseismology & Exoplanets: A Kepler Success Story DTSTART;TZID=Asia/Shanghai:20140815T120000 DTEND;TZID=Asia/Shanghai:20140815T130000 LAST-MODIFIED:20140721T073233Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Asteroseismology & Exoplanets: A Kepler Success Story URL;TYPE=URI:/info/1025/4872.htm END:VEVENT BEGIN:VEVENT UID:4875@kiaa.pku.edu.cn DTSTAMP:20140811T094756Z CREATED:20140811T094756Z DESCRIPTION:The Outskirts of Galaxies DTSTART;TZID=Asia/Shanghai:20140819T120000 DTEND;TZID=Asia/Shanghai:20140819T130000 LAST-MODIFIED:20140811T094756Z LOCATION:KIAA, 1s floor seminar room SUMMARY:The Outskirts of Galaxies URL;TYPE=URI:/info/1025/4875.htm END:VEVENT BEGIN:VEVENT UID:4871@kiaa.pku.edu.cn DTSTAMP:20140617T195451Z CREATED:20140617T195451Z DESCRIPTION:Do GMCs care about their environment? DTSTART;TZID=Asia/Shanghai:20140822T120000 DTEND;TZID=Asia/Shanghai:20140822T130000 LAST-MODIFIED:20140617T195451Z LOCATION:KIAA, 1st floor seminar room SUMMARY:Do GMCs care about their environment? URL;TYPE=URI:/info/1025/4871.htm END:VEVENT BEGIN:VEVENT UID:5155@kiaa.pku.edu.cn DTSTAMP:20140320T223140Z CREATED:20140320T223140Z DESCRIPTION:IAU Symposium 312 DTSTART;TZID=Asia/Shanghai:20140825T093000 DTEND;TZID=Asia/Shanghai:20140829T173000 LAST-MODIFIED:20140320T223140Z LOCATION:Beijing, China SUMMARY:IAU Symposium 312 URL;TYPE=URI:/info/1026/5155.htm END:VEVENT BEGIN:VEVENT UID:4861@kiaa.pku.edu.cn DTSTAMP:20140410T115435Z CREATED:20140410T115435Z DESCRIPTION:Surveying the Evolution of Galaxies and Structure Formation with the Square Kilometre Array DTSTART;TZID=Asia/Shanghai:20140825T120000 DTEND;TZID=Asia/Shanghai:20140825T130000 LAST-MODIFIED:20140410T115435Z LOCATION:DoA, Rm 2907 SUMMARY:Surveying the Evolution of Galaxies and Structure Formation with the Square Kilometre Array URL;TYPE=URI:/info/1025/4861.htm END:VEVENT BEGIN:VEVENT UID:4476@kiaa.pku.edu.cn DTSTAMP:20140711T132457Z CREATED:20140711T132457Z DESCRIPTION:Pulsars, gravitational waves, clocks, planets, spacecraft and black holes DTSTART;TZID=Asia/Shanghai:20140828T160000 DTEND;TZID=Asia/Shanghai:20140828T170000 LAST-MODIFIED:20140711T132457Z LOCATION:KIAA-PKU Auditorium SUMMARY:Pulsars, gravitational waves, clocks, planets, spacecraft and black holes URL;TYPE=URI:/info/1024/4476.htm END:VEVENT BEGIN:VEVENT UID:5154@kiaa.pku.edu.cn DTSTAMP:20140320T222643Z CREATED:20140320T222643Z DESCRIPTION:Binary systems, their evolution and environments DTSTART;TZID=Asia/Shanghai:20140901T093000 DTEND;TZID=Asia/Shanghai:20140905T173000 LAST-MODIFIED:20140320T222643Z LOCATION:Ulaan Baatar, Mongolia SUMMARY:Binary systems, their evolution and environments URL;TYPE=URI:/info/1026/5154.htm END:VEVENT BEGIN:VEVENT UID:4876@kiaa.pku.edu.cn DTSTAMP:20140822T133921Z CREATED:20140822T133921Z DESCRIPTION:One Theoretical Investigation of GRB Host Galaxies DTSTART;TZID=Asia/Shanghai:20140901T120000 DTEND;TZID=Asia/Shanghai:20140901T130000 LAST-MODIFIED:20140822T133921Z LOCATION:DoA, Rm 2907 SUMMARY:One Theoretical Investigation of GRB Host Galaxies URL;TYPE=URI:/info/1025/4876.htm END:VEVENT BEGIN:VEVENT UID:4873@kiaa.pku.edu.cn DTSTAMP:20140807T163753Z CREATED:20140807T163753Z DESCRIPTION:RR Lyrae Stars, Cosmic Light Houses with a twist DTSTART;TZID=Asia/Shanghai:20140909T120000 DTEND;TZID=Asia/Shanghai:20140909T130000 LAST-MODIFIED:20140807T163753Z LOCATION:Kavli Institute for Astronomy and Astrophysics Meeting room, 1st floor SUMMARY:RR Lyrae Stars, Cosmic Light Houses with a twist URL;TYPE=URI:/info/1025/4873.htm END:VEVENT BEGIN:VEVENT UID:4480@kiaa.pku.edu.cn DTSTAMP:20140818T155949Z CREATED:20140818T155949Z DESCRIPTION:Hunting for the first stars DTSTART;TZID=Asia/Shanghai:20140911T160000 DTEND;TZID=Asia/Shanghai:20140911T170000 LAST-MODIFIED:20140818T155949Z LOCATION:KIAA-PKU Auditorium SUMMARY:Hunting for the first stars URL;TYPE=URI:/info/1024/4480.htm END:VEVENT BEGIN:VEVENT UID:4482@kiaa.pku.edu.cn DTSTAMP:20140828T105633Z CREATED:20140828T105633Z DESCRIPTION:CANDELS Greatest Hits DTSTART;TZID=Asia/Shanghai:20140918T160000 DTEND;TZID=Asia/Shanghai:20140918T160000 LAST-MODIFIED:20140828T105633Z LOCATION:KIAA-PKU Auditorium SUMMARY:CANDELS Greatest Hits URL;TYPE=URI:/info/1024/4482.htm END:VEVENT BEGIN:VEVENT UID:4483@kiaa.pku.edu.cn DTSTAMP:20140828T110714Z CREATED:20140828T110714Z DESCRIPTION:Neutrinos as a Cosmic Messenger DTSTART;TZID=Asia/Shanghai:20140925T160000 DTEND;TZID=Asia/Shanghai:20140925T160000 LAST-MODIFIED:20140828T110714Z LOCATION:KIAA-PKU Auditorium SUMMARY:Neutrinos as a Cosmic Messenger URL;TYPE=URI:/info/1024/4483.htm END:VEVENT BEGIN:VEVENT UID:4874@kiaa.pku.edu.cn DTSTAMP:20140807T170450Z CREATED:20140807T170450Z DESCRIPTION:Globular cluster systems in extreme environments DTSTART;TZID=Asia/Shanghai:20140929T120000 DTEND;TZID=Asia/Shanghai:20140929T130000 LAST-MODIFIED:20140807T170450Z LOCATION:DoA, Rm 2907 SUMMARY:Globular cluster systems in extreme environments URL;TYPE=URI:/info/1025/4874.htm END:VEVENT BEGIN:VEVENT UID:4699@kiaa.pku.edu.cn DTSTAMP:20141212T144354Z CREATED:20141212T144354Z DESCRIPTION:Constrain the mass/radius of neutron stars in Low mass x-ray binary DTSTART;TZID=Asia/Shanghai:20140930T120000 DTEND;TZID=Asia/Shanghai:20140930T124500 LAST-MODIFIED:20141212T144354Z LOCATION:KIAA-PKU SUMMARY:Constrain the mass/radius of neutron stars in Low mass x-ray binary URL;TYPE=URI:/info/1028/4699.htm END:VEVENT BEGIN:VEVENT UID:4481@kiaa.pku.edu.cn DTSTAMP:20140821T105004Z CREATED:20140821T105004Z DESCRIPTION:The gaseous features of the Magellanic System DTSTART;TZID=Asia/Shanghai:20141009T160000 DTEND;TZID=Asia/Shanghai:20141009T160000 LAST-MODIFIED:20140821T105004Z LOCATION:KIAA-PKU Auditorium SUMMARY:The gaseous features of the Magellanic System URL;TYPE=URI:/info/1024/4481.htm END:VEVENT BEGIN:VEVENT UID:4877@kiaa.pku.edu.cn DTSTAMP:20140915T101614Z CREATED:20140915T101614Z DESCRIPTION:Probing theories of gravity in the Galactic Centre DTSTART;TZID=Asia/Shanghai:20141013T120000 DTEND;TZID=Asia/Shanghai:20141013T120000 LAST-MODIFIED:20140915T101614Z LOCATION:DoA, Rm 2907 SUMMARY:Probing theories of gravity in the Galactic Centre URL;TYPE=URI:/info/1025/4877.htm END:VEVENT BEGIN:VEVENT UID:4780@kiaa.pku.edu.cn DTSTAMP:20141016T201538Z CREATED:20141016T201538Z DESCRIPTION:Significant age range in massive star cluster excluded by tight sub-giant-branch morphology DTSTART;TZID=Asia/Shanghai:20141013T170000 DTEND;TZID=Asia/Shanghai:20141013T180000 LAST-MODIFIED:20141016T201538Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Significant age range in massive star cluster excluded by tight sub-giant-branch morphology URL;TYPE=URI:/info/1029/4780.htm END:VEVENT BEGIN:VEVENT UID:4698@kiaa.pku.edu.cn DTSTAMP:20141010T122708Z CREATED:20141010T122708Z DESCRIPTION:Aiming for the next bright earth — Synergies of Ground and Space based Transiting Planets Survey DTSTART;TZID=Asia/Shanghai:20141014T120000 DTEND;TZID=Asia/Shanghai:20141014T130000 LAST-MODIFIED:20141010T122708Z LOCATION:KIAA-PKU SUMMARY:Aiming for the next bright earth — Synergies of Ground and Space based Transiting Planets Survey URL;TYPE=URI:/info/1028/4698.htm END:VEVENT BEGIN:VEVENT UID:4475@kiaa.pku.edu.cn DTSTAMP:20140709T152104Z CREATED:20140709T152104Z DESCRIPTION:The Future of Optical Astronomy: from Photons to Petabytes DTSTART;TZID=Asia/Shanghai:20141016T160000 DTEND;TZID=Asia/Shanghai:20141016T160000 LAST-MODIFIED:20140709T152104Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Future of Optical Astronomy: from Photons to Petabytes URL;TYPE=URI:/info/1024/4475.htm END:VEVENT BEGIN:VEVENT UID:4878@kiaa.pku.edu.cn DTSTAMP:20141002T152739Z CREATED:20141002T152739Z DESCRIPTION:BCGs and cluster galaxy populations across cosmic time DTSTART;TZID=Asia/Shanghai:20141017T120000 DTEND;TZID=Asia/Shanghai:20141017T130000 LAST-MODIFIED:20141002T152739Z LOCATION:KIAA-PKU Meeting room, 1st floor SUMMARY:BCGs and cluster galaxy populations across cosmic time URL;TYPE=URI:/info/1025/4878.htm END:VEVENT BEGIN:VEVENT UID:5153@kiaa.pku.edu.cn DTSTAMP:20140320T213134Z CREATED:20140320T213134Z DESCRIPTION:Quarks and Compact Stars 2014 DTSTART;TZID=Asia/Shanghai:20141020T093000 DTEND;TZID=Asia/Shanghai:20141022T173000 LAST-MODIFIED:20140320T213134Z LOCATION:KIAA-PKU SUMMARY:Quarks and Compact Stars 2014 URL;TYPE=URI:/info/1026/5153.htm END:VEVENT BEGIN:VEVENT UID:4782@kiaa.pku.edu.cn DTSTAMP:20141017T164939Z CREATED:20141017T164939Z DESCRIPTION:Probe the evolution history of planet with high precision Kepler light curves DTSTART;TZID=Asia/Shanghai:20141020T170000 DTEND;TZID=Asia/Shanghai:20141020T180000 LAST-MODIFIED:20141017T164939Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Probe the evolution history of planet with high precision Kepler light curves URL;TYPE=URI:/info/1029/4782.htm END:VEVENT BEGIN:VEVENT UID:6666@kiaa.pku.edu.cn DTSTAMP:20141016T120424Z CREATED:20141016T120424Z DESCRIPTION:Postdoc Science Day DTSTART;TZID=Asia/Shanghai:20141023T093000 DTEND;TZID=Asia/Shanghai:20141023T180000 LAST-MODIFIED:20141016T120424Z LOCATION:KIAA Auditorium SUMMARY:Postdoc Science Day URL;TYPE=URI:/info/1089/6666.htm END:VEVENT BEGIN:VEVENT UID:5164@kiaa.pku.edu.cn DTSTAMP:20150302T095945Z CREATED:20150302T095945Z DESCRIPTION:KIAA/DoA 2014 Postdoc Science Day DTSTART;TZID=Asia/Shanghai:20141023T093000 DTEND;TZID=Asia/Shanghai:20141023T180000 LAST-MODIFIED:20150302T095945Z LOCATION:KIAA-PKU Auditorium SUMMARY:KIAA/DoA 2014 Postdoc Science Day URL;TYPE=URI:/info/1026/5164.htm END:VEVENT BEGIN:VEVENT UID:5156@kiaa.pku.edu.cn DTSTAMP:20140722T231039Z CREATED:20140722T231039Z DESCRIPTION:2014 KIAA-PKU Astrophysics Forum DTSTART;TZID=Asia/Shanghai:20141102T080000 DTEND;TZID=Asia/Shanghai:20141104T080000 LAST-MODIFIED:20140722T231039Z LOCATION:KIAA-PKU, Beijing, China SUMMARY:2014 KIAA-PKU Astrophysics Forum URL;TYPE=URI:/info/1026/5156.htm END:VEVENT BEGIN:VEVENT UID:4881@kiaa.pku.edu.cn DTSTAMP:20141024T150627Z CREATED:20141024T150627Z DESCRIPTION:Both a possible evidence for existence of the magnetic monopole and Failure of the black hole model of the GC DTSTART;TZID=Asia/Shanghai:20141105T120000 DTEND;TZID=Asia/Shanghai:20141105T130000 LAST-MODIFIED:20141024T150627Z LOCATION:KIAA-PKU, Meeting Room, First Floor SUMMARY:Both a possible evidence for existence of the magnetic monopole and Failure of the black hole model of the GC URL;TYPE=URI:/info/1025/4881.htm END:VEVENT BEGIN:VEVENT UID:4478@kiaa.pku.edu.cn DTSTAMP:20140803T175407Z CREATED:20140803T175407Z DESCRIPTION:A Parallel AMR Method for Binary Black Hole Simulation DTSTART;TZID=Asia/Shanghai:20141106T160000 DTEND;TZID=Asia/Shanghai:20141106T160000 LAST-MODIFIED:20140803T175407Z LOCATION:KIAA-PKU Auditorium SUMMARY:A Parallel AMR Method for Binary Black Hole Simulation URL;TYPE=URI:/info/1024/4478.htm END:VEVENT BEGIN:VEVENT UID:4783@kiaa.pku.edu.cn DTSTAMP:20141018T103933Z CREATED:20141018T103933Z DESCRIPTION:The large scale structure around HzRG with GMRT and Herschel SPIRE data DTSTART;TZID=Asia/Shanghai:20141110T170000 DTEND;TZID=Asia/Shanghai:20141110T180000 LAST-MODIFIED:20141018T103933Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The large scale structure around HzRG with GMRT and Herschel SPIRE data URL;TYPE=URI:/info/1029/4783.htm END:VEVENT BEGIN:VEVENT UID:4879@kiaa.pku.edu.cn DTSTAMP:20141005T124616Z CREATED:20141005T124616Z DESCRIPTION:The Milky Way’s gravitational potential DTSTART;TZID=Asia/Shanghai:20141112T120000 DTEND;TZID=Asia/Shanghai:20141112T130000 LAST-MODIFIED:20141005T124616Z LOCATION:Kavli Institute for Astronomy and Astrophysics Meeting room, 1st floor SUMMARY:The Milky Way’s gravitational potential URL;TYPE=URI:/info/1025/4879.htm END:VEVENT BEGIN:VEVENT UID:4880@kiaa.pku.edu.cn DTSTAMP:20141023T115055Z CREATED:20141023T115055Z DESCRIPTION:AGN Jets and Lobes in Galaxy Clusters — Constraints on the Jet Properties and Their Feedback DTSTART;TZID=Asia/Shanghai:20141114T120000 DTEND;TZID=Asia/Shanghai:20141114T130000 LAST-MODIFIED:20141023T115055Z LOCATION:KIAA First Floor Meeting Room SUMMARY:AGN Jets and Lobes in Galaxy Clusters — Constraints on the Jet Properties and Their Feedback URL;TYPE=URI:/info/1025/4880.htm END:VEVENT BEGIN:VEVENT UID:5158@kiaa.pku.edu.cn DTSTAMP:20140923T163903Z CREATED:20140923T163903Z DESCRIPTION:CHILI "Cook-off" Meeting DTSTART;TZID=Asia/Shanghai:20141115T090000 DTEND;TZID=Asia/Shanghai:20141115T090000 LAST-MODIFIED:20140923T163903Z LOCATION:KIAA-PKU SUMMARY:CHILI "Cook-off" Meeting URL;TYPE=URI:/info/1026/5158.htm END:VEVENT BEGIN:VEVENT UID:6667@kiaa.pku.edu.cn DTSTAMP:20141113T113151Z CREATED:20141113T113151Z DESCRIPTION:NBODY2014 training workshop on gravitational N-body simulations DTSTART;TZID=Asia/Shanghai:20141115T100000 DTEND;TZID=Asia/Shanghai:20141123T170000 LAST-MODIFIED:20141113T113151Z LOCATION:KIAA-PKU SUMMARY:NBODY2014 training workshop on gravitational N-body simulations URL;TYPE=URI:/info/1089/6667.htm END:VEVENT BEGIN:VEVENT UID:4484@kiaa.pku.edu.cn DTSTAMP:20140921T172345Z CREATED:20140921T172345Z DESCRIPTION:MaNGA: Mapping Nearby Galaxies at Apache Point Observatory -- An IFU Survey of 10,000 Galaxies DTSTART;TZID=Asia/Shanghai:20141117T160000 DTEND;TZID=Asia/Shanghai:20141117T160000 LAST-MODIFIED:20140921T172345Z LOCATION:KIAA-PKU Auditorium SUMMARY:MaNGA: Mapping Nearby Galaxies at Apache Point Observatory -- An IFU Survey of 10,000 Galaxies URL;TYPE=URI:/info/1024/4484.htm END:VEVENT BEGIN:VEVENT UID:4781@kiaa.pku.edu.cn DTSTAMP:20141016T202101Z CREATED:20141016T202101Z DESCRIPTION:Study dark matter subhaloes with galaxy-galaxy lensing DTSTART;TZID=Asia/Shanghai:20141117T170000 DTEND;TZID=Asia/Shanghai:20141117T180000 LAST-MODIFIED:20141016T202101Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Study dark matter subhaloes with galaxy-galaxy lensing URL;TYPE=URI:/info/1029/4781.htm END:VEVENT BEGIN:VEVENT UID:4886@kiaa.pku.edu.cn DTSTAMP:20141104T103738Z CREATED:20141104T103738Z DESCRIPTION:MApping the Most Massive Overdensity Through Hydrogen (MAMMOTH) DTSTART;TZID=Asia/Shanghai:20141119T120000 DTEND;TZID=Asia/Shanghai:20141119T130000 LAST-MODIFIED:20141104T103738Z LOCATION:KIAA-PKU, Meeting Room, 1st Floor SUMMARY:MApping the Most Massive Overdensity Through Hydrogen (MAMMOTH) URL;TYPE=URI:/info/1025/4886.htm END:VEVENT BEGIN:VEVENT UID:4883@kiaa.pku.edu.cn DTSTAMP:20141031T093615Z CREATED:20141031T093615Z DESCRIPTION:Peering in to the Dark: Probing the Initial Conditions for the Formation of Stellar Clusters and Massive Stars DTSTART;TZID=Asia/Shanghai:20141120T120000 DTEND;TZID=Asia/Shanghai:20141120T130000 LAST-MODIFIED:20141031T093615Z LOCATION:KIAA-PKU Meeting room, 1st floor SUMMARY:Peering in to the Dark: Probing the Initial Conditions for the Formation of Stellar Clusters and Massive Stars URL;TYPE=URI:/info/1025/4883.htm END:VEVENT BEGIN:VEVENT UID:4503@kiaa.pku.edu.cn DTSTAMP:20141025T090933Z CREATED:20141025T090933Z DESCRIPTION:New constraints on the structure of galaxy clusters and cosmological parameters via stacked weak lensing and peak statistics DTSTART;TZID=Asia/Shanghai:20141120T160000 DTEND;TZID=Asia/Shanghai:20141120T160000 LAST-MODIFIED:20141025T090933Z LOCATION:KIAA-PKU Auditorium SUMMARY:New constraints on the structure of galaxy clusters and cosmological parameters via stacked weak lensing and peak statistics URL;TYPE=URI:/info/1024/4503.htm END:VEVENT BEGIN:VEVENT UID:4882@kiaa.pku.edu.cn DTSTAMP:20141030T083830Z CREATED:20141030T083830Z DESCRIPTION:Circum-galactic Medium Around Local Spiral Galaxies --- A New Window to Understand Galaxy Evolution DTSTART;TZID=Asia/Shanghai:20141121T120000 DTEND;TZID=Asia/Shanghai:20141121T130000 LAST-MODIFIED:20141030T083830Z LOCATION:KIAA-PKU, Meeting room, 1st floor SUMMARY:Circum-galactic Medium Around Local Spiral Galaxies --- A New Window to Understand Galaxy Evolution URL;TYPE=URI:/info/1025/4882.htm END:VEVENT BEGIN:VEVENT UID:4502@kiaa.pku.edu.cn DTSTAMP:20141022T115558Z CREATED:20141022T115558Z DESCRIPTION:Mid-Infrared Selected Dust-Rich Quasars: Recovering the Extended Quasar Population DTSTART;TZID=Asia/Shanghai:20141127T160000 DTEND;TZID=Asia/Shanghai:20141127T160000 LAST-MODIFIED:20141022T115558Z LOCATION:KIAA-PKU Auditorium SUMMARY:Mid-Infrared Selected Dust-Rich Quasars: Recovering the Extended Quasar Population URL;TYPE=URI:/info/1024/4502.htm END:VEVENT BEGIN:VEVENT UID:4888@kiaa.pku.edu.cn DTSTAMP:20141121T161608Z CREATED:20141121T161608Z DESCRIPTION:How Long does a Burst Burst? DTSTART;TZID=Asia/Shanghai:20141201T120000 DTEND;TZID=Asia/Shanghai:20141201T130000 LAST-MODIFIED:20141121T161608Z LOCATION:DoA, Rm 2907 SUMMARY:How Long does a Burst Burst? URL;TYPE=URI:/info/1025/4888.htm END:VEVENT BEGIN:VEVENT UID:4784@kiaa.pku.edu.cn DTSTAMP:20141120T165043Z CREATED:20141120T165043Z DESCRIPTION:Technical perspectives for computational astrophysics DTSTART;TZID=Asia/Shanghai:20141201T170000 DTEND;TZID=Asia/Shanghai:20141201T180000 LAST-MODIFIED:20141120T165043Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Technical perspectives for computational astrophysics URL;TYPE=URI:/info/1029/4784.htm END:VEVENT BEGIN:VEVENT UID:4700@kiaa.pku.edu.cn DTSTAMP:20141212T144545Z CREATED:20141212T144545Z DESCRIPTION:The search for longitude: Preliminary insights from a 17th Century Dutch perspective DTSTART;TZID=Asia/Shanghai:20141202T120000 DTEND;TZID=Asia/Shanghai:20141202T124500 LAST-MODIFIED:20141212T144545Z LOCATION:KIAA-PKU SUMMARY:The search for longitude: Preliminary insights from a 17th Century Dutch perspective URL;TYPE=URI:/info/1028/4700.htm END:VEVENT BEGIN:VEVENT UID:4485@kiaa.pku.edu.cn DTSTAMP:20141013T105400Z CREATED:20141013T105400Z DESCRIPTION:Star formation quenching in low-redshift galaxies DTSTART;TZID=Asia/Shanghai:20141204T160000 DTEND;TZID=Asia/Shanghai:20141204T160000 LAST-MODIFIED:20141013T105400Z LOCATION:KIAA-PKU Auditorium SUMMARY:Star formation quenching in low-redshift galaxies URL;TYPE=URI:/info/1024/4485.htm END:VEVENT BEGIN:VEVENT UID:4890@kiaa.pku.edu.cn DTSTAMP:20141130T210201Z CREATED:20141130T210201Z DESCRIPTION:San Pedro Martir UBVRI photometric survey of stellar clusters and associations DTSTART;TZID=Asia/Shanghai:20141205T120000 DTEND;TZID=Asia/Shanghai:20141205T130000 LAST-MODIFIED:20141130T210201Z LOCATION:KIAA, First floor meeting room SUMMARY:San Pedro Martir UBVRI photometric survey of stellar clusters and associations URL;TYPE=URI:/info/1025/4890.htm END:VEVENT BEGIN:VEVENT UID:4701@kiaa.pku.edu.cn DTSTAMP:20141212T144639Z CREATED:20141212T144639Z DESCRIPTION:Testing the Kerr Metric of the Massive black hole in the galactic center using stellar orbital motion. DTSTART;TZID=Asia/Shanghai:20141209T120000 DTEND;TZID=Asia/Shanghai:20141209T124500 LAST-MODIFIED:20141212T144639Z LOCATION:KIAA-PKU SUMMARY:Testing the Kerr Metric of the Massive black hole in the galactic center using stellar orbital motion. URL;TYPE=URI:/info/1028/4701.htm END:VEVENT BEGIN:VEVENT UID:4505@kiaa.pku.edu.cn DTSTAMP:20141203T232115Z CREATED:20141203T232115Z DESCRIPTION:Pulsar timing technique and its applications in gravitational experiments DTSTART;TZID=Asia/Shanghai:20141211T160000 DTEND;TZID=Asia/Shanghai:20141211T160000 LAST-MODIFIED:20141203T232115Z LOCATION:KIAA-PKU Auditorium SUMMARY:Pulsar timing technique and its applications in gravitational experiments URL;TYPE=URI:/info/1024/4505.htm END:VEVENT BEGIN:VEVENT UID:4884@kiaa.pku.edu.cn DTSTAMP:20141103T105729Z CREATED:20141103T105729Z DESCRIPTION:Understanding the evolution of disk galaxies through the bars DTSTART;TZID=Asia/Shanghai:20141212T120000 DTEND;TZID=Asia/Shanghai:20141212T130000 LAST-MODIFIED:20141103T105729Z LOCATION:KIAA, First Floor Meeting Room SUMMARY:Understanding the evolution of disk galaxies through the bars URL;TYPE=URI:/info/1025/4884.htm END:VEVENT BEGIN:VEVENT UID:4885@kiaa.pku.edu.cn DTSTAMP:20141103T105815Z CREATED:20141103T105815Z DESCRIPTION:Observational Evidence for the Coevolution between Supermassive Black Holes and Host Galaxies DTSTART;TZID=Asia/Shanghai:20141215T120000 DTEND;TZID=Asia/Shanghai:20141215T130000 LAST-MODIFIED:20141103T105815Z LOCATION:DoA, Rm 2907 SUMMARY:Observational Evidence for the Coevolution between Supermassive Black Holes and Host Galaxies URL;TYPE=URI:/info/1025/4885.htm END:VEVENT BEGIN:VEVENT UID:4506@kiaa.pku.edu.cn DTSTAMP:20141213T233726Z CREATED:20141213T233726Z DESCRIPTION:From Galaxies to Halos - Reverse Engineering of the Galaxy Population DTSTART;TZID=Asia/Shanghai:20141216T160000 DTEND;TZID=Asia/Shanghai:20141216T160000 LAST-MODIFIED:20141213T233726Z LOCATION:KIAA-PKU Auditorium SUMMARY:From Galaxies to Halos - Reverse Engineering of the Galaxy Population URL;TYPE=URI:/info/1024/4506.htm END:VEVENT BEGIN:VEVENT UID:4504@kiaa.pku.edu.cn DTSTAMP:20141111T104237Z CREATED:20141111T104237Z DESCRIPTION:Ubiquity of planets and diversity of planetary systems: Origin and Destiny of multiple super Earths and gas giants DTSTART;TZID=Asia/Shanghai:20141217T160000 DTEND;TZID=Asia/Shanghai:20141217T160000 LAST-MODIFIED:20141111T104237Z LOCATION:KIAA-PKU Auditorium SUMMARY:Ubiquity of planets and diversity of planetary systems: Origin and Destiny of multiple super Earths and gas giants URL;TYPE=URI:/info/1024/4504.htm END:VEVENT BEGIN:VEVENT UID:4477@kiaa.pku.edu.cn DTSTAMP:20140803T014550Z CREATED:20140803T014550Z DESCRIPTION:A close-up of the nearest supermasive black hole --- Sgr A* DTSTART;TZID=Asia/Shanghai:20141218T160000 DTEND;TZID=Asia/Shanghai:20141218T160000 LAST-MODIFIED:20140803T014550Z LOCATION:KIAA-PKU Auditorium SUMMARY:A close-up of the nearest supermasive black hole --- Sgr A* URL;TYPE=URI:/info/1024/4477.htm END:VEVENT BEGIN:VEVENT UID:4702@kiaa.pku.edu.cn DTSTAMP:20141212T144756Z CREATED:20141212T144756Z DESCRIPTION:Prestellar Core Formation, Evolution, and Accretion DTSTART;TZID=Asia/Shanghai:20141219T120000 DTEND;TZID=Asia/Shanghai:20141219T124500 LAST-MODIFIED:20141212T144756Z LOCATION:KIAA-PKU SUMMARY:Prestellar Core Formation, Evolution, and Accretion URL;TYPE=URI:/info/1028/4702.htm END:VEVENT BEGIN:VEVENT UID:4889@kiaa.pku.edu.cn DTSTAMP:20141126T101623Z CREATED:20141126T101623Z DESCRIPTION:Unveiling the Massive Stars in the Galactic Centre DTSTART;TZID=Asia/Shanghai:20141222T120000 DTEND;TZID=Asia/Shanghai:20141222T130000 LAST-MODIFIED:20141126T101623Z LOCATION:DoA, Rm 2907 SUMMARY:Unveiling the Massive Stars in the Galactic Centre URL;TYPE=URI:/info/1025/4889.htm END:VEVENT BEGIN:VEVENT UID:4785@kiaa.pku.edu.cn DTSTAMP:20141219T161834Z CREATED:20141219T161834Z DESCRIPTION:Prestellar core formation, evolution and accretion DTSTART;TZID=Asia/Shanghai:20141222T170000 DTEND;TZID=Asia/Shanghai:20141222T180000 LAST-MODIFIED:20141219T161834Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Prestellar core formation, evolution and accretion URL;TYPE=URI:/info/1029/4785.htm END:VEVENT BEGIN:VEVENT UID:4703@kiaa.pku.edu.cn DTSTAMP:20141212T144943Z CREATED:20141212T144943Z DESCRIPTION:Herschel study of high-z weak line quasars DTSTART;TZID=Asia/Shanghai:20141223T120000 DTEND;TZID=Asia/Shanghai:20141223T124500 LAST-MODIFIED:20141212T144943Z LOCATION:KIAA-PKU SUMMARY:Herschel study of high-z weak line quasars URL;TYPE=URI:/info/1028/4703.htm END:VEVENT BEGIN:VEVENT UID:4887@kiaa.pku.edu.cn DTSTAMP:20141113T130049Z CREATED:20141113T130049Z DESCRIPTION:Large European Array of Pulsars DTSTART;TZID=Asia/Shanghai:20150105T120000 DTEND;TZID=Asia/Shanghai:20150105T130000 LAST-MODIFIED:20141113T130049Z LOCATION:DoA, Rm 2907 SUMMARY:Large European Array of Pulsars URL;TYPE=URI:/info/1025/4887.htm END:VEVENT BEGIN:VEVENT UID:4479@kiaa.pku.edu.cn DTSTAMP:20140811T211454Z CREATED:20140811T211454Z DESCRIPTION:Architecture and Timing of Planetary Systems DTSTART;TZID=Asia/Shanghai:20150108T160000 DTEND;TZID=Asia/Shanghai:20150108T160000 LAST-MODIFIED:20140811T211454Z LOCATION:KIAA-PKU Auditorium SUMMARY:Architecture and Timing of Planetary Systems URL;TYPE=URI:/info/1024/4479.htm END:VEVENT BEGIN:VEVENT UID:4786@kiaa.pku.edu.cn DTSTAMP:20150110T170312Z CREATED:20150110T170312Z DESCRIPTION:ECLIPSING BINARIES FROM THE CSTAR PROJECT AT DOME A, ANTARCTICA DTSTART;TZID=Asia/Shanghai:20150112T170000 DTEND;TZID=Asia/Shanghai:20150112T180000 LAST-MODIFIED:20150110T170312Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:ECLIPSING BINARIES FROM THE CSTAR PROJECT AT DOME A, ANTARCTICA URL;TYPE=URI:/info/1029/4786.htm END:VEVENT BEGIN:VEVENT UID:4704@kiaa.pku.edu.cn DTSTAMP:20150105T093533Z CREATED:20150105T093533Z DESCRIPTION:Circumbinary Planets DTSTART;TZID=Asia/Shanghai:20150113T000000 DTEND;TZID=Asia/Shanghai:20150113T003000 LAST-MODIFIED:20150105T093533Z LOCATION:KIAA-PKU SUMMARY:Circumbinary Planets URL;TYPE=URI:/info/1028/4704.htm END:VEVENT BEGIN:VEVENT UID:4508@kiaa.pku.edu.cn DTSTAMP:20150105T165831Z CREATED:20150105T165831Z DESCRIPTION:Massive Galaxy Growth since Cosmic Noon DTSTART;TZID=Asia/Shanghai:20150114T160000 DTEND;TZID=Asia/Shanghai:20150114T160000 LAST-MODIFIED:20150105T165831Z LOCATION:KIAA-PKU Auditorium SUMMARY:Massive Galaxy Growth since Cosmic Noon URL;TYPE=URI:/info/1024/4508.htm END:VEVENT BEGIN:VEVENT UID:4487@kiaa.pku.edu.cn DTSTAMP:20141013T134335Z CREATED:20141013T134335Z DESCRIPTION:The Local Universe with High Resolution X-ray Imaging: From Galactic Massive Star Forming Regions to Nearby Active Galaxies DTSTART;TZID=Asia/Shanghai:20150115T160000 DTEND;TZID=Asia/Shanghai:20150115T160000 LAST-MODIFIED:20141013T134335Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Local Universe with High Resolution X-ray Imaging: From Galactic Massive Star Forming Regions to Nearby Active Galaxies URL;TYPE=URI:/info/1024/4487.htm END:VEVENT BEGIN:VEVENT UID:4891@kiaa.pku.edu.cn DTSTAMP:20150109T094031Z CREATED:20150109T094031Z DESCRIPTION:Local Analogs for High-redshift Galaxies: Resembling the Physical Conditions of Interstellar Medium in High-redshift Galaxies. DTSTART;TZID=Asia/Shanghai:20150116T120000 DTEND;TZID=Asia/Shanghai:20150116T130000 LAST-MODIFIED:20150109T094031Z LOCATION:1st floor meeting room, KIAA, PKU SUMMARY:Local Analogs for High-redshift Galaxies: Resembling the Physical Conditions of Interstellar Medium in High-redshift Galaxies. URL;TYPE=URI:/info/1025/4891.htm END:VEVENT BEGIN:VEVENT UID:4507@kiaa.pku.edu.cn DTSTAMP:20150105T152211Z CREATED:20150105T152211Z DESCRIPTION:Turbulence-induced collision velocity of dust particles DTSTART;TZID=Asia/Shanghai:20150119T160000 DTEND;TZID=Asia/Shanghai:20150119T160000 LAST-MODIFIED:20150105T152211Z LOCATION:KIAA-PKU Auditorium SUMMARY:Turbulence-induced collision velocity of dust particles URL;TYPE=URI:/info/1024/4507.htm END:VEVENT BEGIN:VEVENT UID:4787@kiaa.pku.edu.cn DTSTAMP:20150117T130613Z CREATED:20150117T130613Z DESCRIPTION:migration and growth of embryos in protoplanetary disks DTSTART;TZID=Asia/Shanghai:20150119T170000 DTEND;TZID=Asia/Shanghai:20150119T180000 LAST-MODIFIED:20150117T130613Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:migration and growth of embryos in protoplanetary disks URL;TYPE=URI:/info/1029/4787.htm END:VEVENT BEGIN:VEVENT UID:6670@kiaa.pku.edu.cn DTSTAMP:20150121T104853Z CREATED:20150121T104853Z DESCRIPTION:Beijing Exoplanet Focus Group (BEFG) Meeting DTSTART;TZID=Asia/Shanghai:20150121T100000 DTEND;TZID=Asia/Shanghai:20150121T120000 LAST-MODIFIED:20150121T104853Z LOCATION:KIAA-PKU, first floor seminar room SUMMARY:Beijing Exoplanet Focus Group (BEFG) Meeting URL;TYPE=URI:/info/1089/6670.htm END:VEVENT BEGIN:VEVENT UID:4509@kiaa.pku.edu.cn DTSTAMP:20150107T113915Z CREATED:20150107T113915Z DESCRIPTION:Galactic Tomography with the LAMOST and SDSS DTSTART;TZID=Asia/Shanghai:20150121T160000 DTEND;TZID=Asia/Shanghai:20150121T160000 LAST-MODIFIED:20150107T113915Z LOCATION:KIAA-PKU Auditorium SUMMARY:Galactic Tomography with the LAMOST and SDSS URL;TYPE=URI:/info/1024/4509.htm END:VEVENT BEGIN:VEVENT UID:4705@kiaa.pku.edu.cn DTSTAMP:20150120T142943Z CREATED:20150120T142943Z DESCRIPTION:Mars DTSTART;TZID=Asia/Shanghai:20150127T120000 DTEND;TZID=Asia/Shanghai:20150127T120000 LAST-MODIFIED:20150120T142943Z LOCATION:KIAA-PKU SUMMARY:Mars URL;TYPE=URI:/info/1028/4705.htm END:VEVENT BEGIN:VEVENT UID:4895@kiaa.pku.edu.cn DTSTAMP:20150129T223510Z CREATED:20150129T223510Z DESCRIPTION:Planet Formation Under Different Environments DTSTART;TZID=Asia/Shanghai:20150304T120000 DTEND;TZID=Asia/Shanghai:20150304T130000 LAST-MODIFIED:20150129T223510Z LOCATION:KIAA 1st floor meeting room SUMMARY:Planet Formation Under Different Environments URL;TYPE=URI:/info/1025/4895.htm END:VEVENT BEGIN:VEVENT UID:4514@kiaa.pku.edu.cn DTSTAMP:20150202T152228Z CREATED:20150202T152228Z DESCRIPTION:An Ultra-luminous Quasar with Most Massive Black Hole in the Distant Universe DTSTART;TZID=Asia/Shanghai:20150305T160000 DTEND;TZID=Asia/Shanghai:20150305T160000 LAST-MODIFIED:20150202T152228Z LOCATION:KIAA-PKU Auditorium SUMMARY:An Ultra-luminous Quasar with Most Massive Black Hole in the Distant Universe URL;TYPE=URI:/info/1024/4514.htm END:VEVENT BEGIN:VEVENT UID:4893@kiaa.pku.edu.cn DTSTAMP:20150116T141639Z CREATED:20150116T141639Z DESCRIPTION:Investigating the Physics of Hard X-­ray Outbursts from the Galactic Center Supermassive Black Hole Sagittarius A* with NuSTAR DTSTART;TZID=Asia/Shanghai:20150306T120000 DTEND;TZID=Asia/Shanghai:20150306T130000 LAST-MODIFIED:20150116T141639Z LOCATION:1st floor meeting room, KIAA, PKU SUMMARY:Investigating the Physics of Hard X-­ray Outbursts from the Galactic Center Supermassive Black Hole Sagittarius A* with NuSTAR URL;TYPE=URI:/info/1025/4893.htm END:VEVENT BEGIN:VEVENT UID:4892@kiaa.pku.edu.cn DTSTAMP:20150112T161618Z CREATED:20150112T161618Z DESCRIPTION:Testing Spacetime Symmetries with Radio Pulsars DTSTART;TZID=Asia/Shanghai:20150309T120000 DTEND;TZID=Asia/Shanghai:20150309T130000 LAST-MODIFIED:20150112T161618Z LOCATION:DoA, Rm 2907 SUMMARY:Testing Spacetime Symmetries with Radio Pulsars URL;TYPE=URI:/info/1025/4892.htm END:VEVENT BEGIN:VEVENT UID:4894@kiaa.pku.edu.cn DTSTAMP:20150126T111019Z CREATED:20150126T111019Z DESCRIPTION:The Physics of Gamma-ray Burst Prompt Emission and Afterglow DTSTART;TZID=Asia/Shanghai:20150311T120000 DTEND;TZID=Asia/Shanghai:20150311T130000 LAST-MODIFIED:20150126T111019Z LOCATION:KIAA first floor meeting room SUMMARY:The Physics of Gamma-ray Burst Prompt Emission and Afterglow URL;TYPE=URI:/info/1025/4894.htm END:VEVENT BEGIN:VEVENT UID:4515@kiaa.pku.edu.cn DTSTAMP:20150202T180041Z CREATED:20150202T180041Z DESCRIPTION:Star formation law of nearby galaxies DTSTART;TZID=Asia/Shanghai:20150312T160000 DTEND;TZID=Asia/Shanghai:20150312T160000 LAST-MODIFIED:20150202T180041Z LOCATION:KIAA-PKU Auditorium SUMMARY:Star formation law of nearby galaxies URL;TYPE=URI:/info/1024/4515.htm END:VEVENT BEGIN:VEVENT UID:5161@kiaa.pku.edu.cn DTSTAMP:20150202T150848Z CREATED:20150202T150848Z DESCRIPTION:Quasars and Active Galactic Nuclei over Cosmic Time DTSTART;TZID=Asia/Shanghai:20150316T090000 DTEND;TZID=Asia/Shanghai:20150320T170000 LAST-MODIFIED:20150202T150848Z LOCATION:KIAA-PKU SUMMARY:Quasars and Active Galactic Nuclei over Cosmic Time URL;TYPE=URI:/info/1026/5161.htm END:VEVENT BEGIN:VEVENT UID:4512@kiaa.pku.edu.cn DTSTAMP:20150115T213236Z CREATED:20150115T213236Z DESCRIPTION:What drives the Star Formation History of the Universe? DTSTART;TZID=Asia/Shanghai:20150319T160000 DTEND;TZID=Asia/Shanghai:20150319T160000 LAST-MODIFIED:20150115T213236Z LOCATION:KIAA-PKU Auditorium SUMMARY:What drives the Star Formation History of the Universe? URL;TYPE=URI:/info/1024/4512.htm END:VEVENT BEGIN:VEVENT UID:4486@kiaa.pku.edu.cn DTSTAMP:20141013T110624Z CREATED:20141013T110624Z DESCRIPTION:Characterizing Circumgalactic Gas with Absorption Spectroscopy DTSTART;TZID=Asia/Shanghai:20150326T160000 DTEND;TZID=Asia/Shanghai:20150326T160000 LAST-MODIFIED:20141013T110624Z LOCATION:KIAA-PKU Auditorium SUMMARY:Characterizing Circumgalactic Gas with Absorption Spectroscopy URL;TYPE=URI:/info/1024/4486.htm END:VEVENT BEGIN:VEVENT UID:4706@kiaa.pku.edu.cn DTSTAMP:20150323T090117Z CREATED:20150323T090117Z DESCRIPTION:Mining the SDSS spectroscopic archive DTSTART;TZID=Asia/Shanghai:20150327T120000 DTEND;TZID=Asia/Shanghai:20150327T130000 LAST-MODIFIED:20150323T090117Z LOCATION:KIAA-PKU SUMMARY:Mining the SDSS spectroscopic archive URL;TYPE=URI:/info/1028/4706.htm END:VEVENT BEGIN:VEVENT UID:6668@kiaa.pku.edu.cn DTSTAMP:20150105T120350Z CREATED:20150105T120350Z DESCRIPTION:KIAA SAC Visit DTSTART;TZID=Asia/Shanghai:20150328T090000 DTEND;TZID=Asia/Shanghai:20150329T170000 LAST-MODIFIED:20150105T120350Z LOCATION: SUMMARY:KIAA SAC Visit URL;TYPE=URI:/info/1089/6668.htm END:VEVENT BEGIN:VEVENT UID:4896@kiaa.pku.edu.cn DTSTAMP:20150311T085720Z CREATED:20150311T085720Z DESCRIPTION:Mega-maser Cosmology Project: Hubble Constant, M-σ relationship and Accretion Disks DTSTART;TZID=Asia/Shanghai:20150330T120000 DTEND;TZID=Asia/Shanghai:20150330T130000 LAST-MODIFIED:20150311T085720Z LOCATION:KIAA SUMMARY:Mega-maser Cosmology Project: Hubble Constant, M-σ relationship and Accretion Disks URL;TYPE=URI:/info/1025/4896.htm END:VEVENT BEGIN:VEVENT UID:4511@kiaa.pku.edu.cn DTSTAMP:20150113T161850Z CREATED:20150113T161850Z DESCRIPTION:Dark Matter Dynamics DTSTART;TZID=Asia/Shanghai:20150330T160000 DTEND;TZID=Asia/Shanghai:20150330T160000 LAST-MODIFIED:20150113T161850Z LOCATION:KIAA-PKU Auditorium SUMMARY:Dark Matter Dynamics URL;TYPE=URI:/info/1024/4511.htm END:VEVENT BEGIN:VEVENT UID:5163@kiaa.pku.edu.cn DTSTAMP:20150301T113641Z CREATED:20150301T113641Z DESCRIPTION:The 2015 Nanjing-Beijing Bilateral Astrophysics Workshop DTSTART;TZID=Asia/Shanghai:20150402T090000 DTEND;TZID=Asia/Shanghai:20150403T170000 LAST-MODIFIED:20150301T113641Z LOCATION:Nanjing University SUMMARY:The 2015 Nanjing-Beijing Bilateral Astrophysics Workshop URL;TYPE=URI:/info/1026/5163.htm END:VEVENT BEGIN:VEVENT UID:4513@kiaa.pku.edu.cn DTSTAMP:20150120T140328Z CREATED:20150120T140328Z DESCRIPTION:Millisecond pulsar binaries at transition DTSTART;TZID=Asia/Shanghai:20150409T160000 DTEND;TZID=Asia/Shanghai:20150409T160000 LAST-MODIFIED:20150120T140328Z LOCATION:KIAA-PKU Auditorium SUMMARY:Millisecond pulsar binaries at transition URL;TYPE=URI:/info/1024/4513.htm END:VEVENT BEGIN:VEVENT UID:4707@kiaa.pku.edu.cn DTSTAMP:20150330T112951Z CREATED:20150330T112951Z DESCRIPTION:Cosmic velocity field DTSTART;TZID=Asia/Shanghai:20150414T120000 DTEND;TZID=Asia/Shanghai:20150414T123000 LAST-MODIFIED:20150330T112951Z LOCATION:KIAA-PKU SUMMARY:Cosmic velocity field URL;TYPE=URI:/info/1028/4707.htm END:VEVENT BEGIN:VEVENT UID:4516@kiaa.pku.edu.cn DTSTAMP:20150302T104544Z CREATED:20150302T104544Z DESCRIPTION:Probing Planetary Formation at the Angular Resolution Frontier DTSTART;TZID=Asia/Shanghai:20150416T160000 DTEND;TZID=Asia/Shanghai:20150416T160000 LAST-MODIFIED:20150302T104544Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing Planetary Formation at the Angular Resolution Frontier URL;TYPE=URI:/info/1024/4516.htm END:VEVENT BEGIN:VEVENT UID:4899@kiaa.pku.edu.cn DTSTAMP:20150413T145501Z CREATED:20150413T145501Z DESCRIPTION:The Galactic Center as a unique laboratory for a new physics DTSTART;TZID=Asia/Shanghai:20150417T120000 DTEND;TZID=Asia/Shanghai:20150417T130000 LAST-MODIFIED:20150413T145501Z LOCATION:KIAA, 1st meeting room SUMMARY:The Galactic Center as a unique laboratory for a new physics URL;TYPE=URI:/info/1025/4899.htm END:VEVENT BEGIN:VEVENT UID:4522@kiaa.pku.edu.cn DTSTAMP:20150415T214424Z CREATED:20150415T214424Z DESCRIPTION:A Scheme for Star Formation — Molecules, Cores, Filaments, and Psychology DTSTART;TZID=Asia/Shanghai:20150423T160000 DTEND;TZID=Asia/Shanghai:20150423T160000 LAST-MODIFIED:20150415T214424Z LOCATION:KIAA-PKU Auditorium SUMMARY:A Scheme for Star Formation — Molecules, Cores, Filaments, and Psychology URL;TYPE=URI:/info/1024/4522.htm END:VEVENT BEGIN:VEVENT UID:4709@kiaa.pku.edu.cn DTSTAMP:20150426T115918Z CREATED:20150426T115918Z DESCRIPTION:From Cloud Cores to Protostars (Facts, Fiction, and Speculation) DTSTART;TZID=Asia/Shanghai:20150429T120000 DTEND;TZID=Asia/Shanghai:20150429T130000 LAST-MODIFIED:20150426T115918Z LOCATION:KIAA-PKU SUMMARY:From Cloud Cores to Protostars (Facts, Fiction, and Speculation) URL;TYPE=URI:/info/1028/4709.htm END:VEVENT BEGIN:VEVENT UID:4517@kiaa.pku.edu.cn DTSTAMP:20150303T104115Z CREATED:20150303T104115Z DESCRIPTION:The Evolution of Star-Forming Cores in Molecular Clouds: Using Theoretical Models to Inform Observations DTSTART;TZID=Asia/Shanghai:20150430T160000 DTEND;TZID=Asia/Shanghai:20150430T160000 LAST-MODIFIED:20150303T104115Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Evolution of Star-Forming Cores in Molecular Clouds: Using Theoretical Models to Inform Observations URL;TYPE=URI:/info/1024/4517.htm END:VEVENT BEGIN:VEVENT UID:4902@kiaa.pku.edu.cn DTSTAMP:20150504T183857Z CREATED:20150504T183857Z DESCRIPTION:Cosmological applications of pulsars: Gravitational waves and fast-radio bursts DTSTART;TZID=Asia/Shanghai:20150506T120000 DTEND;TZID=Asia/Shanghai:20150506T130000 LAST-MODIFIED:20150504T183857Z LOCATION:KIAA, first floor meeting room SUMMARY:Cosmological applications of pulsars: Gravitational waves and fast-radio bursts URL;TYPE=URI:/info/1025/4902.htm END:VEVENT BEGIN:VEVENT UID:4510@kiaa.pku.edu.cn DTSTAMP:20150107T163824Z CREATED:20150107T163824Z DESCRIPTION:The Lick Observatory Supernova Search with the Katzman Automatic Imaging Telescope DTSTART;TZID=Asia/Shanghai:20150507T160000 DTEND;TZID=Asia/Shanghai:20150507T160000 LAST-MODIFIED:20150107T163824Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Lick Observatory Supernova Search with the Katzman Automatic Imaging Telescope URL;TYPE=URI:/info/1024/4510.htm END:VEVENT BEGIN:VEVENT UID:4897@kiaa.pku.edu.cn DTSTAMP:20150320T104811Z CREATED:20150320T104811Z DESCRIPTION:Needles in a haystack of galaxies: searching for debris disks in wide area extragalactic surveys DTSTART;TZID=Asia/Shanghai:20150508T120000 DTEND;TZID=Asia/Shanghai:20150508T130000 LAST-MODIFIED:20150320T104811Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Needles in a haystack of galaxies: searching for debris disks in wide area extragalactic surveys URL;TYPE=URI:/info/1025/4897.htm END:VEVENT BEGIN:VEVENT UID:4901@kiaa.pku.edu.cn DTSTAMP:20150422T124611Z CREATED:20150422T124611Z DESCRIPTION:Influence of Perturbations on Pulsar Radio Emission DTSTART;TZID=Asia/Shanghai:20150511T120000 DTEND;TZID=Asia/Shanghai:20150511T130000 LAST-MODIFIED:20150422T124611Z LOCATION:DoA, Rm 2907 SUMMARY:Influence of Perturbations on Pulsar Radio Emission URL;TYPE=URI:/info/1025/4901.htm END:VEVENT BEGIN:VEVENT UID:4708@kiaa.pku.edu.cn DTSTAMP:20150420T114224Z CREATED:20150420T114224Z DESCRIPTION:The Efficiency of Galaxy Formation on the Smallest Scales: Lessons from Virgo DTSTART;TZID=Asia/Shanghai:20150512T120000 DTEND;TZID=Asia/Shanghai:20150512T123000 LAST-MODIFIED:20150420T114224Z LOCATION:KIAA-PKU (Pizza discussion) SUMMARY:The Efficiency of Galaxy Formation on the Smallest Scales: Lessons from Virgo URL;TYPE=URI:/info/1028/4708.htm END:VEVENT BEGIN:VEVENT UID:4898@kiaa.pku.edu.cn DTSTAMP:20150331T163540Z CREATED:20150331T163540Z DESCRIPTION:The Compton Spectrometer and Imager (COSI) Project DTSTART;TZID=Asia/Shanghai:20150513T120000 DTEND;TZID=Asia/Shanghai:20150513T130000 LAST-MODIFIED:20150331T163540Z LOCATION:KIAA first floor meeting room SUMMARY:The Compton Spectrometer and Imager (COSI) Project URL;TYPE=URI:/info/1025/4898.htm END:VEVENT BEGIN:VEVENT UID:4521@kiaa.pku.edu.cn DTSTAMP:20150413T095011Z CREATED:20150413T095011Z DESCRIPTION:Modeling galaxy formation and distribution DTSTART;TZID=Asia/Shanghai:20150514T160000 DTEND;TZID=Asia/Shanghai:20150514T160000 LAST-MODIFIED:20150413T095011Z LOCATION:KIAA-PKU Auditorium SUMMARY:Modeling galaxy formation and distribution URL;TYPE=URI:/info/1024/4521.htm END:VEVENT BEGIN:VEVENT UID:5159@kiaa.pku.edu.cn DTSTAMP:20150114T141358Z CREATED:20150114T141358Z DESCRIPTION:2015 KIAA-SHAO Bilateral Workshop DTSTART;TZID=Asia/Shanghai:20150518T090000 DTEND;TZID=Asia/Shanghai:20150519T190000 LAST-MODIFIED:20150114T141358Z LOCATION:KIAA-PKU SUMMARY:2015 KIAA-SHAO Bilateral Workshop URL;TYPE=URI:/info/1026/5159.htm END:VEVENT BEGIN:VEVENT UID:6669@kiaa.pku.edu.cn DTSTAMP:20150120T152918Z CREATED:20150120T152918Z DESCRIPTION:Probing Active Galactic Nuclei with Radio Techniques DTSTART;TZID=Asia/Shanghai:20150521T090000 DTEND;TZID=Asia/Shanghai:20150525T180000 LAST-MODIFIED:20150120T152918Z LOCATION:Yining, Xinjiang, China SUMMARY:Probing Active Galactic Nuclei with Radio Techniques URL;TYPE=URI:/info/1089/6669.htm END:VEVENT BEGIN:VEVENT UID:5162@kiaa.pku.edu.cn DTSTAMP:20150202T151425Z CREATED:20150202T151425Z DESCRIPTION:Probing Active Galactic Nuclei with Radio techniques DTSTART;TZID=Asia/Shanghai:20150521T090000 DTEND;TZID=Asia/Shanghai:20150525T170000 LAST-MODIFIED:20150202T151425Z LOCATION:Yining, Xinjiang, China SUMMARY:Probing Active Galactic Nuclei with Radio techniques URL;TYPE=URI:/info/1026/5162.htm END:VEVENT BEGIN:VEVENT UID:4523@kiaa.pku.edu.cn DTSTAMP:20150416T093806Z CREATED:20150416T093806Z DESCRIPTION:White dwarfs: intrinsic properties and applications DTSTART;TZID=Asia/Shanghai:20150521T160000 DTEND;TZID=Asia/Shanghai:20150521T160000 LAST-MODIFIED:20150416T093806Z LOCATION:KIAA-PKU Auditorium SUMMARY:White dwarfs: intrinsic properties and applications URL;TYPE=URI:/info/1024/4523.htm END:VEVENT BEGIN:VEVENT UID:4900@kiaa.pku.edu.cn DTSTAMP:20150416T144119Z CREATED:20150416T144119Z DESCRIPTION:How to get published in Nature Physics DTSTART;TZID=Asia/Shanghai:20150522T120000 DTEND;TZID=Asia/Shanghai:20150522T130000 LAST-MODIFIED:20150416T144119Z LOCATION:KIAA, 1st floor meeting room SUMMARY:How to get published in Nature Physics URL;TYPE=URI:/info/1025/4900.htm END:VEVENT BEGIN:VEVENT UID:4710@kiaa.pku.edu.cn DTSTAMP:20150518T090718Z CREATED:20150518T090718Z DESCRIPTION:Hyper-Suprime Camera Survey: Trailer and the First Year DTSTART;TZID=Asia/Shanghai:20150526T120000 DTEND;TZID=Asia/Shanghai:20150526T130000 LAST-MODIFIED:20150518T090718Z LOCATION:KIAA-PKU (Pizza discussion) SUMMARY:Hyper-Suprime Camera Survey: Trailer and the First Year URL;TYPE=URI:/info/1028/4710.htm END:VEVENT BEGIN:VEVENT UID:4518@kiaa.pku.edu.cn DTSTAMP:20150327T093405Z CREATED:20150327T093405Z DESCRIPTION:Direct Imaging Research of Exoplanet with Current Middle-sized Telescopes and Fututre Projects DTSTART;TZID=Asia/Shanghai:20150528T160000 DTEND;TZID=Asia/Shanghai:20150528T160000 LAST-MODIFIED:20150327T093405Z LOCATION:KIAA-PKU Auditorium SUMMARY:Direct Imaging Research of Exoplanet with Current Middle-sized Telescopes and Fututre Projects URL;TYPE=URI:/info/1024/4518.htm END:VEVENT BEGIN:VEVENT UID:4526@kiaa.pku.edu.cn DTSTAMP:20150512T105641Z CREATED:20150512T105641Z DESCRIPTION:Galaxy formation in the cosmological context DTSTART;TZID=Asia/Shanghai:20150604T160000 DTEND;TZID=Asia/Shanghai:20150604T160000 LAST-MODIFIED:20150512T105641Z LOCATION:KIAA-PKU Auditorium SUMMARY:Galaxy formation in the cosmological context URL;TYPE=URI:/info/1024/4526.htm END:VEVENT BEGIN:VEVENT UID:4519@kiaa.pku.edu.cn DTSTAMP:20150329T105849Z CREATED:20150329T105849Z DESCRIPTION:Numerical Simulations of Black Hole Accretion DTSTART;TZID=Asia/Shanghai:20150608T160000 DTEND;TZID=Asia/Shanghai:20150608T160000 LAST-MODIFIED:20150329T105849Z LOCATION:KIAA-PKU Auditorium SUMMARY:Numerical Simulations of Black Hole Accretion URL;TYPE=URI:/info/1024/4519.htm END:VEVENT BEGIN:VEVENT UID:4524@kiaa.pku.edu.cn DTSTAMP:20150506T162408Z CREATED:20150506T162408Z DESCRIPTION:Investigating [X/Fe], IMF and Compositeness in Integrated Models DTSTART;TZID=Asia/Shanghai:20150611T160000 DTEND;TZID=Asia/Shanghai:20150611T160000 LAST-MODIFIED:20150506T162408Z LOCATION:KIAA-PKU Auditorium SUMMARY:Investigating [X/Fe], IMF and Compositeness in Integrated Models URL;TYPE=URI:/info/1024/4524.htm END:VEVENT BEGIN:VEVENT UID:4711@kiaa.pku.edu.cn DTSTAMP:20150526T132008Z CREATED:20150526T132008Z DESCRIPTION:Escaping the explosion: understanding fast and slow runaways from type Ia supernovae DTSTART;TZID=Asia/Shanghai:20150616T120000 DTEND;TZID=Asia/Shanghai:20150616T130000 LAST-MODIFIED:20150526T132008Z LOCATION:KIAA-PKU (Pizza discussion) SUMMARY:Escaping the explosion: understanding fast and slow runaways from type Ia supernovae URL;TYPE=URI:/info/1028/4711.htm END:VEVENT BEGIN:VEVENT UID:4904@kiaa.pku.edu.cn DTSTAMP:20150613T221018Z CREATED:20150613T221018Z DESCRIPTION:Can life survive Gamma-Ray Bursts in high-redshift universe? DTSTART;TZID=Asia/Shanghai:20150617T120000 DTEND;TZID=Asia/Shanghai:20150617T130000 LAST-MODIFIED:20150613T221018Z LOCATION:KIAA, first floor meeting room SUMMARY:Can life survive Gamma-Ray Bursts in high-redshift universe? URL;TYPE=URI:/info/1025/4904.htm END:VEVENT BEGIN:VEVENT UID:4525@kiaa.pku.edu.cn DTSTAMP:20150507T093921Z CREATED:20150507T093921Z DESCRIPTION:High duty-cycle time-series photometric observations in multiple colors for asteroseismology from Dome A, Antarctica DTSTART;TZID=Asia/Shanghai:20150618T160000 DTEND;TZID=Asia/Shanghai:20150618T160000 LAST-MODIFIED:20150507T093921Z LOCATION:KIAA-PKU Auditorium SUMMARY:High duty-cycle time-series photometric observations in multiple colors for asteroseismology from Dome A, Antarctica URL;TYPE=URI:/info/1024/4525.htm END:VEVENT BEGIN:VEVENT UID:4903@kiaa.pku.edu.cn DTSTAMP:20150610T105357Z CREATED:20150610T105357Z DESCRIPTION:Revealing the mysteries behind galaxy formation feedback using Bayesian computation and back-of-envelope calculation DTSTART;TZID=Asia/Shanghai:20150619T120000 DTEND;TZID=Asia/Shanghai:20150619T130000 LAST-MODIFIED:20150610T105357Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Revealing the mysteries behind galaxy formation feedback using Bayesian computation and back-of-envelope calculation URL;TYPE=URI:/info/1025/4903.htm END:VEVENT BEGIN:VEVENT UID:4712@kiaa.pku.edu.cn DTSTAMP:20150622T121000Z CREATED:20150622T121000Z DESCRIPTION:Volcanism on Venus DTSTART;TZID=Asia/Shanghai:20150630T120000 DTEND;TZID=Asia/Shanghai:20150630T130000 LAST-MODIFIED:20150622T121000Z LOCATION:KIAA-PKU SUMMARY:Volcanism on Venus URL;TYPE=URI:/info/1028/4712.htm END:VEVENT BEGIN:VEVENT UID:4520@kiaa.pku.edu.cn DTSTAMP:20150401T004233Z CREATED:20150401T004233Z DESCRIPTION:Cosmic-ray Streaming Instabilities using MHD-Particle-in-Cell Method DTSTART;TZID=Asia/Shanghai:20150709T160000 DTEND;TZID=Asia/Shanghai:20150709T160000 LAST-MODIFIED:20150401T004233Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmic-ray Streaming Instabilities using MHD-Particle-in-Cell Method URL;TYPE=URI:/info/1024/4520.htm END:VEVENT BEGIN:VEVENT UID:5160@kiaa.pku.edu.cn DTSTAMP:20150202T145421Z CREATED:20150202T145421Z DESCRIPTION:2015 East-Asia AGN Workshop DTSTART;TZID=Asia/Shanghai:20150714T090000 DTEND;TZID=Asia/Shanghai:20150716T170000 LAST-MODIFIED:20150202T145421Z LOCATION:Changchun, China SUMMARY:2015 East-Asia AGN Workshop URL;TYPE=URI:/info/1026/5160.htm END:VEVENT BEGIN:VEVENT UID:4529@kiaa.pku.edu.cn DTSTAMP:20150706T163237Z CREATED:20150706T163237Z DESCRIPTION:Footprints of gas accretion in low redshift massive galaxies DTSTART;TZID=Asia/Shanghai:20150723T160000 DTEND;TZID=Asia/Shanghai:20150723T160000 LAST-MODIFIED:20150706T163237Z LOCATION:KIAA-PKU Auditorium SUMMARY:Footprints of gas accretion in low redshift massive galaxies URL;TYPE=URI:/info/1024/4529.htm END:VEVENT BEGIN:VEVENT UID:4906@kiaa.pku.edu.cn DTSTAMP:20150723T094615Z CREATED:20150723T094615Z DESCRIPTION:The early phase of star formation: Disk and Jet formation DTSTART;TZID=Asia/Shanghai:20150731T120000 DTEND;TZID=Asia/Shanghai:20150731T130000 LAST-MODIFIED:20150723T094615Z LOCATION:KIAA, Meeting room, 1st floor SUMMARY:The early phase of star formation: Disk and Jet formation URL;TYPE=URI:/info/1025/4906.htm END:VEVENT BEGIN:VEVENT UID:4713@kiaa.pku.edu.cn DTSTAMP:20150727T174858Z CREATED:20150727T174858Z DESCRIPTION:How do massive stars get their super-Eddington luminosity? DTSTART;TZID=Asia/Shanghai:20150826T120000 DTEND;TZID=Asia/Shanghai:20150826T130000 LAST-MODIFIED:20150727T174858Z LOCATION:KIAA-PKU SUMMARY:How do massive stars get their super-Eddington luminosity? URL;TYPE=URI:/info/1028/4713.htm END:VEVENT BEGIN:VEVENT UID:4788@kiaa.pku.edu.cn DTSTAMP:20150828T105141Z CREATED:20150828T105141Z DESCRIPTION:The systematic search of dual AGN and as probe to study the co-evolution between host galaxy and black hole DTSTART;TZID=Asia/Shanghai:20150831T170000 DTEND;TZID=Asia/Shanghai:20150831T180000 LAST-MODIFIED:20150828T105141Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The systematic search of dual AGN and as probe to study the co-evolution between host galaxy and black hole URL;TYPE=URI:/info/1029/4788.htm END:VEVENT BEGIN:VEVENT UID:4907@kiaa.pku.edu.cn DTSTAMP:20150813T123623Z CREATED:20150813T123623Z DESCRIPTION:Investigating Properties of AGNs Through Multi-wavelength Reverberation Mapping DTSTART;TZID=Asia/Shanghai:20150902T120000 DTEND;TZID=Asia/Shanghai:20150902T130000 LAST-MODIFIED:20150813T123623Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Investigating Properties of AGNs Through Multi-wavelength Reverberation Mapping URL;TYPE=URI:/info/1025/4907.htm END:VEVENT BEGIN:VEVENT UID:4789@kiaa.pku.edu.cn DTSTAMP:20150828T105250Z CREATED:20150828T105250Z DESCRIPTION:A comprehensive inspection of an AGN/host spectral decomposition technique DTSTART;TZID=Asia/Shanghai:20150907T170000 DTEND;TZID=Asia/Shanghai:20150907T180000 LAST-MODIFIED:20150828T105250Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:A comprehensive inspection of an AGN/host spectral decomposition technique URL;TYPE=URI:/info/1029/4789.htm END:VEVENT BEGIN:VEVENT UID:4909@kiaa.pku.edu.cn DTSTAMP:20150824T092651Z CREATED:20150824T092651Z DESCRIPTION:GAMMA-RAY EMISSION FROM SUPERNOVA REMNANTS INTERACTING WITH MOLECULAR CLUMPS DTSTART;TZID=Asia/Shanghai:20150909T120000 DTEND;TZID=Asia/Shanghai:20150909T130000 LAST-MODIFIED:20150824T092651Z LOCATION:KIAA, 1st floor meeting room SUMMARY:GAMMA-RAY EMISSION FROM SUPERNOVA REMNANTS INTERACTING WITH MOLECULAR CLUMPS URL;TYPE=URI:/info/1025/4909.htm END:VEVENT BEGIN:VEVENT UID:4534@kiaa.pku.edu.cn DTSTAMP:20150806T161559Z CREATED:20150806T161559Z DESCRIPTION:Recent Results from the Australian SKA Site DTSTART;TZID=Asia/Shanghai:20150910T160000 DTEND;TZID=Asia/Shanghai:20150910T160000 LAST-MODIFIED:20150806T161559Z LOCATION:KIAA-PKU Auditorium SUMMARY:Recent Results from the Australian SKA Site URL;TYPE=URI:/info/1024/4534.htm END:VEVENT BEGIN:VEVENT UID:4791@kiaa.pku.edu.cn DTSTAMP:20150912T164759Z CREATED:20150912T164759Z DESCRIPTION:Bayesian Inference in Gravitational Wave Data Analysis DTSTART;TZID=Asia/Shanghai:20150914T170000 DTEND;TZID=Asia/Shanghai:20150914T180000 LAST-MODIFIED:20150912T164759Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Bayesian Inference in Gravitational Wave Data Analysis URL;TYPE=URI:/info/1029/4791.htm END:VEVENT BEGIN:VEVENT UID:4532@kiaa.pku.edu.cn DTSTAMP:20150715T230912Z CREATED:20150715T230912Z DESCRIPTION:Preparing for the SKA DTSTART;TZID=Asia/Shanghai:20150917T160000 DTEND;TZID=Asia/Shanghai:20150917T160000 LAST-MODIFIED:20150715T230912Z LOCATION:KIAA-PKU Auditorium SUMMARY:Preparing for the SKA URL;TYPE=URI:/info/1024/4532.htm END:VEVENT BEGIN:VEVENT UID:4528@kiaa.pku.edu.cn DTSTAMP:20150701T084221Z CREATED:20150701T084221Z DESCRIPTION:The High Energy Astroparticle Physics Frontier DTSTART;TZID=Asia/Shanghai:20150921T160000 DTEND;TZID=Asia/Shanghai:20150921T160000 LAST-MODIFIED:20150701T084221Z LOCATION:KIAA-PKU Auditorium SUMMARY:The High Energy Astroparticle Physics Frontier URL;TYPE=URI:/info/1024/4528.htm END:VEVENT BEGIN:VEVENT UID:4790@kiaa.pku.edu.cn DTSTAMP:20150828T105346Z CREATED:20150828T105346Z DESCRIPTION:Gas Kinematics in a Galaxy’s Circumgalacitc Medium (CGM): Simulation and Observation DTSTART;TZID=Asia/Shanghai:20150921T173000 DTEND;TZID=Asia/Shanghai:20150921T183000 LAST-MODIFIED:20150828T105346Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Gas Kinematics in a Galaxy’s Circumgalacitc Medium (CGM): Simulation and Observation URL;TYPE=URI:/info/1029/4790.htm END:VEVENT BEGIN:VEVENT UID:4908@kiaa.pku.edu.cn DTSTAMP:20150818T171134Z CREATED:20150818T171134Z DESCRIPTION:MHD simulations of collision-induced magnetic reconnection in Poynting-flux-dominated jets and interpretation to the polarization observations of GRBs and blazar flares DTSTART;TZID=Asia/Shanghai:20150922T120000 DTEND;TZID=Asia/Shanghai:20150922T130000 LAST-MODIFIED:20150818T171134Z LOCATION:KIAA, 1st floor meeting room SUMMARY:MHD simulations of collision-induced magnetic reconnection in Poynting-flux-dominated jets and interpretation to the polarization observations of GRBs and blazar flares URL;TYPE=URI:/info/1025/4908.htm END:VEVENT BEGIN:VEVENT UID:4913@kiaa.pku.edu.cn DTSTAMP:20150918T124112Z CREATED:20150918T124112Z DESCRIPTION:The gamma-ray afterglow of tidal disruption events DTSTART;TZID=Asia/Shanghai:20150924T120000 DTEND;TZID=Asia/Shanghai:20150924T130000 LAST-MODIFIED:20150918T124112Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The gamma-ray afterglow of tidal disruption events URL;TYPE=URI:/info/1025/4913.htm END:VEVENT BEGIN:VEVENT UID:5165@kiaa.pku.edu.cn DTSTAMP:20150715T140530Z CREATED:20150715T140530Z DESCRIPTION:KIAA Workshop on Astroparticle Physics DTSTART;TZID=Asia/Shanghai:20150928T090000 DTEND;TZID=Asia/Shanghai:20150929T170000 LAST-MODIFIED:20150715T140530Z LOCATION:KIAA-PKU SUMMARY:KIAA Workshop on Astroparticle Physics URL;TYPE=URI:/info/1026/5165.htm END:VEVENT BEGIN:VEVENT UID:4535@kiaa.pku.edu.cn DTSTAMP:20150813T123621Z CREATED:20150813T123621Z DESCRIPTION:Searching for chemical relics of first stars with LAMOST DTSTART;TZID=Asia/Shanghai:20151008T160000 DTEND;TZID=Asia/Shanghai:20151008T160000 LAST-MODIFIED:20150813T123621Z LOCATION:KIAA-PKU Auditorium SUMMARY:Searching for chemical relics of first stars with LAMOST URL;TYPE=URI:/info/1024/4535.htm END:VEVENT BEGIN:VEVENT UID:4910@kiaa.pku.edu.cn DTSTAMP:20150907T141431Z CREATED:20150907T141431Z DESCRIPTION:What is gravity doing in star-forming regions? An observational view DTSTART;TZID=Asia/Shanghai:20151012T120000 DTEND;TZID=Asia/Shanghai:20151012T130000 LAST-MODIFIED:20150907T141431Z LOCATION:DoA, Rm 2907 SUMMARY:What is gravity doing in star-forming regions? An observational view URL;TYPE=URI:/info/1025/4910.htm END:VEVENT BEGIN:VEVENT UID:4792@kiaa.pku.edu.cn DTSTAMP:20150926T135430Z CREATED:20150926T135430Z DESCRIPTION:Practice talking for CAS meeting DTSTART;TZID=Asia/Shanghai:20151012T170000 DTEND;TZID=Asia/Shanghai:20151012T180000 LAST-MODIFIED:20150926T135430Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Practice talking for CAS meeting URL;TYPE=URI:/info/1029/4792.htm END:VEVENT BEGIN:VEVENT UID:4912@kiaa.pku.edu.cn DTSTAMP:20150914T140052Z CREATED:20150914T140052Z DESCRIPTION:The Deuteration Clock for Massive starless Cores DTSTART;TZID=Asia/Shanghai:20151013T120000 DTEND;TZID=Asia/Shanghai:20151013T130000 LAST-MODIFIED:20150914T140052Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The Deuteration Clock for Massive starless Cores URL;TYPE=URI:/info/1025/4912.htm END:VEVENT BEGIN:VEVENT UID:4911@kiaa.pku.edu.cn DTSTAMP:20150907T141618Z CREATED:20150907T141618Z DESCRIPTION:Non-thermal pressure in galaxy clusters: what astrophysics can do for cosmology and vice versa DTSTART;TZID=Asia/Shanghai:20151014T120000 DTEND;TZID=Asia/Shanghai:20151014T130000 LAST-MODIFIED:20150907T141618Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Non-thermal pressure in galaxy clusters: what astrophysics can do for cosmology and vice versa URL;TYPE=URI:/info/1025/4911.htm END:VEVENT BEGIN:VEVENT UID:4793@kiaa.pku.edu.cn DTSTAMP:20151007T212055Z CREATED:20151007T212055Z DESCRIPTION:Practice talking for CAS meeting DTSTART;TZID=Asia/Shanghai:20151014T170000 DTEND;TZID=Asia/Shanghai:20151014T180000 LAST-MODIFIED:20151007T212055Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Practice talking for CAS meeting URL;TYPE=URI:/info/1029/4793.htm END:VEVENT BEGIN:VEVENT UID:4533@kiaa.pku.edu.cn DTSTAMP:20150731T002330Z CREATED:20150731T002330Z DESCRIPTION:Infrared photometric/spectroscopic observations of Cepheid variable stars as tracers of the Milky Way DTSTART;TZID=Asia/Shanghai:20151015T160000 DTEND;TZID=Asia/Shanghai:20151015T160000 LAST-MODIFIED:20150731T002330Z LOCATION:KIAA-PKU Auditorium SUMMARY:Infrared photometric/spectroscopic observations of Cepheid variable stars as tracers of the Milky Way URL;TYPE=URI:/info/1024/4533.htm END:VEVENT BEGIN:VEVENT UID:4540@kiaa.pku.edu.cn DTSTAMP:20150922T145303Z CREATED:20150922T145303Z DESCRIPTION:Giant Monopoles as a Dark Matter Candidate DTSTART;TZID=Asia/Shanghai:20151022T160000 DTEND;TZID=Asia/Shanghai:20151022T160000 LAST-MODIFIED:20150922T145303Z LOCATION:KIAA-PKU Auditorium SUMMARY:Giant Monopoles as a Dark Matter Candidate URL;TYPE=URI:/info/1024/4540.htm END:VEVENT BEGIN:VEVENT UID:4915@kiaa.pku.edu.cn DTSTAMP:20151006T112848Z CREATED:20151006T112848Z DESCRIPTION:$\sigma_8$ tension and Horndeski Gravity DTSTART;TZID=Asia/Shanghai:20151026T120000 DTEND;TZID=Asia/Shanghai:20151026T130000 LAST-MODIFIED:20151006T112848Z LOCATION:DoA, Rm 2907 SUMMARY:$\sigma_8$ tension and Horndeski Gravity URL;TYPE=URI:/info/1025/4915.htm END:VEVENT BEGIN:VEVENT UID:4914@kiaa.pku.edu.cn DTSTAMP:20150922T150551Z CREATED:20150922T150551Z DESCRIPTION:H2O in Herschel high-z galaxies, a new diagnosis of their dense cores DTSTART;TZID=Asia/Shanghai:20151028T120000 DTEND;TZID=Asia/Shanghai:20151028T130000 LAST-MODIFIED:20150922T150551Z LOCATION:KIAA, 1st floor meeting room SUMMARY:H2O in Herschel high-z galaxies, a new diagnosis of their dense cores URL;TYPE=URI:/info/1025/4914.htm END:VEVENT BEGIN:VEVENT UID:4527@kiaa.pku.edu.cn DTSTAMP:20150630T163551Z CREATED:20150630T163551Z DESCRIPTION:AGN-driven outflows, stellar feedback and strangulation: the multiple routes to quench star formation DTSTART;TZID=Asia/Shanghai:20151029T160000 DTEND;TZID=Asia/Shanghai:20151029T160000 LAST-MODIFIED:20150630T163551Z LOCATION:KIAA-PKU Auditorium SUMMARY:AGN-driven outflows, stellar feedback and strangulation: the multiple routes to quench star formation URL;TYPE=URI:/info/1024/4527.htm END:VEVENT BEGIN:VEVENT UID:4715@kiaa.pku.edu.cn DTSTAMP:20150923T113231Z CREATED:20150923T113231Z DESCRIPTION:Radiative efficiency of Quasars DTSTART;TZID=Asia/Shanghai:20151030T120000 DTEND;TZID=Asia/Shanghai:20151030T130000 LAST-MODIFIED:20150923T113231Z LOCATION:KIAA-PKU (Pizza discussion) SUMMARY:Radiative efficiency of Quasars URL;TYPE=URI:/info/1028/4715.htm END:VEVENT BEGIN:VEVENT UID:4905@kiaa.pku.edu.cn DTSTAMP:20150713T122828Z CREATED:20150713T122828Z DESCRIPTION:Pulsars and Gravity DTSTART;TZID=Asia/Shanghai:20151102T120000 DTEND;TZID=Asia/Shanghai:20151102T130000 LAST-MODIFIED:20150713T122828Z LOCATION:DoA, Rm 2907 SUMMARY:Pulsars and Gravity URL;TYPE=URI:/info/1025/4905.htm END:VEVENT BEGIN:VEVENT UID:4916@kiaa.pku.edu.cn DTSTAMP:20151006T113537Z CREATED:20151006T113537Z DESCRIPTION:The University of Arizona and The Next Generation of Astronomical Observatories DTSTART;TZID=Asia/Shanghai:20151102T140000 DTEND;TZID=Asia/Shanghai:20151102T150000 LAST-MODIFIED:20151006T113537Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The University of Arizona and The Next Generation of Astronomical Observatories URL;TYPE=URI:/info/1025/4916.htm END:VEVENT BEGIN:VEVENT UID:4795@kiaa.pku.edu.cn DTSTAMP:20151030T161925Z CREATED:20151030T161925Z DESCRIPTION:Dynamical and Chemical Structure of Galactic Halos DTSTART;TZID=Asia/Shanghai:20151102T170000 DTEND;TZID=Asia/Shanghai:20151102T180000 LAST-MODIFIED:20151030T161925Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Dynamical and Chemical Structure of Galactic Halos URL;TYPE=URI:/info/1029/4795.htm END:VEVENT BEGIN:VEVENT UID:4530@kiaa.pku.edu.cn DTSTAMP:20150709T144601Z CREATED:20150709T144601Z DESCRIPTION:Supermassive Black Hole Binary Evolution in Galaxy Mergers - A stellar dynamical perspective DTSTART;TZID=Asia/Shanghai:20151105T160000 DTEND;TZID=Asia/Shanghai:20151105T160000 LAST-MODIFIED:20150709T144601Z LOCATION:KIAA-PKU Auditorium SUMMARY:Supermassive Black Hole Binary Evolution in Galaxy Mergers - A stellar dynamical perspective URL;TYPE=URI:/info/1024/4530.htm END:VEVENT BEGIN:VEVENT UID:4714@kiaa.pku.edu.cn DTSTAMP:20150922T153407Z CREATED:20150922T153407Z DESCRIPTION:The secular evolution of the Milky Way disk DTSTART;TZID=Asia/Shanghai:20151110T120000 DTEND;TZID=Asia/Shanghai:20151110T120000 LAST-MODIFIED:20150922T153407Z LOCATION:KIAA-PKU (Pizza discussion) SUMMARY:The secular evolution of the Milky Way disk URL;TYPE=URI:/info/1028/4714.htm END:VEVENT BEGIN:VEVENT UID:5167@kiaa.pku.edu.cn DTSTAMP:20151030T114027Z CREATED:20151030T114027Z DESCRIPTION:KIAA/DoA 2015 Postdoc Science Day DTSTART;TZID=Asia/Shanghai:20151111T100000 DTEND;TZID=Asia/Shanghai:20151111T170000 LAST-MODIFIED:20151030T114027Z LOCATION:KIAA Auditorium SUMMARY:KIAA/DoA 2015 Postdoc Science Day URL;TYPE=URI:/info/1026/5167.htm END:VEVENT BEGIN:VEVENT UID:4794@kiaa.pku.edu.cn DTSTAMP:20151028T192954Z CREATED:20151028T192954Z DESCRIPTION:Simulating the Chemo-Dynamical Evolution of Dwarf-Galaxy Discs DTSTART;TZID=Asia/Shanghai:20151111T173000 DTEND;TZID=Asia/Shanghai:20151111T173000 LAST-MODIFIED:20151028T192954Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Simulating the Chemo-Dynamical Evolution of Dwarf-Galaxy Discs URL;TYPE=URI:/info/1029/4794.htm END:VEVENT BEGIN:VEVENT UID:4539@kiaa.pku.edu.cn DTSTAMP:20150922T001041Z CREATED:20150922T001041Z DESCRIPTION:The Physics and Roles of Black Holes and Cosmic Rays in Cosmic Structure Evolution DTSTART;TZID=Asia/Shanghai:20151112T160000 DTEND;TZID=Asia/Shanghai:20151112T160000 LAST-MODIFIED:20150922T001041Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Physics and Roles of Black Holes and Cosmic Rays in Cosmic Structure Evolution URL;TYPE=URI:/info/1024/4539.htm END:VEVENT BEGIN:VEVENT UID:5166@kiaa.pku.edu.cn DTSTAMP:20151023T114524Z CREATED:20151023T114524Z DESCRIPTION:KIAA-PKU Forum 2015 DTSTART;TZID=Asia/Shanghai:20151116T090000 DTEND;TZID=Asia/Shanghai:20151117T170000 LAST-MODIFIED:20151023T114524Z LOCATION:KIAA Auditorium SUMMARY:KIAA-PKU Forum 2015 URL;TYPE=URI:/info/1026/5166.htm END:VEVENT BEGIN:VEVENT UID:4798@kiaa.pku.edu.cn DTSTAMP:20151103T175808Z CREATED:20151103T175808Z DESCRIPTION:Modeling stellar population from multi-wavelength galaxy SEDs DTSTART;TZID=Asia/Shanghai:20151118T170000 DTEND;TZID=Asia/Shanghai:20151118T180000 LAST-MODIFIED:20151103T175808Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Modeling stellar population from multi-wavelength galaxy SEDs URL;TYPE=URI:/info/1029/4798.htm END:VEVENT BEGIN:VEVENT UID:4531@kiaa.pku.edu.cn DTSTAMP:20150711T234219Z CREATED:20150711T234219Z DESCRIPTION:Neutrino Oscillations: Past, Present and Future DTSTART;TZID=Asia/Shanghai:20151119T160000 DTEND;TZID=Asia/Shanghai:20151119T160000 LAST-MODIFIED:20150711T234219Z LOCATION:KIAA-PKU Auditorium SUMMARY:Neutrino Oscillations: Past, Present and Future URL;TYPE=URI:/info/1024/4531.htm END:VEVENT BEGIN:VEVENT UID:4918@kiaa.pku.edu.cn DTSTAMP:20151028T184628Z CREATED:20151028T184628Z DESCRIPTION:The Innermost Mass Distribution of the Gravitational Lens SDP.81 from ALMA Observations DTSTART;TZID=Asia/Shanghai:20151120T120000 DTEND;TZID=Asia/Shanghai:20151120T130000 LAST-MODIFIED:20151028T184628Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The Innermost Mass Distribution of the Gravitational Lens SDP.81 from ALMA Observations URL;TYPE=URI:/info/1025/4918.htm END:VEVENT BEGIN:VEVENT UID:4917@kiaa.pku.edu.cn DTSTAMP:20151027T152333Z CREATED:20151027T152333Z DESCRIPTION:Hydrodynamic Simulations of the Central Molecular Zone with a Realistic Galactic Potential DTSTART;TZID=Asia/Shanghai:20151123T120000 DTEND;TZID=Asia/Shanghai:20151123T130000 LAST-MODIFIED:20151027T152333Z LOCATION:DoA, Rm 2907 SUMMARY:Hydrodynamic Simulations of the Central Molecular Zone with a Realistic Galactic Potential URL;TYPE=URI:/info/1025/4917.htm END:VEVENT BEGIN:VEVENT UID:4796@kiaa.pku.edu.cn DTSTAMP:20151102T161432Z CREATED:20151102T161432Z DESCRIPTION:A Chandra archive survey of AGNs in nearby galaxies DTSTART;TZID=Asia/Shanghai:20151123T170000 DTEND;TZID=Asia/Shanghai:20151123T180000 LAST-MODIFIED:20151102T161432Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:A Chandra archive survey of AGNs in nearby galaxies URL;TYPE=URI:/info/1029/4796.htm END:VEVENT BEGIN:VEVENT UID:4716@kiaa.pku.edu.cn DTSTAMP:20151124T141710Z CREATED:20151124T141710Z DESCRIPTION:Large Surveys in Astronomy (with Particular Focus on SDSS and LSST DTSTART;TZID=Asia/Shanghai:20151124T120000 DTEND;TZID=Asia/Shanghai:20151124T130000 LAST-MODIFIED:20151124T141710Z LOCATION:KIAA-PKU SUMMARY:Large Surveys in Astronomy (with Particular Focus on SDSS and LSST URL;TYPE=URI:/info/1028/4716.htm END:VEVENT BEGIN:VEVENT UID:4541@kiaa.pku.edu.cn DTSTAMP:20150924T221955Z CREATED:20150924T221955Z DESCRIPTION:Supermassive binary black holes in Active Galactic Nuclei: theoretical and observational perspectives DTSTART;TZID=Asia/Shanghai:20151126T160000 DTEND;TZID=Asia/Shanghai:20151126T160000 LAST-MODIFIED:20150924T221955Z LOCATION:KIAA-PKU Auditorium SUMMARY:Supermassive binary black holes in Active Galactic Nuclei: theoretical and observational perspectives URL;TYPE=URI:/info/1024/4541.htm END:VEVENT BEGIN:VEVENT UID:4797@kiaa.pku.edu.cn DTSTAMP:20151102T161631Z CREATED:20151102T161631Z DESCRIPTION:Modern resources for data science in astronomy DTSTART;TZID=Asia/Shanghai:20151130T170000 DTEND;TZID=Asia/Shanghai:20151130T180000 LAST-MODIFIED:20151102T161631Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Modern resources for data science in astronomy URL;TYPE=URI:/info/1029/4797.htm END:VEVENT BEGIN:VEVENT UID:4922@kiaa.pku.edu.cn DTSTAMP:20151117T130137Z CREATED:20151117T130137Z DESCRIPTION:The Gaia mission DTSTART;TZID=Asia/Shanghai:20151201T120000 DTEND;TZID=Asia/Shanghai:20151201T130000 LAST-MODIFIED:20151117T130137Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The Gaia mission URL;TYPE=URI:/info/1025/4922.htm END:VEVENT BEGIN:VEVENT UID:4717@kiaa.pku.edu.cn DTSTAMP:20151125T161202Z CREATED:20151125T161202Z DESCRIPTION:Past and future X-ray surveys - a brief and biased overview DTSTART;TZID=Asia/Shanghai:20151202T120000 DTEND;TZID=Asia/Shanghai:20151202T130000 LAST-MODIFIED:20151125T161202Z LOCATION:KIAA-PKU SUMMARY:Past and future X-ray surveys - a brief and biased overview URL;TYPE=URI:/info/1028/4717.htm END:VEVENT BEGIN:VEVENT UID:4538@kiaa.pku.edu.cn DTSTAMP:20150919T193534Z CREATED:20150919T193534Z DESCRIPTION:Interaction of stars with discs around AGNs DTSTART;TZID=Asia/Shanghai:20151203T160000 DTEND;TZID=Asia/Shanghai:20151203T160000 LAST-MODIFIED:20150919T193534Z LOCATION:KIAA-PKU Auditorium SUMMARY:Interaction of stars with discs around AGNs URL;TYPE=URI:/info/1024/4538.htm END:VEVENT BEGIN:VEVENT UID:4920@kiaa.pku.edu.cn DTSTAMP:20151112T144224Z CREATED:20151112T144224Z DESCRIPTION:The Magellanic Stream: "ram pressure plus collision" scenario DTSTART;TZID=Asia/Shanghai:20151204T120000 DTEND;TZID=Asia/Shanghai:20151204T130000 LAST-MODIFIED:20151112T144224Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The Magellanic Stream: "ram pressure plus collision" scenario URL;TYPE=URI:/info/1025/4920.htm END:VEVENT BEGIN:VEVENT UID:4718@kiaa.pku.edu.cn DTSTAMP:20151125T161246Z CREATED:20151125T161246Z DESCRIPTION:The first light instruments of TMT and GMT DTSTART;TZID=Asia/Shanghai:20151208T120000 DTEND;TZID=Asia/Shanghai:20151208T130000 LAST-MODIFIED:20151125T161246Z LOCATION:KIAA-PKU SUMMARY:The first light instruments of TMT and GMT URL;TYPE=URI:/info/1028/4718.htm END:VEVENT BEGIN:VEVENT UID:4921@kiaa.pku.edu.cn DTSTAMP:20151117T085811Z CREATED:20151117T085811Z DESCRIPTION:Active galaxies among X-ray, IR and radio sources DTSTART;TZID=Asia/Shanghai:20151209T120000 DTEND;TZID=Asia/Shanghai:20151209T130000 LAST-MODIFIED:20151117T085811Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Active galaxies among X-ray, IR and radio sources URL;TYPE=URI:/info/1025/4921.htm END:VEVENT BEGIN:VEVENT UID:4536@kiaa.pku.edu.cn DTSTAMP:20150827T230421Z CREATED:20150827T230421Z DESCRIPTION:The Rugged Landscape of the Core-Collapse Supernova Explosions DTSTART;TZID=Asia/Shanghai:20151210T160000 DTEND;TZID=Asia/Shanghai:20151210T160000 LAST-MODIFIED:20150827T230421Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Rugged Landscape of the Core-Collapse Supernova Explosions URL;TYPE=URI:/info/1024/4536.htm END:VEVENT BEGIN:VEVENT UID:4923@kiaa.pku.edu.cn DTSTAMP:20151125T163546Z CREATED:20151125T163546Z DESCRIPTION:Kinetic Temperatures of Molecular Gas: The Galactic center Region DTSTART;TZID=Asia/Shanghai:20151211T120000 DTEND;TZID=Asia/Shanghai:20151211T130000 LAST-MODIFIED:20151125T163546Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Kinetic Temperatures of Molecular Gas: The Galactic center Region URL;TYPE=URI:/info/1025/4923.htm END:VEVENT BEGIN:VEVENT UID:4719@kiaa.pku.edu.cn DTSTAMP:20151125T161349Z CREATED:20151125T161349Z DESCRIPTION:Inference techniques for stellar spectroscopy DTSTART;TZID=Asia/Shanghai:20151216T120000 DTEND;TZID=Asia/Shanghai:20151216T130000 LAST-MODIFIED:20151125T161349Z LOCATION:KIAA-PKU SUMMARY:Inference techniques for stellar spectroscopy URL;TYPE=URI:/info/1028/4719.htm END:VEVENT BEGIN:VEVENT UID:4537@kiaa.pku.edu.cn DTSTAMP:20150908T081052Z CREATED:20150908T081052Z DESCRIPTION:Cosmological studies with the REFLEX cluster survey DTSTART;TZID=Asia/Shanghai:20151217T160000 DTEND;TZID=Asia/Shanghai:20151217T160000 LAST-MODIFIED:20150908T081052Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmological studies with the REFLEX cluster survey URL;TYPE=URI:/info/1024/4537.htm END:VEVENT BEGIN:VEVENT UID:4924@kiaa.pku.edu.cn DTSTAMP:20151202T154900Z CREATED:20151202T154900Z DESCRIPTION:Lithium evolution from Pre-Main Sequence to the Spite plateau: An environmental solution to the cosmological lithium problem DTSTART;TZID=Asia/Shanghai:20151221T120000 DTEND;TZID=Asia/Shanghai:20151221T130000 LAST-MODIFIED:20151202T154900Z LOCATION:DoA, Rm 2907 SUMMARY:Lithium evolution from Pre-Main Sequence to the Spite plateau: An environmental solution to the cosmological lithium problem URL;TYPE=URI:/info/1025/4924.htm END:VEVENT BEGIN:VEVENT UID:4799@kiaa.pku.edu.cn DTSTAMP:20151204T194550Z CREATED:20151204T194550Z DESCRIPTION:Disk of the Small Magellanic Cloud as traced by Cepheids DTSTART;TZID=Asia/Shanghai:20151221T170000 DTEND;TZID=Asia/Shanghai:20151221T180000 LAST-MODIFIED:20151204T194550Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Disk of the Small Magellanic Cloud as traced by Cepheids URL;TYPE=URI:/info/1029/4799.htm END:VEVENT BEGIN:VEVENT UID:4720@kiaa.pku.edu.cn DTSTAMP:20151125T161504Z CREATED:20151125T161504Z DESCRIPTION:Ground-based and Space Missions for Asteroseismology DTSTART;TZID=Asia/Shanghai:20151222T120000 DTEND;TZID=Asia/Shanghai:20151222T130000 LAST-MODIFIED:20151125T161504Z LOCATION:KIAA-PKU SUMMARY:Ground-based and Space Missions for Asteroseismology URL;TYPE=URI:/info/1028/4720.htm END:VEVENT BEGIN:VEVENT UID:4919@kiaa.pku.edu.cn DTSTAMP:20151106T175418Z CREATED:20151106T175418Z DESCRIPTION:Relativistic deformability of compact stars DTSTART;TZID=Asia/Shanghai:20151228T120000 DTEND;TZID=Asia/Shanghai:20151228T130000 LAST-MODIFIED:20151106T175418Z LOCATION:DoA, Rm 2907 SUMMARY:Relativistic deformability of compact stars URL;TYPE=URI:/info/1025/4919.htm END:VEVENT BEGIN:VEVENT UID:4800@kiaa.pku.edu.cn DTSTAMP:20151217T012007Z CREATED:20151217T012007Z DESCRIPTION:Gaseous structures and mass drift in spiral galaxies DTSTART;TZID=Asia/Shanghai:20151228T170000 DTEND;TZID=Asia/Shanghai:20151228T180000 LAST-MODIFIED:20151217T012007Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Gaseous structures and mass drift in spiral galaxies URL;TYPE=URI:/info/1029/4800.htm END:VEVENT BEGIN:VEVENT UID:4721@kiaa.pku.edu.cn DTSTAMP:20151125T161554Z CREATED:20151125T161554Z DESCRIPTION:Filamentary structures in ISM - Herschel view DTSTART;TZID=Asia/Shanghai:20151229T120000 DTEND;TZID=Asia/Shanghai:20151229T130000 LAST-MODIFIED:20151125T161554Z LOCATION:KIAA-PKU SUMMARY:Filamentary structures in ISM - Herschel view URL;TYPE=URI:/info/1028/4721.htm END:VEVENT BEGIN:VEVENT UID:4927@kiaa.pku.edu.cn DTSTAMP:20151216T115351Z CREATED:20151216T115351Z DESCRIPTION:The nIFTy galaxy cluster comparison project DTSTART;TZID=Asia/Shanghai:20160105T120000 DTEND;TZID=Asia/Shanghai:20160105T130000 LAST-MODIFIED:20151216T115351Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The nIFTy galaxy cluster comparison project URL;TYPE=URI:/info/1025/4927.htm END:VEVENT BEGIN:VEVENT UID:4925@kiaa.pku.edu.cn DTSTAMP:20151212T140238Z CREATED:20151212T140238Z DESCRIPTION:Cosmology and Astrophysics with Galaxy Clusters, from the Numerical Perspective DTSTART;TZID=Asia/Shanghai:20160108T120000 DTEND;TZID=Asia/Shanghai:20160108T130000 LAST-MODIFIED:20151212T140238Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Cosmology and Astrophysics with Galaxy Clusters, from the Numerical Perspective URL;TYPE=URI:/info/1025/4925.htm END:VEVENT BEGIN:VEVENT UID:4926@kiaa.pku.edu.cn DTSTAMP:20151213T122410Z CREATED:20151213T122410Z DESCRIPTION:Circumbinary Planets DTSTART;TZID=Asia/Shanghai:20160111T120000 DTEND;TZID=Asia/Shanghai:20160111T130000 LAST-MODIFIED:20151213T122410Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Circumbinary Planets URL;TYPE=URI:/info/1025/4926.htm END:VEVENT BEGIN:VEVENT UID:4723@kiaa.pku.edu.cn DTSTAMP:20151228T105403Z CREATED:20151228T105403Z DESCRIPTION:Hierarchical Three-body Dynamics --- How to Flip a Binary without a Spatula DTSTART;TZID=Asia/Shanghai:20160112T120000 DTEND;TZID=Asia/Shanghai:20160112T130000 LAST-MODIFIED:20151228T105403Z LOCATION:KIAA-PKU SUMMARY:Hierarchical Three-body Dynamics --- How to Flip a Binary without a Spatula URL;TYPE=URI:/info/1028/4723.htm END:VEVENT BEGIN:VEVENT UID:4543@kiaa.pku.edu.cn DTSTAMP:20160102T164412Z CREATED:20160102T164412Z DESCRIPTION:Exceptional X-ray Weak Quasars---Implications for Accretion Flows, BLRs, & Winds DTSTART;TZID=Asia/Shanghai:20160114T160000 DTEND;TZID=Asia/Shanghai:20160114T160000 LAST-MODIFIED:20160102T164412Z LOCATION:KIAA-PKU Auditorium SUMMARY:Exceptional X-ray Weak Quasars---Implications for Accretion Flows, BLRs, & Winds URL;TYPE=URI:/info/1024/4543.htm END:VEVENT BEGIN:VEVENT UID:4928@kiaa.pku.edu.cn DTSTAMP:20151217T191325Z CREATED:20151217T191325Z DESCRIPTION:The origin of the cosmic X-ray background - Challenging results from angular correlation studies with XBOOTES DTSTART;TZID=Asia/Shanghai:20160115T120000 DTEND;TZID=Asia/Shanghai:20160115T130000 LAST-MODIFIED:20151217T191325Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The origin of the cosmic X-ray background - Challenging results from angular correlation studies with XBOOTES URL;TYPE=URI:/info/1025/4928.htm END:VEVENT BEGIN:VEVENT UID:4801@kiaa.pku.edu.cn DTSTAMP:20160113T182815Z CREATED:20160113T182815Z DESCRIPTION:Chemical substructures in the high-mass star-forming regions DTSTART;TZID=Asia/Shanghai:20160115T170000 DTEND;TZID=Asia/Shanghai:20160115T180000 LAST-MODIFIED:20160113T182815Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Chemical substructures in the high-mass star-forming regions URL;TYPE=URI:/info/1029/4801.htm END:VEVENT BEGIN:VEVENT UID:4546@kiaa.pku.edu.cn DTSTAMP:20160113T092314Z CREATED:20160113T092314Z DESCRIPTION:Supermassive black hole formation at high redshifts DTSTART;TZID=Asia/Shanghai:20160118T160000 DTEND;TZID=Asia/Shanghai:20160118T160000 LAST-MODIFIED:20160113T092314Z LOCATION:KIAA-PKU Auditorium SUMMARY:Supermassive black hole formation at high redshifts URL;TYPE=URI:/info/1024/4546.htm END:VEVENT BEGIN:VEVENT UID:4547@kiaa.pku.edu.cn DTSTAMP:20160113T104331Z CREATED:20160113T104331Z DESCRIPTION:Numerical Modeling of Massive Star Clusters: An Evolving Story of the Black Holes DTSTART;TZID=Asia/Shanghai:20160119T160000 DTEND;TZID=Asia/Shanghai:20160119T160000 LAST-MODIFIED:20160113T104331Z LOCATION:KIAA-PKU Auditorium SUMMARY:Numerical Modeling of Massive Star Clusters: An Evolving Story of the Black Holes URL;TYPE=URI:/info/1024/4547.htm END:VEVENT BEGIN:VEVENT UID:4545@kiaa.pku.edu.cn DTSTAMP:20160113T091305Z CREATED:20160113T091305Z DESCRIPTION:HI in a Multi-wavelength Dissertation of Galaxies DTSTART;TZID=Asia/Shanghai:20160120T160000 DTEND;TZID=Asia/Shanghai:20160120T160000 LAST-MODIFIED:20160113T091305Z LOCATION:KIAA-PKU Auditorium SUMMARY:HI in a Multi-wavelength Dissertation of Galaxies URL;TYPE=URI:/info/1024/4545.htm END:VEVENT BEGIN:VEVENT UID:4929@kiaa.pku.edu.cn DTSTAMP:20160130T110739Z CREATED:20160130T110739Z DESCRIPTION:Modeling of hot Jupiter HD 189733b H alpha transmission spectral line & Formation and Asteroseismology of Extremely Low-mass White Dwarfs DTSTART;TZID=Asia/Shanghai:20160222T120000 DTEND;TZID=Asia/Shanghai:20160222T130000 LAST-MODIFIED:20160130T110739Z LOCATION:DoA, Rm 2907 SUMMARY:Modeling of hot Jupiter HD 189733b H alpha transmission spectral line & Formation and Asteroseismology of Extremely Low-mass White Dwarfs URL;TYPE=URI:/info/1025/4929.htm END:VEVENT BEGIN:VEVENT UID:4555@kiaa.pku.edu.cn DTSTAMP:20160204T190713Z CREATED:20160204T190713Z DESCRIPTION:Magnetar-Powered Transients DTSTART;TZID=Asia/Shanghai:20160225T160000 DTEND;TZID=Asia/Shanghai:20160225T160000 LAST-MODIFIED:20160204T190713Z LOCATION:KIAA-PKU Auditorium SUMMARY:Magnetar-Powered Transients URL;TYPE=URI:/info/1024/4555.htm END:VEVENT BEGIN:VEVENT UID:4802@kiaa.pku.edu.cn DTSTAMP:20160222T231743Z CREATED:20160222T231743Z DESCRIPTION:MESA 101 - An Introduction of a Stella Evolution Code DTSTART;TZID=Asia/Shanghai:20160225T171500 DTEND;TZID=Asia/Shanghai:20160225T181500 LAST-MODIFIED:20160222T231743Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:MESA 101 - An Introduction of a Stella Evolution Code URL;TYPE=URI:/info/1029/4802.htm END:VEVENT BEGIN:VEVENT UID:4724@kiaa.pku.edu.cn DTSTAMP:20160112T144214Z CREATED:20160112T144214Z DESCRIPTION:N-body simulations and Coarray Fortran parallelization DTSTART;TZID=Asia/Shanghai:20160301T120000 DTEND;TZID=Asia/Shanghai:20160301T130000 LAST-MODIFIED:20160112T144214Z LOCATION:KIAA-PKU SUMMARY:N-body simulations and Coarray Fortran parallelization URL;TYPE=URI:/info/1028/4724.htm END:VEVENT BEGIN:VEVENT UID:4548@kiaa.pku.edu.cn DTSTAMP:20160122T115104Z CREATED:20160122T115104Z DESCRIPTION:Searching for​ ​particle physics​ ​signals​ ​in the cosmological collider via​ ​gravitational wave​ ​surveys DTSTART;TZID=Asia/Shanghai:20160303T160000 DTEND;TZID=Asia/Shanghai:20160303T160000 LAST-MODIFIED:20160122T115104Z LOCATION:KIAA-PKU Auditorium SUMMARY:Searching for​ ​particle physics​ ​signals​ ​in the cosmological collider via​ ​gravitational wave​ ​surveys URL;TYPE=URI:/info/1024/4548.htm END:VEVENT BEGIN:VEVENT UID:4930@kiaa.pku.edu.cn DTSTAMP:20160201T174457Z CREATED:20160201T174457Z DESCRIPTION:The optical transients powered by millisecond magnetars DTSTART;TZID=Asia/Shanghai:20160304T120000 DTEND;TZID=Asia/Shanghai:20160304T130000 LAST-MODIFIED:20160201T174457Z LOCATION:KIAA, 1st floor meeting room SUMMARY:The optical transients powered by millisecond magnetars URL;TYPE=URI:/info/1025/4930.htm END:VEVENT BEGIN:VEVENT UID:4725@kiaa.pku.edu.cn DTSTAMP:20160112T144259Z CREATED:20160112T144259Z DESCRIPTION:(Weak) Gravitational Lensing: a brief overview DTSTART;TZID=Asia/Shanghai:20160308T120000 DTEND;TZID=Asia/Shanghai:20160308T130000 LAST-MODIFIED:20160112T144259Z LOCATION:KIAA-PKU SUMMARY:(Weak) Gravitational Lensing: a brief overview URL;TYPE=URI:/info/1028/4725.htm END:VEVENT BEGIN:VEVENT UID:4932@kiaa.pku.edu.cn DTSTAMP:20160305T121759Z CREATED:20160305T121759Z DESCRIPTION:Herschel observed Stripe 82 quasars and their host galaxies: connections between the AGN activity and the host galaxy star formation DTSTART;TZID=Asia/Shanghai:20160309T120000 DTEND;TZID=Asia/Shanghai:20160309T130000 LAST-MODIFIED:20160305T121759Z LOCATION:DoA, Rm 2907 SUMMARY:Herschel observed Stripe 82 quasars and their host galaxies: connections between the AGN activity and the host galaxy star formation URL;TYPE=URI:/info/1025/4932.htm END:VEVENT BEGIN:VEVENT UID:4556@kiaa.pku.edu.cn DTSTAMP:20160219T150034Z CREATED:20160219T150034Z DESCRIPTION:Probing the dark Universe with weak lensing effects DTSTART;TZID=Asia/Shanghai:20160310T160000 DTEND;TZID=Asia/Shanghai:20160310T160000 LAST-MODIFIED:20160219T150034Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing the dark Universe with weak lensing effects URL;TYPE=URI:/info/1024/4556.htm END:VEVENT BEGIN:VEVENT UID:4934@kiaa.pku.edu.cn DTSTAMP:20160308T133303Z CREATED:20160308T133303Z DESCRIPTION:New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star forming dwarf galaxies DTSTART;TZID=Asia/Shanghai:20160314T120000 DTEND;TZID=Asia/Shanghai:20160314T130000 LAST-MODIFIED:20160308T133303Z LOCATION:DoA, Rm 2907 SUMMARY:New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star forming dwarf galaxies URL;TYPE=URI:/info/1025/4934.htm END:VEVENT BEGIN:VEVENT UID:4722@kiaa.pku.edu.cn DTSTAMP:20151228T105256Z CREATED:20151228T105256Z DESCRIPTION:Photometric variables in the new era of surveys DTSTART;TZID=Asia/Shanghai:20160315T120000 DTEND;TZID=Asia/Shanghai:20160315T130000 LAST-MODIFIED:20151228T105256Z LOCATION:KIAA-PKU SUMMARY:Photometric variables in the new era of surveys URL;TYPE=URI:/info/1028/4722.htm END:VEVENT BEGIN:VEVENT UID:4935@kiaa.pku.edu.cn DTSTAMP:20160316T171754Z CREATED:20160316T171754Z DESCRIPTION:Searching for Inflationary Gravitational Waves and the Ali CMB project DTSTART;TZID=Asia/Shanghai:20160317T120000 DTEND;TZID=Asia/Shanghai:20160317T120000 LAST-MODIFIED:20160316T171754Z LOCATION:KIAA First floor meeting room SUMMARY:Searching for Inflationary Gravitational Waves and the Ali CMB project URL;TYPE=URI:/info/1025/4935.htm END:VEVENT BEGIN:VEVENT UID:4803@kiaa.pku.edu.cn DTSTAMP:20160313T091005Z CREATED:20160313T091005Z DESCRIPTION:Silicate Dust in AGNs DTSTART;TZID=Asia/Shanghai:20160317T171500 DTEND;TZID=Asia/Shanghai:20160317T181500 LAST-MODIFIED:20160313T091005Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Silicate Dust in AGNs URL;TYPE=URI:/info/1029/4803.htm END:VEVENT BEGIN:VEVENT UID:4726@kiaa.pku.edu.cn DTSTAMP:20160303T152754Z CREATED:20160303T152754Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20160322T120000 DTEND;TZID=Asia/Shanghai:20160322T130000 LAST-MODIFIED:20160303T152754Z LOCATION:KIAA-PKU SUMMARY:TBD URL;TYPE=URI:/info/1028/4726.htm END:VEVENT BEGIN:VEVENT UID:4805@kiaa.pku.edu.cn DTSTAMP:20160317T001522Z CREATED:20160317T001522Z DESCRIPTION:Large Surveys in Astronomy (with Particular Focus on SDSS and LSST) DTSTART;TZID=Asia/Shanghai:20160322T170000 DTEND;TZID=Asia/Shanghai:20160322T180000 LAST-MODIFIED:20160317T001522Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Large Surveys in Astronomy (with Particular Focus on SDSS and LSST) URL;TYPE=URI:/info/1029/4805.htm END:VEVENT BEGIN:VEVENT UID:4560@kiaa.pku.edu.cn DTSTAMP:20160317T174458Z CREATED:20160317T174458Z DESCRIPTION:Sterile neutrinos in particle physics and cosmology DTSTART;TZID=Asia/Shanghai:20160324T160000 DTEND;TZID=Asia/Shanghai:20160324T160000 LAST-MODIFIED:20160317T174458Z LOCATION:KIAA-PKU Auditorium SUMMARY:Sterile neutrinos in particle physics and cosmology URL;TYPE=URI:/info/1024/4560.htm END:VEVENT BEGIN:VEVENT UID:4936@kiaa.pku.edu.cn DTSTAMP:20160323T064036Z CREATED:20160323T064036Z DESCRIPTION:Using galaxy alignments to probe large scale structures DTSTART;TZID=Asia/Shanghai:20160325T120000 DTEND;TZID=Asia/Shanghai:20160325T130000 LAST-MODIFIED:20160323T064036Z LOCATION:KIAA, First Floor Meeting Room SUMMARY:Using galaxy alignments to probe large scale structures URL;TYPE=URI:/info/1025/4936.htm END:VEVENT BEGIN:VEVENT UID:4727@kiaa.pku.edu.cn DTSTAMP:20160303T152847Z CREATED:20160303T152847Z DESCRIPTION:A road map for the generation of NIR guide star catalog for TMT observations DTSTART;TZID=Asia/Shanghai:20160329T120000 DTEND;TZID=Asia/Shanghai:20160329T130000 LAST-MODIFIED:20160303T152847Z LOCATION:KIAA-PKU SUMMARY:A road map for the generation of NIR guide star catalog for TMT observations URL;TYPE=URI:/info/1028/4727.htm END:VEVENT BEGIN:VEVENT UID:4551@kiaa.pku.edu.cn DTSTAMP:20160123T235855Z CREATED:20160123T235855Z DESCRIPTION:Self-interacting dark matter and the supermassive black holes in the early universe DTSTART;TZID=Asia/Shanghai:20160331T160000 DTEND;TZID=Asia/Shanghai:20160331T160000 LAST-MODIFIED:20160123T235855Z LOCATION:KIAA-PKU Auditorium SUMMARY:Self-interacting dark matter and the supermassive black holes in the early universe URL;TYPE=URI:/info/1024/4551.htm END:VEVENT BEGIN:VEVENT UID:4804@kiaa.pku.edu.cn DTSTAMP:20160314T135113Z CREATED:20160314T135113Z DESCRIPTION:Stellar M/L ratio gradients of E+S0 galaxies and their implication to IMF variation DTSTART;TZID=Asia/Shanghai:20160331T170000 DTEND;TZID=Asia/Shanghai:20160331T180000 LAST-MODIFIED:20160314T135113Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Stellar M/L ratio gradients of E+S0 galaxies and their implication to IMF variation URL;TYPE=URI:/info/1029/4804.htm END:VEVENT BEGIN:VEVENT UID:4931@kiaa.pku.edu.cn DTSTAMP:20160304T114725Z CREATED:20160304T114725Z DESCRIPTION:Interstellar fullerenes and diffuse interstellar bands DTSTART;TZID=Asia/Shanghai:20160405T120000 DTEND;TZID=Asia/Shanghai:20160405T130000 LAST-MODIFIED:20160304T114725Z LOCATION:KIAA, First floor meeting room SUMMARY:Interstellar fullerenes and diffuse interstellar bands URL;TYPE=URI:/info/1025/4931.htm END:VEVENT BEGIN:VEVENT UID:4549@kiaa.pku.edu.cn DTSTAMP:20160123T160121Z CREATED:20160123T160121Z DESCRIPTION:Gas inflow patterns and nuclear rings in barred galaxies DTSTART;TZID=Asia/Shanghai:20160407T160000 DTEND;TZID=Asia/Shanghai:20160407T160000 LAST-MODIFIED:20160123T160121Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gas inflow patterns and nuclear rings in barred galaxies URL;TYPE=URI:/info/1024/4549.htm END:VEVENT BEGIN:VEVENT UID:4806@kiaa.pku.edu.cn DTSTAMP:20160325T111411Z CREATED:20160325T111411Z DESCRIPTION:Environmental dependence of galaxy metallicity and age gradients DTSTART;TZID=Asia/Shanghai:20160407T170000 DTEND;TZID=Asia/Shanghai:20160407T180000 LAST-MODIFIED:20160325T111411Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Environmental dependence of galaxy metallicity and age gradients URL;TYPE=URI:/info/1029/4806.htm END:VEVENT BEGIN:VEVENT UID:4728@kiaa.pku.edu.cn DTSTAMP:20160303T152952Z CREATED:20160303T152952Z DESCRIPTION:Dynamical and Kinematic features of the Gas in Disk Galaxies DTSTART;TZID=Asia/Shanghai:20160412T120000 DTEND;TZID=Asia/Shanghai:20160412T130000 LAST-MODIFIED:20160303T152952Z LOCATION:KIAA-PKU SUMMARY:Dynamical and Kinematic features of the Gas in Disk Galaxies URL;TYPE=URI:/info/1028/4728.htm END:VEVENT BEGIN:VEVENT UID:4559@kiaa.pku.edu.cn DTSTAMP:20160229T111253Z CREATED:20160229T111253Z DESCRIPTION:Dwarf Galaxies: Laboratories for Nucleosynthesis and Dark Matter DTSTART;TZID=Asia/Shanghai:20160412T160000 DTEND;TZID=Asia/Shanghai:20160412T160000 LAST-MODIFIED:20160229T111253Z LOCATION:KIAA-PKU Auditorium SUMMARY:Dwarf Galaxies: Laboratories for Nucleosynthesis and Dark Matter URL;TYPE=URI:/info/1024/4559.htm END:VEVENT BEGIN:VEVENT UID:4542@kiaa.pku.edu.cn DTSTAMP:20151127T214724Z CREATED:20151127T214724Z DESCRIPTION:The Galaxy-Halo Connection From The Velocity Field DTSTART;TZID=Asia/Shanghai:20160414T160000 DTEND;TZID=Asia/Shanghai:20160414T160000 LAST-MODIFIED:20151127T214724Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Galaxy-Halo Connection From The Velocity Field URL;TYPE=URI:/info/1024/4542.htm END:VEVENT BEGIN:VEVENT UID:4938@kiaa.pku.edu.cn DTSTAMP:20160405T111154Z CREATED:20160405T111154Z DESCRIPTION:What does LIGO event GW150914 teach us about stellar dynamics? DTSTART;TZID=Asia/Shanghai:20160418T120000 DTEND;TZID=Asia/Shanghai:20160418T130000 LAST-MODIFIED:20160405T111154Z LOCATION:DoA, Rm 2907 SUMMARY:What does LIGO event GW150914 teach us about stellar dynamics? URL;TYPE=URI:/info/1025/4938.htm END:VEVENT BEGIN:VEVENT UID:4550@kiaa.pku.edu.cn DTSTAMP:20160123T160208Z CREATED:20160123T160208Z DESCRIPTION:The Co-evolution of AGNs and Galaxies, Viewed from 2D Spectroscopy DTSTART;TZID=Asia/Shanghai:20160421T160000 DTEND;TZID=Asia/Shanghai:20160421T160000 LAST-MODIFIED:20160123T160208Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Co-evolution of AGNs and Galaxies, Viewed from 2D Spectroscopy URL;TYPE=URI:/info/1024/4550.htm END:VEVENT BEGIN:VEVENT UID:4729@kiaa.pku.edu.cn DTSTAMP:20160303T153120Z CREATED:20160303T153120Z DESCRIPTION:The stellar population structure of the Galactic disk from the LAMOST survey DTSTART;TZID=Asia/Shanghai:20160426T120000 DTEND;TZID=Asia/Shanghai:20160426T130000 LAST-MODIFIED:20160303T153120Z LOCATION:KIAA-PKU SUMMARY:The stellar population structure of the Galactic disk from the LAMOST survey URL;TYPE=URI:/info/1028/4729.htm END:VEVENT BEGIN:VEVENT UID:4544@kiaa.pku.edu.cn DTSTAMP:20160107T092659Z CREATED:20160107T092659Z DESCRIPTION:Brown Dwarfs as Exoplanet Analogs DTSTART;TZID=Asia/Shanghai:20160428T160000 DTEND;TZID=Asia/Shanghai:20160428T160000 LAST-MODIFIED:20160107T092659Z LOCATION:KIAA-PKU Auditorium SUMMARY:Brown Dwarfs as Exoplanet Analogs URL;TYPE=URI:/info/1024/4544.htm END:VEVENT BEGIN:VEVENT UID:4807@kiaa.pku.edu.cn DTSTAMP:20160418T151939Z CREATED:20160418T151939Z DESCRIPTION:Multi-wavelength galaxy profile fitting, and combining structural decomposition with stellar population synthesis DTSTART;TZID=Asia/Shanghai:20160428T170000 DTEND;TZID=Asia/Shanghai:20160428T180000 LAST-MODIFIED:20160418T151939Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Multi-wavelength galaxy profile fitting, and combining structural decomposition with stellar population synthesis URL;TYPE=URI:/info/1029/4807.htm END:VEVENT BEGIN:VEVENT UID:4942@kiaa.pku.edu.cn DTSTAMP:20160415T105826Z CREATED:20160415T105826Z DESCRIPTION:Quasars and dark energy DTSTART;TZID=Asia/Shanghai:20160429T120000 DTEND;TZID=Asia/Shanghai:20160429T130000 LAST-MODIFIED:20160415T105826Z LOCATION:KIAA First Floor meeting room SUMMARY:Quasars and dark energy URL;TYPE=URI:/info/1025/4942.htm END:VEVENT BEGIN:VEVENT UID:4557@kiaa.pku.edu.cn DTSTAMP:20160224T105632Z CREATED:20160224T105632Z DESCRIPTION:Neutron star equations of state: implications for cold, dense QCD DTSTART;TZID=Asia/Shanghai:20160505T160000 DTEND;TZID=Asia/Shanghai:20160505T160000 LAST-MODIFIED:20160224T105632Z LOCATION:KIAA-PKU Auditorium SUMMARY:Neutron star equations of state: implications for cold, dense QCD URL;TYPE=URI:/info/1024/4557.htm END:VEVENT BEGIN:VEVENT UID:5169@kiaa.pku.edu.cn DTSTAMP:20160302T163219Z CREATED:20160302T163219Z DESCRIPTION:The 2016 Beijing-Nanjing Bilateral Astrophysics Workshop DTSTART;TZID=Asia/Shanghai:20160509T090000 DTEND;TZID=Asia/Shanghai:20160510T170000 LAST-MODIFIED:20160302T163219Z LOCATION:Kavli Institute for Astronomy and Astrophysics, Peking University SUMMARY:The 2016 Beijing-Nanjing Bilateral Astrophysics Workshop URL;TYPE=URI:/info/1026/5169.htm END:VEVENT BEGIN:VEVENT UID:4562@kiaa.pku.edu.cn DTSTAMP:20160419T085537Z CREATED:20160419T085537Z DESCRIPTION:Ensemble Mass Distribution of Galaxy Clusters from the CLASH Survey: Concentration–Mass Relation, Stacked Mass Profile, and Splashback Radius DTSTART;TZID=Asia/Shanghai:20160511T160000 DTEND;TZID=Asia/Shanghai:20160511T160000 LAST-MODIFIED:20160419T085537Z LOCATION:KIAA-PKU Auditorium SUMMARY:Ensemble Mass Distribution of Galaxy Clusters from the CLASH Survey: Concentration–Mass Relation, Stacked Mass Profile, and Splashback Radius URL;TYPE=URI:/info/1024/4562.htm END:VEVENT BEGIN:VEVENT UID:4552@kiaa.pku.edu.cn DTSTAMP:20160128T110030Z CREATED:20160128T110030Z DESCRIPTION:Spirals, Gaps, and Cavities in Protoplanetary Disks: Are We Watching Planets Forming in Action? DTSTART;TZID=Asia/Shanghai:20160512T160000 DTEND;TZID=Asia/Shanghai:20160512T160000 LAST-MODIFIED:20160128T110030Z LOCATION:KIAA-PKU Auditorium SUMMARY:Spirals, Gaps, and Cavities in Protoplanetary Disks: Are We Watching Planets Forming in Action? URL;TYPE=URI:/info/1024/4552.htm END:VEVENT BEGIN:VEVENT UID:4730@kiaa.pku.edu.cn DTSTAMP:20160429T100023Z CREATED:20160429T100023Z DESCRIPTION:A Brief Introduction to James Web Space Telescope and It's main Science Goals DTSTART;TZID=Asia/Shanghai:20160517T120000 DTEND;TZID=Asia/Shanghai:20160517T130000 LAST-MODIFIED:20160429T100023Z LOCATION:KIAA-PKU SUMMARY:A Brief Introduction to James Web Space Telescope and It's main Science Goals URL;TYPE=URI:/info/1028/4730.htm END:VEVENT BEGIN:VEVENT UID:4939@kiaa.pku.edu.cn DTSTAMP:20160407T093056Z CREATED:20160407T093056Z DESCRIPTION:The AGN Population and the Cosmic X-ray Background DTSTART;TZID=Asia/Shanghai:20160518T120000 DTEND;TZID=Asia/Shanghai:20160518T130000 LAST-MODIFIED:20160407T093056Z LOCATION:KIAA First Floor Meeting Room SUMMARY:The AGN Population and the Cosmic X-ray Background URL;TYPE=URI:/info/1025/4939.htm END:VEVENT BEGIN:VEVENT UID:4554@kiaa.pku.edu.cn DTSTAMP:20160202T124637Z CREATED:20160202T124637Z DESCRIPTION:Early Galactic Nucleosynthesis of Iron-Group Elements: New Spectroscopic Constraints DTSTART;TZID=Asia/Shanghai:20160519T160000 DTEND;TZID=Asia/Shanghai:20160519T160000 LAST-MODIFIED:20160202T124637Z LOCATION:KIAA-PKU Auditorium SUMMARY:Early Galactic Nucleosynthesis of Iron-Group Elements: New Spectroscopic Constraints URL;TYPE=URI:/info/1024/4554.htm END:VEVENT BEGIN:VEVENT UID:4937@kiaa.pku.edu.cn DTSTAMP:20160330T231044Z CREATED:20160330T231044Z DESCRIPTION:Astronomy and Astrophysics at the Chinese University of Hong Kong DTSTART;TZID=Asia/Shanghai:20160520T120000 DTEND;TZID=Asia/Shanghai:20160520T130000 LAST-MODIFIED:20160330T231044Z LOCATION:KIAA, First Floor Meeting Room SUMMARY:Astronomy and Astrophysics at the Chinese University of Hong Kong URL;TYPE=URI:/info/1025/4937.htm END:VEVENT BEGIN:VEVENT UID:5168@kiaa.pku.edu.cn DTSTAMP:20160218T095115Z CREATED:20160218T095115Z DESCRIPTION:Astronomical Distance Determination in the Space Age DTSTART;TZID=Asia/Shanghai:20160523T090000 DTEND;TZID=Asia/Shanghai:20160527T170000 LAST-MODIFIED:20160218T095115Z LOCATION:ISSI-Beijing, Beijing SUMMARY:Astronomical Distance Determination in the Space Age URL;TYPE=URI:/info/1026/5168.htm END:VEVENT BEGIN:VEVENT UID:4731@kiaa.pku.edu.cn DTSTAMP:20160523T095223Z CREATED:20160523T095223Z DESCRIPTION:Pizza discussion DTSTART;TZID=Asia/Shanghai:20160524T120000 DTEND;TZID=Asia/Shanghai:20160524T130000 LAST-MODIFIED:20160523T095223Z LOCATION:KIAA-PKU SUMMARY:Pizza discussion URL;TYPE=URI:/info/1028/4731.htm END:VEVENT BEGIN:VEVENT UID:4941@kiaa.pku.edu.cn DTSTAMP:20160414T110351Z CREATED:20160414T110351Z DESCRIPTION:An unified model of supernova driven by magnetic monopoles DTSTART;TZID=Asia/Shanghai:20160525T120000 DTEND;TZID=Asia/Shanghai:20160525T130000 LAST-MODIFIED:20160414T110351Z LOCATION:KIAA First Floor Meeting Room SUMMARY:An unified model of supernova driven by magnetic monopoles URL;TYPE=URI:/info/1025/4941.htm END:VEVENT BEGIN:VEVENT UID:4553@kiaa.pku.edu.cn DTSTAMP:20160129T174412Z CREATED:20160129T174412Z DESCRIPTION:Stellar rotation and exoplanets obliquity -- What can we learn from the Kepler space mission data gold mine? DTSTART;TZID=Asia/Shanghai:20160526T160000 DTEND;TZID=Asia/Shanghai:20160526T160000 LAST-MODIFIED:20160129T174412Z LOCATION:KIAA-PKU Auditorium SUMMARY:Stellar rotation and exoplanets obliquity -- What can we learn from the Kepler space mission data gold mine? URL;TYPE=URI:/info/1024/4553.htm END:VEVENT BEGIN:VEVENT UID:4946@kiaa.pku.edu.cn DTSTAMP:20160524T132122Z CREATED:20160524T132122Z DESCRIPTION:The BEER (BEaming, Ellipsoidal, and Reflection) algorithm: How it works, Discoveries to date, and the LAMOST-BEER collaboration DTSTART;TZID=Asia/Shanghai:20160527T120000 DTEND;TZID=Asia/Shanghai:20160527T130000 LAST-MODIFIED:20160524T132122Z LOCATION:KIAA, first floor meeting room SUMMARY:The BEER (BEaming, Ellipsoidal, and Reflection) algorithm: How it works, Discoveries to date, and the LAMOST-BEER collaboration URL;TYPE=URI:/info/1025/4946.htm END:VEVENT BEGIN:VEVENT UID:4933@kiaa.pku.edu.cn DTSTAMP:20160305T162820Z CREATED:20160305T162820Z DESCRIPTION:Giant planet migration and survival on wide orbits DTSTART;TZID=Asia/Shanghai:20160530T120000 DTEND;TZID=Asia/Shanghai:20160530T130000 LAST-MODIFIED:20160305T162820Z LOCATION:DoA, Rm 2907 SUMMARY:Giant planet migration and survival on wide orbits URL;TYPE=URI:/info/1025/4933.htm END:VEVENT BEGIN:VEVENT UID:4808@kiaa.pku.edu.cn DTSTAMP:20160523T215500Z CREATED:20160523T215500Z DESCRIPTION:models of fast radio bursts DTSTART;TZID=Asia/Shanghai:20160530T170000 DTEND;TZID=Asia/Shanghai:20160530T180000 LAST-MODIFIED:20160523T215500Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:models of fast radio bursts URL;TYPE=URI:/info/1029/4808.htm END:VEVENT BEGIN:VEVENT UID:4944@kiaa.pku.edu.cn DTSTAMP:20160421T134650Z CREATED:20160421T134650Z DESCRIPTION:Tidal disruption events in the multi-wavelength era DTSTART;TZID=Asia/Shanghai:20160531T120000 DTEND;TZID=Asia/Shanghai:20160531T130000 LAST-MODIFIED:20160421T134650Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Tidal disruption events in the multi-wavelength era URL;TYPE=URI:/info/1025/4944.htm END:VEVENT BEGIN:VEVENT UID:4689@kiaa.pku.edu.cn DTSTAMP:20160527T105221Z CREATED:20160527T105221Z DESCRIPTION:Some applications of rotating MHD DTSTART;TZID=Asia/Shanghai:20160531T150000 DTEND;TZID=Asia/Shanghai:20160531T150000 LAST-MODIFIED:20160527T105221Z LOCATION:KIAA Auditorium SUMMARY:Some applications of rotating MHD URL;TYPE=URI:/info/1024/4689.htm END:VEVENT BEGIN:VEVENT UID:4558@kiaa.pku.edu.cn DTSTAMP:20160224T152436Z CREATED:20160224T152436Z DESCRIPTION:Black hole accretion and outflow DTSTART;TZID=Asia/Shanghai:20160602T160000 DTEND;TZID=Asia/Shanghai:20160602T160000 LAST-MODIFIED:20160224T152436Z LOCATION:KIAA-PKU Auditorium SUMMARY:Black hole accretion and outflow URL;TYPE=URI:/info/1024/4558.htm END:VEVENT BEGIN:VEVENT UID:6671@kiaa.pku.edu.cn DTSTAMP:20160530T102005Z CREATED:20160530T102005Z DESCRIPTION:Public talk by Edward C. Stone(Caltech): Voyager in Interstellar Space and The Universe in High Definition DTSTART;TZID=Asia/Shanghai:20160606T200000 DTEND;TZID=Asia/Shanghai:20160606T210000 LAST-MODIFIED:20160530T102005Z LOCATION: SUMMARY:Public talk by Edward C. Stone(Caltech): Voyager in Interstellar Space and The Universe in High Definition URL;TYPE=URI:/info/1089/6671.htm END:VEVENT BEGIN:VEVENT UID:5170@kiaa.pku.edu.cn DTSTAMP:20160530T141025Z CREATED:20160530T141025Z DESCRIPTION:The China-US Universities Astronomy Collaboration Summit DTSTART;TZID=Asia/Shanghai:20160607T150000 DTEND;TZID=Asia/Shanghai:20160607T150000 LAST-MODIFIED:20160530T141025Z LOCATION:Chen Shouren International Research Center, Peking University. SUMMARY:The China-US Universities Astronomy Collaboration Summit URL;TYPE=URI:/info/1026/5170.htm END:VEVENT BEGIN:VEVENT UID:4943@kiaa.pku.edu.cn DTSTAMP:20160417T210919Z CREATED:20160417T210919Z DESCRIPTION:The "TOP-SCOPE": Follow-up observations of Planck cold clumps with ground-based telescopes. DTSTART;TZID=Asia/Shanghai:20160608T120000 DTEND;TZID=Asia/Shanghai:20160608T130000 LAST-MODIFIED:20160417T210919Z LOCATION:KIAA First Floor Meeting Room SUMMARY:The "TOP-SCOPE": Follow-up observations of Planck cold clumps with ground-based telescopes. URL;TYPE=URI:/info/1025/4943.htm END:VEVENT BEGIN:VEVENT UID:4692@kiaa.pku.edu.cn DTSTAMP:20160516T142010Z CREATED:20160516T142010Z DESCRIPTION:Nearby Galaxy Mergers Seen with Adaptive Optics: A Sharper Image DTSTART;TZID=Asia/Shanghai:20160608T160000 DTEND;TZID=Asia/Shanghai:20160608T160000 LAST-MODIFIED:20160516T142010Z LOCATION:KIAA-PKU Auditorium SUMMARY:Nearby Galaxy Mergers Seen with Adaptive Optics: A Sharper Image URL;TYPE=URI:/info/1024/4692.htm END:VEVENT BEGIN:VEVENT UID:4947@kiaa.pku.edu.cn DTSTAMP:20160527T134026Z CREATED:20160527T134026Z DESCRIPTION:The Fundamental Properties of Young Stars DTSTART;TZID=Asia/Shanghai:20160609T120000 DTEND;TZID=Asia/Shanghai:20160609T130000 LAST-MODIFIED:20160527T134026Z LOCATION:KIAA, first floor meeting room. SUMMARY:The Fundamental Properties of Young Stars URL;TYPE=URI:/info/1025/4947.htm END:VEVENT BEGIN:VEVENT UID:4951@kiaa.pku.edu.cn DTSTAMP:20160608T174012Z CREATED:20160608T174012Z DESCRIPTION:Potential Effects of Accretion-Disk Neutrinos on High-Energy Neutrinos Produced in Gamma-Ray Bursts and Core-Collapse Supernovae DTSTART;TZID=Asia/Shanghai:20160610T120000 DTEND;TZID=Asia/Shanghai:20160610T130000 LAST-MODIFIED:20160608T174012Z LOCATION:KIAA, first floor meeting room SUMMARY:Potential Effects of Accretion-Disk Neutrinos on High-Energy Neutrinos Produced in Gamma-Ray Bursts and Core-Collapse Supernovae URL;TYPE=URI:/info/1025/4951.htm END:VEVENT BEGIN:VEVENT UID:4809@kiaa.pku.edu.cn DTSTAMP:20160531T155820Z CREATED:20160531T155820Z DESCRIPTION:Studying high-mass star formation from observations DTSTART;TZID=Asia/Shanghai:20160610T170000 DTEND;TZID=Asia/Shanghai:20160610T180000 LAST-MODIFIED:20160531T155820Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Studying high-mass star formation from observations URL;TYPE=URI:/info/1029/4809.htm END:VEVENT BEGIN:VEVENT UID:4945@kiaa.pku.edu.cn DTSTAMP:20160516T103714Z CREATED:20160516T103714Z DESCRIPTION:Electromagnetic Counterparts of Neutron Star Mergers - Past and Future DTSTART;TZID=Asia/Shanghai:20160613T120000 DTEND;TZID=Asia/Shanghai:20160613T130000 LAST-MODIFIED:20160516T103714Z LOCATION:DoA, Rm 2907 SUMMARY:Electromagnetic Counterparts of Neutron Star Mergers - Past and Future URL;TYPE=URI:/info/1025/4945.htm END:VEVENT BEGIN:VEVENT UID:4949@kiaa.pku.edu.cn DTSTAMP:20160607T105252Z CREATED:20160607T105252Z DESCRIPTION:Modeling the large-scale gas features of the Milky Way DTSTART;TZID=Asia/Shanghai:20160615T120000 DTEND;TZID=Asia/Shanghai:20160615T130000 LAST-MODIFIED:20160607T105252Z LOCATION:KIAA, First Floor Meeting Room SUMMARY:Modeling the large-scale gas features of the Milky Way URL;TYPE=URI:/info/1025/4949.htm END:VEVENT BEGIN:VEVENT UID:4940@kiaa.pku.edu.cn DTSTAMP:20160414T093858Z CREATED:20160414T093858Z DESCRIPTION:The Dharma Planet Survey of Rocky Planets around Nearby Solar Type Stars DTSTART;TZID=Asia/Shanghai:20160616T120000 DTEND;TZID=Asia/Shanghai:20160616T130000 LAST-MODIFIED:20160414T093858Z LOCATION:KIAA First floor meeting room SUMMARY:The Dharma Planet Survey of Rocky Planets around Nearby Solar Type Stars URL;TYPE=URI:/info/1025/4940.htm END:VEVENT BEGIN:VEVENT UID:4691@kiaa.pku.edu.cn DTSTAMP:20160516T194213Z CREATED:20160516T194213Z DESCRIPTION:Detection of the missing baryons with thermal and kinetic Sunyaev-Zeldovich effect DTSTART;TZID=Asia/Shanghai:20160616T160000 DTEND;TZID=Asia/Shanghai:20160616T160000 LAST-MODIFIED:20160516T194213Z LOCATION:KIAA-PKU Auditorium SUMMARY:Detection of the missing baryons with thermal and kinetic Sunyaev-Zeldovich effect URL;TYPE=URI:/info/1024/4691.htm END:VEVENT BEGIN:VEVENT UID:4810@kiaa.pku.edu.cn DTSTAMP:20160615T230347Z CREATED:20160615T230347Z DESCRIPTION:Practice Talk for Thesis Proposal DTSTART;TZID=Asia/Shanghai:20160616T180000 DTEND;TZID=Asia/Shanghai:20160616T200000 LAST-MODIFIED:20160615T230347Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Practice Talk for Thesis Proposal URL;TYPE=URI:/info/1029/4810.htm END:VEVENT BEGIN:VEVENT UID:4690@kiaa.pku.edu.cn DTSTAMP:20160516T201043Z CREATED:20160516T201043Z DESCRIPTION:Gamma-Ray Bursts in the Last Observing Window: the >10 GeV Energy Band DTSTART;TZID=Asia/Shanghai:20160623T160000 DTEND;TZID=Asia/Shanghai:20160623T160000 LAST-MODIFIED:20160516T201043Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gamma-Ray Bursts in the Last Observing Window: the >10 GeV Energy Band URL;TYPE=URI:/info/1024/4690.htm END:VEVENT BEGIN:VEVENT UID:6672@kiaa.pku.edu.cn DTSTAMP:20160623T084655Z CREATED:20160623T084655Z DESCRIPTION:The First AST (Ali Six-point-five-meter Telescope) Workshop DTSTART;TZID=Asia/Shanghai:20160703T130000 DTEND;TZID=Asia/Shanghai:20160703T180000 LAST-MODIFIED:20160623T084655Z LOCATION:KIAA Auditorium SUMMARY:The First AST (Ali Six-point-five-meter Telescope) Workshop URL;TYPE=URI:/info/1089/6672.htm END:VEVENT BEGIN:VEVENT UID:5171@kiaa.pku.edu.cn DTSTAMP:20160630T114323Z CREATED:20160630T114323Z DESCRIPTION:MOST project meeting DTSTART;TZID=Asia/Shanghai:20160704T090000 DTEND;TZID=Asia/Shanghai:20160704T120000 LAST-MODIFIED:20160630T114323Z LOCATION:KIAA SUMMARY:MOST project meeting URL;TYPE=URI:/info/1026/5171.htm END:VEVENT BEGIN:VEVENT UID:4688@kiaa.pku.edu.cn DTSTAMP:20160527T113139Z CREATED:20160527T113139Z DESCRIPTION:Mysteries of cosmic high-energy neutrinos DTSTART;TZID=Asia/Shanghai:20160707T160000 DTEND;TZID=Asia/Shanghai:20160707T160000 LAST-MODIFIED:20160527T113139Z LOCATION:KIAA-PKU Auditorium SUMMARY:Mysteries of cosmic high-energy neutrinos URL;TYPE=URI:/info/1024/4688.htm END:VEVENT BEGIN:VEVENT UID:4950@kiaa.pku.edu.cn DTSTAMP:20160608T085226Z CREATED:20160608T085226Z DESCRIPTION:Science at Low Frequencies with the Long Wavelength Array DTSTART;TZID=Asia/Shanghai:20160708T120000 DTEND;TZID=Asia/Shanghai:20160708T130000 LAST-MODIFIED:20160608T085226Z LOCATION:KIAA First Floor Meeting Room SUMMARY:Science at Low Frequencies with the Long Wavelength Array URL;TYPE=URI:/info/1025/4950.htm END:VEVENT BEGIN:VEVENT UID:4952@kiaa.pku.edu.cn DTSTAMP:20160711T142148Z CREATED:20160711T142148Z DESCRIPTION:Milky Way Dust in 3D DTSTART;TZID=Asia/Shanghai:20160714T120000 DTEND;TZID=Asia/Shanghai:20160714T130000 LAST-MODIFIED:20160711T142148Z LOCATION:KIAA First Floor Classroom SUMMARY:Milky Way Dust in 3D URL;TYPE=URI:/info/1025/4952.htm END:VEVENT BEGIN:VEVENT UID:4953@kiaa.pku.edu.cn DTSTAMP:20160713T155252Z CREATED:20160713T155252Z DESCRIPTION:Rocky Planet Interiors DTSTART;TZID=Asia/Shanghai:20160725T120000 DTEND;TZID=Asia/Shanghai:20160725T130000 LAST-MODIFIED:20160713T155252Z LOCATION:KIAA,first floor meeting room SUMMARY:Rocky Planet Interiors URL;TYPE=URI:/info/1025/4953.htm END:VEVENT BEGIN:VEVENT UID:4561@kiaa.pku.edu.cn DTSTAMP:20160414T092415Z CREATED:20160414T092415Z DESCRIPTION:PAHs in Astrophysics DTSTART;TZID=Asia/Shanghai:20160804T160000 DTEND;TZID=Asia/Shanghai:20160804T160000 LAST-MODIFIED:20160414T092415Z LOCATION:KIAA-PKU Auditorium SUMMARY:PAHs in Astrophysics URL;TYPE=URI:/info/1024/4561.htm END:VEVENT BEGIN:VEVENT UID:4954@kiaa.pku.edu.cn DTSTAMP:20160728T091455Z CREATED:20160728T091455Z DESCRIPTION:The Gravitational Wave Astronomy Era: From the first detections on Earth to space observatories DTSTART;TZID=Asia/Shanghai:20160805T120000 DTEND;TZID=Asia/Shanghai:20160805T130000 LAST-MODIFIED:20160728T091455Z LOCATION:KIAA, first floor meeting room SUMMARY:The Gravitational Wave Astronomy Era: From the first detections on Earth to space observatories URL;TYPE=URI:/info/1025/4954.htm END:VEVENT BEGIN:VEVENT UID:3892@kiaa.pku.edu.cn DTSTAMP:20160811T102012Z CREATED:20160811T102012Z DESCRIPTION:Agenda for visit by Chilean Delegation DTSTART;TZID=Asia/Shanghai:20160901T103000 DTEND;TZID=Asia/Shanghai:20160901T130000 LAST-MODIFIED:20160811T102012Z LOCATION:First Meeting Room, KIAA-PKU SUMMARY:Agenda for visit by Chilean Delegation URL;TYPE=URI:/info/1030/3892.htm END:VEVENT BEGIN:VEVENT UID:4563@kiaa.pku.edu.cn DTSTAMP:20160503T235915Z CREATED:20160503T235915Z DESCRIPTION:The early (feedback-regulated) growth of supermassive black holes DTSTART;TZID=Asia/Shanghai:20160901T160000 DTEND;TZID=Asia/Shanghai:20160901T160000 LAST-MODIFIED:20160503T235915Z LOCATION:KIAA-PKU Auditorium SUMMARY:The early (feedback-regulated) growth of supermassive black holes URL;TYPE=URI:/info/1024/4563.htm END:VEVENT BEGIN:VEVENT UID:4948@kiaa.pku.edu.cn DTSTAMP:20160529T180445Z CREATED:20160529T180445Z DESCRIPTION:Weak lensing in the nonlinear regime DTSTART;TZID=Asia/Shanghai:20160905T120000 DTEND;TZID=Asia/Shanghai:20160905T130000 LAST-MODIFIED:20160529T180445Z LOCATION:DoA, Rm 2907 SUMMARY:Weak lensing in the nonlinear regime URL;TYPE=URI:/info/1025/4948.htm END:VEVENT BEGIN:VEVENT UID:4732@kiaa.pku.edu.cn DTSTAMP:20160829T203315Z CREATED:20160829T203315Z DESCRIPTION:General Discussion DTSTART;TZID=Asia/Shanghai:20160906T120000 DTEND;TZID=Asia/Shanghai:20160906T130000 LAST-MODIFIED:20160829T203315Z LOCATION:KIAA-PKU SUMMARY:General Discussion URL;TYPE=URI:/info/1028/4732.htm END:VEVENT BEGIN:VEVENT UID:4956@kiaa.pku.edu.cn DTSTAMP:20160824T104835Z CREATED:20160824T104835Z DESCRIPTION:Measuring fundamental properties of young stars DTSTART;TZID=Asia/Shanghai:20160907T120000 DTEND;TZID=Asia/Shanghai:20160907T130000 LAST-MODIFIED:20160824T104835Z LOCATION:KIAA first floor meeting room SUMMARY:Measuring fundamental properties of young stars URL;TYPE=URI:/info/1025/4956.htm END:VEVENT BEGIN:VEVENT UID:4686@kiaa.pku.edu.cn DTSTAMP:20160627T163016Z CREATED:20160627T163016Z DESCRIPTION:Hot dust-obscured galaxies: Catching the maximum accretion phase of super massive black holes DTSTART;TZID=Asia/Shanghai:20160908T160000 DTEND;TZID=Asia/Shanghai:20160908T160000 LAST-MODIFIED:20160627T163016Z LOCATION:KIAA-PKU Auditorium SUMMARY:Hot dust-obscured galaxies: Catching the maximum accretion phase of super massive black holes URL;TYPE=URI:/info/1024/4686.htm END:VEVENT BEGIN:VEVENT UID:4958@kiaa.pku.edu.cn DTSTAMP:20160905T090825Z CREATED:20160905T090825Z DESCRIPTION:Comprehensive characterisation of L subdwarfs DTSTART;TZID=Asia/Shanghai:20160909T120000 DTEND;TZID=Asia/Shanghai:20160909T130000 LAST-MODIFIED:20160905T090825Z LOCATION:KIAA first floor meeting room SUMMARY:Comprehensive characterisation of L subdwarfs URL;TYPE=URI:/info/1025/4958.htm END:VEVENT BEGIN:VEVENT UID:4955@kiaa.pku.edu.cn DTSTAMP:20160824T073117Z CREATED:20160824T073117Z DESCRIPTION:Polarized radiation from protoplanetary disk DTSTART;TZID=Asia/Shanghai:20160912T120000 DTEND;TZID=Asia/Shanghai:20160912T130000 LAST-MODIFIED:20160824T073117Z LOCATION:DoA, Rm 2907 SUMMARY:Polarized radiation from protoplanetary disk URL;TYPE=URI:/info/1025/4955.htm END:VEVENT BEGIN:VEVENT UID:4960@kiaa.pku.edu.cn DTSTAMP:20160908T153844Z CREATED:20160908T153844Z DESCRIPTION:Triple companion in gravitational wave signals DTSTART;TZID=Asia/Shanghai:20160914T120000 DTEND;TZID=Asia/Shanghai:20160914T130000 LAST-MODIFIED:20160908T153844Z LOCATION:KIAA, First floor meeting room SUMMARY:Triple companion in gravitational wave signals URL;TYPE=URI:/info/1025/4960.htm END:VEVENT BEGIN:VEVENT UID:4681@kiaa.pku.edu.cn DTSTAMP:20160905T095457Z CREATED:20160905T095457Z DESCRIPTION:Introduction of Laboratory Astrophysics DTSTART;TZID=Asia/Shanghai:20160922T160000 DTEND;TZID=Asia/Shanghai:20160922T160000 LAST-MODIFIED:20160905T095457Z LOCATION:KIAA-PKU Auditorium SUMMARY:Introduction of Laboratory Astrophysics URL;TYPE=URI:/info/1024/4681.htm END:VEVENT BEGIN:VEVENT UID:4957@kiaa.pku.edu.cn DTSTAMP:20160902T092843Z CREATED:20160902T092843Z DESCRIPTION:White dwarfs from SDSS and LAMOST DTSTART;TZID=Asia/Shanghai:20160926T120000 DTEND;TZID=Asia/Shanghai:20160926T130000 LAST-MODIFIED:20160902T092843Z LOCATION:DoA, Rm 2907 SUMMARY:White dwarfs from SDSS and LAMOST URL;TYPE=URI:/info/1025/4957.htm END:VEVENT BEGIN:VEVENT UID:4687@kiaa.pku.edu.cn DTSTAMP:20160618T190416Z CREATED:20160618T190416Z DESCRIPTION:The Multiband Imaging and Slitless Spectroscopy Survey of China’s Manned Space Program DTSTART;TZID=Asia/Shanghai:20160929T160000 DTEND;TZID=Asia/Shanghai:20160929T160000 LAST-MODIFIED:20160618T190416Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Multiband Imaging and Slitless Spectroscopy Survey of China’s Manned Space Program URL;TYPE=URI:/info/1024/4687.htm END:VEVENT BEGIN:VEVENT UID:5176@kiaa.pku.edu.cn DTSTAMP:20160928T114951Z CREATED:20160928T114951Z DESCRIPTION:Black hole - Host Lifecycle Evolution (BHOLE) workshop DTSTART;TZID=Asia/Shanghai:20160930T090000 DTEND;TZID=Asia/Shanghai:20160930T163000 LAST-MODIFIED:20160928T114951Z LOCATION:KIAA auditorium SUMMARY:Black hole - Host Lifecycle Evolution (BHOLE) workshop URL;TYPE=URI:/info/1026/5176.htm END:VEVENT BEGIN:VEVENT UID:4733@kiaa.pku.edu.cn DTSTAMP:20160919T173502Z CREATED:20160919T173502Z DESCRIPTION:The LAMOST Galactic spectroscopic surveys DTSTART;TZID=Asia/Shanghai:20161011T120000 DTEND;TZID=Asia/Shanghai:20161011T130000 LAST-MODIFIED:20160919T173502Z LOCATION:KIAA-PKU SUMMARY:The LAMOST Galactic spectroscopic surveys URL;TYPE=URI:/info/1028/4733.htm END:VEVENT BEGIN:VEVENT UID:4677@kiaa.pku.edu.cn DTSTAMP:20160930T164805Z CREATED:20160930T164805Z DESCRIPTION:Multiple effect of interaction between supernova remnants and molecular clouds DTSTART;TZID=Asia/Shanghai:20161013T160000 DTEND;TZID=Asia/Shanghai:20161013T160000 LAST-MODIFIED:20160930T164805Z LOCATION:KIAA-PKU Auditorium SUMMARY:Multiple effect of interaction between supernova remnants and molecular clouds URL;TYPE=URI:/info/1024/4677.htm END:VEVENT BEGIN:VEVENT UID:4959@kiaa.pku.edu.cn DTSTAMP:20160907T134813Z CREATED:20160907T134813Z DESCRIPTION:On the Statistical Equivalence of the Large-scale Structure DTSTART;TZID=Asia/Shanghai:20161017T120000 DTEND;TZID=Asia/Shanghai:20161017T130000 LAST-MODIFIED:20160907T134813Z LOCATION:DoA, Rm 2907 SUMMARY:On the Statistical Equivalence of the Large-scale Structure URL;TYPE=URI:/info/1025/4959.htm END:VEVENT BEGIN:VEVENT UID:4685@kiaa.pku.edu.cn DTSTAMP:20160705T174335Z CREATED:20160705T174335Z DESCRIPTION:A Good Hard Look at Growing Supermassive Black Holes in the Distant Universe DTSTART;TZID=Asia/Shanghai:20161020T160000 DTEND;TZID=Asia/Shanghai:20161020T160000 LAST-MODIFIED:20160705T174335Z LOCATION:KIAA-PKU Auditorium SUMMARY:A Good Hard Look at Growing Supermassive Black Holes in the Distant Universe URL;TYPE=URI:/info/1024/4685.htm END:VEVENT BEGIN:VEVENT UID:4961@kiaa.pku.edu.cn DTSTAMP:20161007T145429Z CREATED:20161007T145429Z DESCRIPTION:Stellar populations in young star clusters DTSTART;TZID=Asia/Shanghai:20161024T120000 DTEND;TZID=Asia/Shanghai:20161024T130000 LAST-MODIFIED:20161007T145429Z LOCATION:DoA, Rm 2907 SUMMARY:Stellar populations in young star clusters URL;TYPE=URI:/info/1025/4961.htm END:VEVENT BEGIN:VEVENT UID:4734@kiaa.pku.edu.cn DTSTAMP:20160919T173547Z CREATED:20160919T173547Z DESCRIPTION:Lagrangian Space Nonlinear E-mode clustering DTSTART;TZID=Asia/Shanghai:20161025T120000 DTEND;TZID=Asia/Shanghai:20161025T130000 LAST-MODIFIED:20160919T173547Z LOCATION:KIAA-PKU SUMMARY:Lagrangian Space Nonlinear E-mode clustering URL;TYPE=URI:/info/1028/4734.htm END:VEVENT BEGIN:VEVENT UID:4811@kiaa.pku.edu.cn DTSTAMP:20161015T022909Z CREATED:20161015T022909Z DESCRIPTION:Practice Talking for CAS meeting (cancled) DTSTART;TZID=Asia/Shanghai:20161025T170000 DTEND;TZID=Asia/Shanghai:20161025T180000 LAST-MODIFIED:20161015T022909Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Practice Talking for CAS meeting (cancled) URL;TYPE=URI:/info/1029/4811.htm END:VEVENT BEGIN:VEVENT UID:4963@kiaa.pku.edu.cn DTSTAMP:20161007T150921Z CREATED:20161007T150921Z DESCRIPTION:Lighting up the Universe with the First Stars, Supernovae, and Galaxies DTSTART;TZID=Asia/Shanghai:20161026T120000 DTEND;TZID=Asia/Shanghai:20161026T130000 LAST-MODIFIED:20161007T150921Z LOCATION:KIAA first floor meeting room SUMMARY:Lighting up the Universe with the First Stars, Supernovae, and Galaxies URL;TYPE=URI:/info/1025/4963.htm END:VEVENT BEGIN:VEVENT UID:4680@kiaa.pku.edu.cn DTSTAMP:20160905T152718Z CREATED:20160905T152718Z DESCRIPTION:Testing General Relativity with CMB and LSS data DTSTART;TZID=Asia/Shanghai:20161027T160000 DTEND;TZID=Asia/Shanghai:20161027T160000 LAST-MODIFIED:20160905T152718Z LOCATION:KIAA-PKU Auditorium SUMMARY:Testing General Relativity with CMB and LSS data URL;TYPE=URI:/info/1024/4680.htm END:VEVENT BEGIN:VEVENT UID:4675@kiaa.pku.edu.cn DTSTAMP:20161025T150904Z CREATED:20161025T150904Z DESCRIPTION:Pulsars and FRBs: Recent Developments DTSTART;TZID=Asia/Shanghai:20161103T160000 DTEND;TZID=Asia/Shanghai:20161103T160000 LAST-MODIFIED:20161025T150904Z LOCATION:KIAA-PKU Auditorium SUMMARY:Pulsars and FRBs: Recent Developments URL;TYPE=URI:/info/1024/4675.htm END:VEVENT BEGIN:VEVENT UID:4967@kiaa.pku.edu.cn DTSTAMP:20161102T212237Z CREATED:20161102T212237Z DESCRIPTION:The role of vortices in multi-dimensional protoplanetary disks DTSTART;TZID=Asia/Shanghai:20161107T120000 DTEND;TZID=Asia/Shanghai:20161107T130000 LAST-MODIFIED:20161102T212237Z LOCATION:1st meeting room, KIAA SUMMARY:The role of vortices in multi-dimensional protoplanetary disks URL;TYPE=URI:/info/1025/4967.htm END:VEVENT BEGIN:VEVENT UID:4683@kiaa.pku.edu.cn DTSTAMP:20160715T110257Z CREATED:20160715T110257Z DESCRIPTION:What Determines Star Formation Rates? DTSTART;TZID=Asia/Shanghai:20161108T160000 DTEND;TZID=Asia/Shanghai:20161108T160000 LAST-MODIFIED:20160715T110257Z LOCATION:KIAA-PKU Auditorium SUMMARY:What Determines Star Formation Rates? URL;TYPE=URI:/info/1024/4683.htm END:VEVENT BEGIN:VEVENT UID:5175@kiaa.pku.edu.cn DTSTAMP:20160919T084630Z CREATED:20160919T084630Z DESCRIPTION:The 2016 KIAA-PKU Astrophysics Forum: Future Large Optical-Infrared Facilities in China DTSTART;TZID=Asia/Shanghai:20161110T084500 DTEND;TZID=Asia/Shanghai:20161111T180000 LAST-MODIFIED:20160919T084630Z LOCATION:KIAA Auditorium SUMMARY:The 2016 KIAA-PKU Astrophysics Forum: Future Large Optical-Infrared Facilities in China URL;TYPE=URI:/info/1026/5175.htm END:VEVENT BEGIN:VEVENT UID:4969@kiaa.pku.edu.cn DTSTAMP:20161108T150620Z CREATED:20161108T150620Z DESCRIPTION:MOCCA Code for Star Cluster Simulations and the SURVEY Database I Projects DTSTART;TZID=Asia/Shanghai:20161114T120000 DTEND;TZID=Asia/Shanghai:20161114T130000 LAST-MODIFIED:20161108T150620Z LOCATION:DoA, Rm 2907 SUMMARY:MOCCA Code for Star Cluster Simulations and the SURVEY Database I Projects URL;TYPE=URI:/info/1025/4969.htm END:VEVENT BEGIN:VEVENT UID:4736@kiaa.pku.edu.cn DTSTAMP:20160919T173717Z CREATED:20160919T173717Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20161115T120000 DTEND;TZID=Asia/Shanghai:20161115T130000 LAST-MODIFIED:20160919T173717Z LOCATION:KIAA-PKU SUMMARY:TBD URL;TYPE=URI:/info/1028/4736.htm END:VEVENT BEGIN:VEVENT UID:4679@kiaa.pku.edu.cn DTSTAMP:20160907T092320Z CREATED:20160907T092320Z DESCRIPTION:Star formation rates and luminosity functions in the low-redshift Universe DTSTART;TZID=Asia/Shanghai:20161117T160000 DTEND;TZID=Asia/Shanghai:20161117T160000 LAST-MODIFIED:20160907T092320Z LOCATION:KIAA-PKU Auditorium SUMMARY:Star formation rates and luminosity functions in the low-redshift Universe URL;TYPE=URI:/info/1024/4679.htm END:VEVENT BEGIN:VEVENT UID:4735@kiaa.pku.edu.cn DTSTAMP:20160919T173636Z CREATED:20160919T173636Z DESCRIPTION:Low mass stellar population in HII region environments DTSTART;TZID=Asia/Shanghai:20161122T120000 DTEND;TZID=Asia/Shanghai:20161122T130000 LAST-MODIFIED:20160919T173636Z LOCATION:KIAA-PKU SUMMARY:Low mass stellar population in HII region environments URL;TYPE=URI:/info/1028/4735.htm END:VEVENT BEGIN:VEVENT UID:4970@kiaa.pku.edu.cn DTSTAMP:20161122T102327Z CREATED:20161122T102327Z DESCRIPTION:Galaxy Quenching, Color Conformity, and Halo Assembly Bias DTSTART;TZID=Asia/Shanghai:20161123T120000 DTEND;TZID=Asia/Shanghai:20161123T130000 LAST-MODIFIED:20161122T102327Z LOCATION:KIAA: First floor meeting room SUMMARY:Galaxy Quenching, Color Conformity, and Halo Assembly Bias URL;TYPE=URI:/info/1025/4970.htm END:VEVENT BEGIN:VEVENT UID:4670@kiaa.pku.edu.cn DTSTAMP:20161118T111919Z CREATED:20161118T111919Z DESCRIPTION:Supernova progenitors: clues from gamma-ray observations DTSTART;TZID=Asia/Shanghai:20161124T160000 DTEND;TZID=Asia/Shanghai:20161124T160000 LAST-MODIFIED:20161118T111919Z LOCATION:KIAA-PKU Auditorium SUMMARY:Supernova progenitors: clues from gamma-ray observations URL;TYPE=URI:/info/1024/4670.htm END:VEVENT BEGIN:VEVENT UID:4964@kiaa.pku.edu.cn DTSTAMP:20161017T214149Z CREATED:20161017T214149Z DESCRIPTION:Orbit distribution for 300 CALIFA galaxies DTSTART;TZID=Asia/Shanghai:20161128T120000 DTEND;TZID=Asia/Shanghai:20161128T130000 LAST-MODIFIED:20161017T214149Z LOCATION:DoA, Rm 2907 SUMMARY:Orbit distribution for 300 CALIFA galaxies URL;TYPE=URI:/info/1025/4964.htm END:VEVENT BEGIN:VEVENT UID:4968@kiaa.pku.edu.cn DTSTAMP:20161102T213042Z CREATED:20161102T213042Z DESCRIPTION:The interplay between ionized regions and star formation: recent progresses DTSTART;TZID=Asia/Shanghai:20161129T120000 DTEND;TZID=Asia/Shanghai:20161129T130000 LAST-MODIFIED:20161102T213042Z LOCATION:KIAA, first floor meeting room SUMMARY:The interplay between ionized regions and star formation: recent progresses URL;TYPE=URI:/info/1025/4968.htm END:VEVENT BEGIN:VEVENT UID:4812@kiaa.pku.edu.cn DTSTAMP:20161015T023003Z CREATED:20161015T023003Z DESCRIPTION:The Milky Way's rotation curve out to 100 kpc and its constraint on the Galactic mass distribution DTSTART;TZID=Asia/Shanghai:20161129T170000 DTEND;TZID=Asia/Shanghai:20161129T180000 LAST-MODIFIED:20161015T023003Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The Milky Way's rotation curve out to 100 kpc and its constraint on the Galactic mass distribution URL;TYPE=URI:/info/1029/4812.htm END:VEVENT BEGIN:VEVENT UID:4676@kiaa.pku.edu.cn DTSTAMP:20161011T140838Z CREATED:20161011T140838Z DESCRIPTION:"The Science of Heaven" documentary release DTSTART;TZID=Asia/Shanghai:20161130T160000 DTEND;TZID=Asia/Shanghai:20161130T160000 LAST-MODIFIED:20161011T140838Z LOCATION:KIAA-PKU Auditorium SUMMARY:"The Science of Heaven" documentary release URL;TYPE=URI:/info/1024/4676.htm END:VEVENT BEGIN:VEVENT UID:4971@kiaa.pku.edu.cn DTSTAMP:20161130T154011Z CREATED:20161130T154011Z DESCRIPTION:High Lyman Continuum Escape Fraction in a Lensed Compact Dwarf Galaxy at Z=2.5 DTSTART;TZID=Asia/Shanghai:20161201T120000 DTEND;TZID=Asia/Shanghai:20161201T130000 LAST-MODIFIED:20161130T154011Z LOCATION:KIAA, first floor meeting room SUMMARY:High Lyman Continuum Escape Fraction in a Lensed Compact Dwarf Galaxy at Z=2.5 URL;TYPE=URI:/info/1025/4971.htm END:VEVENT BEGIN:VEVENT UID:4684@kiaa.pku.edu.cn DTSTAMP:20160712T234107Z CREATED:20160712T234107Z DESCRIPTION:Reconstructing the actual local universe DTSTART;TZID=Asia/Shanghai:20161201T160000 DTEND;TZID=Asia/Shanghai:20161201T160000 LAST-MODIFIED:20160712T234107Z LOCATION:KIAA-PKU Auditorium SUMMARY:Reconstructing the actual local universe URL;TYPE=URI:/info/1024/4684.htm END:VEVENT BEGIN:VEVENT UID:4965@kiaa.pku.edu.cn DTSTAMP:20161026T112236Z CREATED:20161026T112236Z DESCRIPTION:The Impact of B-fields on Thermal Instability DTSTART;TZID=Asia/Shanghai:20161206T120000 DTEND;TZID=Asia/Shanghai:20161206T130000 LAST-MODIFIED:20161026T112236Z LOCATION:1st meeting room, KIAA SUMMARY:The Impact of B-fields on Thermal Instability URL;TYPE=URI:/info/1025/4965.htm END:VEVENT BEGIN:VEVENT UID:4671@kiaa.pku.edu.cn DTSTAMP:20161111T121502Z CREATED:20161111T121502Z DESCRIPTION:Observations and Modelings of Solar Coronal Waves DTSTART;TZID=Asia/Shanghai:20161208T160000 DTEND;TZID=Asia/Shanghai:20161208T160000 LAST-MODIFIED:20161111T121502Z LOCATION:KIAA-PKU Auditorium SUMMARY:Observations and Modelings of Solar Coronal Waves URL;TYPE=URI:/info/1024/4671.htm END:VEVENT BEGIN:VEVENT UID:5178@kiaa.pku.edu.cn DTSTAMP:20161013T134855Z CREATED:20161013T134855Z DESCRIPTION:2016 Postdoc Forum DTSTART;TZID=Asia/Shanghai:20161212T090000 DTEND;TZID=Asia/Shanghai:20161212T180000 LAST-MODIFIED:20161013T134855Z LOCATION:KIAA Auditorium SUMMARY:2016 Postdoc Forum URL;TYPE=URI:/info/1026/5178.htm END:VEVENT BEGIN:VEVENT UID:5174@kiaa.pku.edu.cn DTSTAMP:20160913T102758Z CREATED:20160913T102758Z DESCRIPTION:Workshop for follow-up surveys of Planck Galactic Cold Clumps DTSTART;TZID=Asia/Shanghai:20161213T083000 DTEND;TZID=Asia/Shanghai:20161215T180000 LAST-MODIFIED:20160913T102758Z LOCATION:KIAA Auditorium SUMMARY:Workshop for follow-up surveys of Planck Galactic Cold Clumps URL;TYPE=URI:/info/1026/5174.htm END:VEVENT BEGIN:VEVENT UID:4966@kiaa.pku.edu.cn DTSTAMP:20161028T104932Z CREATED:20161028T104932Z DESCRIPTION:Cosmic Mammoth - Map the Most Massive Large-scale Structures in early Universe DTSTART;TZID=Asia/Shanghai:20161213T120000 DTEND;TZID=Asia/Shanghai:20161213T130000 LAST-MODIFIED:20161028T104932Z LOCATION:KIAA First floor meeting room SUMMARY:Cosmic Mammoth - Map the Most Massive Large-scale Structures in early Universe URL;TYPE=URI:/info/1025/4966.htm END:VEVENT BEGIN:VEVENT UID:4962@kiaa.pku.edu.cn DTSTAMP:20161007T150030Z CREATED:20161007T150030Z DESCRIPTION:Black Holes Grow More Efficiently in Massive Galaxies DTSTART;TZID=Asia/Shanghai:20161214T120000 DTEND;TZID=Asia/Shanghai:20161214T130000 LAST-MODIFIED:20161007T150030Z LOCATION:KIAA first floor meeting room SUMMARY:Black Holes Grow More Efficiently in Massive Galaxies URL;TYPE=URI:/info/1025/4962.htm END:VEVENT BEGIN:VEVENT UID:4673@kiaa.pku.edu.cn DTSTAMP:20161028T174439Z CREATED:20161028T174439Z DESCRIPTION:Planting seeds for gravitational wave generators around active galactic nuclei: Analog of planetary systems around massive black holes DTSTART;TZID=Asia/Shanghai:20161215T160000 DTEND;TZID=Asia/Shanghai:20161215T160000 LAST-MODIFIED:20161028T174439Z LOCATION:KIAA-PKU first-floor meeting room SUMMARY:Planting seeds for gravitational wave generators around active galactic nuclei: Analog of planetary systems around massive black holes URL;TYPE=URI:/info/1024/4673.htm END:VEVENT BEGIN:VEVENT UID:6673@kiaa.pku.edu.cn DTSTAMP:20161216T134813Z CREATED:20161216T134813Z DESCRIPTION:New Year Party of PKU astronomy family DTSTART;TZID=Asia/Shanghai:20161216T183000 DTEND;TZID=Asia/Shanghai:20161216T220000 LAST-MODIFIED:20161216T134813Z LOCATION:KIAA auditorium SUMMARY:New Year Party of PKU astronomy family URL;TYPE=URI:/info/1089/6673.htm END:VEVENT BEGIN:VEVENT UID:5179@kiaa.pku.edu.cn DTSTAMP:20161212T150007Z CREATED:20161212T150007Z DESCRIPTION:8th Kazakhstan-China-Korea (KCK) workshop on stellar dynamics and related fields DTSTART;TZID=Asia/Shanghai:20161219T100000 DTEND;TZID=Asia/Shanghai:20161221T123000 LAST-MODIFIED:20161212T150007Z LOCATION:Kunming, Yunnan SUMMARY:8th Kazakhstan-China-Korea (KCK) workshop on stellar dynamics and related fields URL;TYPE=URI:/info/1026/5179.htm END:VEVENT BEGIN:VEVENT UID:4737@kiaa.pku.edu.cn DTSTAMP:20160919T173829Z CREATED:20160919T173829Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20161220T120000 DTEND;TZID=Asia/Shanghai:20161220T130000 LAST-MODIFIED:20160919T173829Z LOCATION:KIAA-PKU SUMMARY:TBD URL;TYPE=URI:/info/1028/4737.htm END:VEVENT BEGIN:VEVENT UID:4813@kiaa.pku.edu.cn DTSTAMP:20161217T220132Z CREATED:20161217T220132Z DESCRIPTION:Coevolution of supermassive black holes and host galaxies in AGNs DTSTART;TZID=Asia/Shanghai:20161220T170000 DTEND;TZID=Asia/Shanghai:20161220T180000 LAST-MODIFIED:20161217T220132Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Coevolution of supermassive black holes and host galaxies in AGNs URL;TYPE=URI:/info/1029/4813.htm END:VEVENT BEGIN:VEVENT UID:5180@kiaa.pku.edu.cn DTSTAMP:20161216T103857Z CREATED:20161216T103857Z DESCRIPTION:2016 Graduate Students Annual Report DTSTART;TZID=Asia/Shanghai:20161226T080000 DTEND;TZID=Asia/Shanghai:20161226T173000 LAST-MODIFIED:20161216T103857Z LOCATION:KIAA auditorium SUMMARY:2016 Graduate Students Annual Report URL;TYPE=URI:/info/1026/5180.htm END:VEVENT BEGIN:VEVENT UID:4674@kiaa.pku.edu.cn DTSTAMP:20161028T113039Z CREATED:20161028T113039Z DESCRIPTION:Gravitational Wave Astrophysics - Simulations and Observations DTSTART;TZID=Asia/Shanghai:20161229T160000 DTEND;TZID=Asia/Shanghai:20161229T160000 LAST-MODIFIED:20161028T113039Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gravitational Wave Astrophysics - Simulations and Observations URL;TYPE=URI:/info/1024/4674.htm END:VEVENT BEGIN:VEVENT UID:4672@kiaa.pku.edu.cn DTSTAMP:20161107T155257Z CREATED:20161107T155257Z DESCRIPTION:The 21 cm cosmology and cosmic reionization simulations DTSTART;TZID=Asia/Shanghai:20170105T160000 DTEND;TZID=Asia/Shanghai:20170105T160000 LAST-MODIFIED:20161107T155257Z LOCATION:KIAA-PKU Auditorium SUMMARY:The 21 cm cosmology and cosmic reionization simulations URL;TYPE=URI:/info/1024/4672.htm END:VEVENT BEGIN:VEVENT UID:4973@kiaa.pku.edu.cn DTSTAMP:20161230T155017Z CREATED:20161230T155017Z DESCRIPTION:Discovery of the most distant X-ray galaxy cluster in the universe, and its implications on galaxy formation and cosmology DTSTART;TZID=Asia/Shanghai:20170106T120000 DTEND;TZID=Asia/Shanghai:20170106T130000 LAST-MODIFIED:20161230T155017Z LOCATION:KIAA 1st meeting room SUMMARY:Discovery of the most distant X-ray galaxy cluster in the universe, and its implications on galaxy formation and cosmology URL;TYPE=URI:/info/1025/4973.htm END:VEVENT BEGIN:VEVENT UID:4739@kiaa.pku.edu.cn DTSTAMP:20160919T173959Z CREATED:20160919T173959Z DESCRIPTION:Science wth the cosmic background - an example from X-rays DTSTART;TZID=Asia/Shanghai:20170110T120000 DTEND;TZID=Asia/Shanghai:20170110T130000 LAST-MODIFIED:20160919T173959Z LOCATION:KIAA-PKU SUMMARY:Science wth the cosmic background - an example from X-rays URL;TYPE=URI:/info/1028/4739.htm END:VEVENT BEGIN:VEVENT UID:4778@kiaa.pku.edu.cn DTSTAMP:20170111T112220Z CREATED:20170111T112220Z DESCRIPTION:Pizza Discussion DTSTART;TZID=Asia/Shanghai:20170112T120000 DTEND;TZID=Asia/Shanghai:20170112T130000 LAST-MODIFIED:20170111T112220Z LOCATION:KIAA-PKU SUMMARY:Pizza Discussion URL;TYPE=URI:/info/1028/4778.htm END:VEVENT BEGIN:VEVENT UID:5181@kiaa.pku.edu.cn DTSTAMP:20161216T114449Z CREATED:20161216T114449Z DESCRIPTION:Bilateral workshop between KIAA-PKU and Instituto de Astrofisica, PUC DTSTART;TZID=Asia/Shanghai:20170213T090000 DTEND;TZID=Asia/Shanghai:20170217T060000 LAST-MODIFIED:20161216T114449Z LOCATION:KIAA SUMMARY:Bilateral workshop between KIAA-PKU and Instituto de Astrofisica, PUC URL;TYPE=URI:/info/1026/5181.htm END:VEVENT BEGIN:VEVENT UID:4775@kiaa.pku.edu.cn DTSTAMP:20170219T102541Z CREATED:20170219T102541Z DESCRIPTION:Roland de Putter: Pizza lunch with postdocs DTSTART;TZID=Asia/Shanghai:20170220T120000 DTEND;TZID=Asia/Shanghai:20170220T130000 LAST-MODIFIED:20170219T102541Z LOCATION:2nd meeting room, KIAA SUMMARY:Roland de Putter: Pizza lunch with postdocs URL;TYPE=URI:/info/1028/4775.htm END:VEVENT BEGIN:VEVENT UID:4980@kiaa.pku.edu.cn DTSTAMP:20170219T102157Z CREATED:20170219T102157Z DESCRIPTION:Xuening Bai: Lunch with grad students DTSTART;TZID=Asia/Shanghai:20170220T120000 DTEND;TZID=Asia/Shanghai:20170220T130000 LAST-MODIFIED:20170219T102157Z LOCATION:1st meeting room, KIAA SUMMARY:Xuening Bai: Lunch with grad students URL;TYPE=URI:/info/1025/4980.htm END:VEVENT BEGIN:VEVENT UID:4668@kiaa.pku.edu.cn DTSTAMP:20170218T181325Z CREATED:20170218T181325Z DESCRIPTION:Probing Inflation and more with cosmic large-scale structure DTSTART;TZID=Asia/Shanghai:20170220T160000 DTEND;TZID=Asia/Shanghai:20170220T170000 LAST-MODIFIED:20170218T181325Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing Inflation and more with cosmic large-scale structure URL;TYPE=URI:/info/1024/4668.htm END:VEVENT BEGIN:VEVENT UID:4981@kiaa.pku.edu.cn DTSTAMP:20170219T102713Z CREATED:20170219T102713Z DESCRIPTION:Roland de Putter: Lunch with grad students DTSTART;TZID=Asia/Shanghai:20170221T120000 DTEND;TZID=Asia/Shanghai:20170221T130000 LAST-MODIFIED:20170219T102713Z LOCATION:1st meeting room SUMMARY:Roland de Putter: Lunch with grad students URL;TYPE=URI:/info/1025/4981.htm END:VEVENT BEGIN:VEVENT UID:4777@kiaa.pku.edu.cn DTSTAMP:20170219T101816Z CREATED:20170219T101816Z DESCRIPTION:Lixin Dai: Pizza lunch with Postdocs DTSTART;TZID=Asia/Shanghai:20170221T120000 DTEND;TZID=Asia/Shanghai:20170221T130000 LAST-MODIFIED:20170219T101816Z LOCATION:2nd meeting room, KIAA SUMMARY:Lixin Dai: Pizza lunch with Postdocs URL;TYPE=URI:/info/1028/4777.htm END:VEVENT BEGIN:VEVENT UID:4666@kiaa.pku.edu.cn DTSTAMP:20170218T182024Z CREATED:20170218T182024Z DESCRIPTION:Protoplanetary Disks and Planet Formation: A Microphysical Perspective DTSTART;TZID=Asia/Shanghai:20170221T160000 DTEND;TZID=Asia/Shanghai:20170221T170000 LAST-MODIFIED:20170218T182024Z LOCATION:KIAA-PKU Auditorium SUMMARY:Protoplanetary Disks and Planet Formation: A Microphysical Perspective URL;TYPE=URI:/info/1024/4666.htm END:VEVENT BEGIN:VEVENT UID:4776@kiaa.pku.edu.cn DTSTAMP:20170219T102337Z CREATED:20170219T102337Z DESCRIPTION:Xuening Bai: Pizza Lunch with postdocs DTSTART;TZID=Asia/Shanghai:20170222T120000 DTEND;TZID=Asia/Shanghai:20170222T130000 LAST-MODIFIED:20170219T102337Z LOCATION:2nd meeting room, KIAA SUMMARY:Xuening Bai: Pizza Lunch with postdocs URL;TYPE=URI:/info/1028/4776.htm END:VEVENT BEGIN:VEVENT UID:4979@kiaa.pku.edu.cn DTSTAMP:20170219T102046Z CREATED:20170219T102046Z DESCRIPTION:Lixin Dai: Lunch with grad students DTSTART;TZID=Asia/Shanghai:20170222T120000 DTEND;TZID=Asia/Shanghai:20170222T130000 LAST-MODIFIED:20170219T102046Z LOCATION:1st meeting room, KIAA SUMMARY:Lixin Dai: Lunch with grad students URL;TYPE=URI:/info/1025/4979.htm END:VEVENT BEGIN:VEVENT UID:4667@kiaa.pku.edu.cn DTSTAMP:20170218T181859Z CREATED:20170218T181859Z DESCRIPTION:Probing super-Eddington accretion via tidal disruption events DTSTART;TZID=Asia/Shanghai:20170222T160000 DTEND;TZID=Asia/Shanghai:20170222T170000 LAST-MODIFIED:20170218T181859Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing super-Eddington accretion via tidal disruption events URL;TYPE=URI:/info/1024/4667.htm END:VEVENT BEGIN:VEVENT UID:4977@kiaa.pku.edu.cn DTSTAMP:20170215T184753Z CREATED:20170215T184753Z DESCRIPTION:UniDAM -- A Unified tool to estimate stellar distances, ages and masses from spectrophotometric data DTSTART;TZID=Asia/Shanghai:20170223T120000 DTEND;TZID=Asia/Shanghai:20170223T130000 LAST-MODIFIED:20170215T184753Z LOCATION:KIAA meeting room SUMMARY:UniDAM -- A Unified tool to estimate stellar distances, ages and masses from spectrophotometric data URL;TYPE=URI:/info/1025/4977.htm END:VEVENT BEGIN:VEVENT UID:4682@kiaa.pku.edu.cn DTSTAMP:20160719T152551Z CREATED:20160719T152551Z DESCRIPTION:Organic Matter in the Universe: from solar system to distant galaxies DTSTART;TZID=Asia/Shanghai:20170223T160000 DTEND;TZID=Asia/Shanghai:20170223T160000 LAST-MODIFIED:20160719T152551Z LOCATION:KIAA-PKU Auditorium SUMMARY:Organic Matter in the Universe: from solar system to distant galaxies URL;TYPE=URI:/info/1024/4682.htm END:VEVENT BEGIN:VEVENT UID:5183@kiaa.pku.edu.cn DTSTAMP:20170221T172504Z CREATED:20170221T172504Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20170224T100000 DTEND;TZID=Asia/Shanghai:20170224T100000 LAST-MODIFIED:20170221T172504Z LOCATION:kiaa SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1026/5183.htm END:VEVENT BEGIN:VEVENT UID:4982@kiaa.pku.edu.cn DTSTAMP:20170222T120729Z CREATED:20170222T120729Z DESCRIPTION:Beyond turbulence: a fundamentally different mode of cluster formation in Orion DTSTART;TZID=Asia/Shanghai:20170227T120000 DTEND;TZID=Asia/Shanghai:20170227T130000 LAST-MODIFIED:20170222T120729Z LOCATION:KIAA first floor meeting room SUMMARY:Beyond turbulence: a fundamentally different mode of cluster formation in Orion URL;TYPE=URI:/info/1025/4982.htm END:VEVENT BEGIN:VEVENT UID:4738@kiaa.pku.edu.cn DTSTAMP:20160919T173922Z CREATED:20160919T173922Z DESCRIPTION:The physics learned from measuring PAHs: the stochastic heating of ultra small grains DTSTART;TZID=Asia/Shanghai:20170228T120000 DTEND;TZID=Asia/Shanghai:20170228T130000 LAST-MODIFIED:20160919T173922Z LOCATION:KIAA-PKU SUMMARY:The physics learned from measuring PAHs: the stochastic heating of ultra small grains URL;TYPE=URI:/info/1028/4738.htm END:VEVENT BEGIN:VEVENT UID:4974@kiaa.pku.edu.cn DTSTAMP:20170104T112549Z CREATED:20170104T112549Z DESCRIPTION:The Virgo intra-cluster population and the mass assembly of M87 DTSTART;TZID=Asia/Shanghai:20170301T120000 DTEND;TZID=Asia/Shanghai:20170301T130000 LAST-MODIFIED:20170104T112549Z LOCATION:KIAA first floor meeting room SUMMARY:The Virgo intra-cluster population and the mass assembly of M87 URL;TYPE=URI:/info/1025/4974.htm END:VEVENT BEGIN:VEVENT UID:4669@kiaa.pku.edu.cn DTSTAMP:20161201T213330Z CREATED:20161201T213330Z DESCRIPTION:Double SMBHs and Double TDEs DTSTART;TZID=Asia/Shanghai:20170302T160000 DTEND;TZID=Asia/Shanghai:20170302T160000 LAST-MODIFIED:20161201T213330Z LOCATION:KIAA-PKU Auditorium SUMMARY:Double SMBHs and Double TDEs URL;TYPE=URI:/info/1024/4669.htm END:VEVENT BEGIN:VEVENT UID:4972@kiaa.pku.edu.cn DTSTAMP:20161214T105140Z CREATED:20161214T105140Z DESCRIPTION:Science with the unresolved cosmic background - An example from X-rays DTSTART;TZID=Asia/Shanghai:20170303T120000 DTEND;TZID=Asia/Shanghai:20170303T130000 LAST-MODIFIED:20161214T105140Z LOCATION:KIAA first floor meeting room SUMMARY:Science with the unresolved cosmic background - An example from X-rays URL;TYPE=URI:/info/1025/4972.htm END:VEVENT BEGIN:VEVENT UID:4983@kiaa.pku.edu.cn DTSTAMP:20170224T085954Z CREATED:20170224T085954Z DESCRIPTION:New constraints on the black hole spin in radio-loud quasars DTSTART;TZID=Asia/Shanghai:20170308T120000 DTEND;TZID=Asia/Shanghai:20170308T130000 LAST-MODIFIED:20170224T085954Z LOCATION:KIAA, first floor meeting room SUMMARY:New constraints on the black hole spin in radio-loud quasars URL;TYPE=URI:/info/1025/4983.htm END:VEVENT BEGIN:VEVENT UID:4664@kiaa.pku.edu.cn DTSTAMP:20170223T145557Z CREATED:20170223T145557Z DESCRIPTION:Characterizing interstellar cloud turbulence DTSTART;TZID=Asia/Shanghai:20170309T160000 DTEND;TZID=Asia/Shanghai:20170309T170000 LAST-MODIFIED:20170223T145557Z LOCATION:KIAA-PKU Auditorium SUMMARY:Characterizing interstellar cloud turbulence URL;TYPE=URI:/info/1024/4664.htm END:VEVENT BEGIN:VEVENT UID:4978@kiaa.pku.edu.cn DTSTAMP:20170218T172355Z CREATED:20170218T172355Z DESCRIPTION:How to infer the mass of the planets that are forming in protoplanetary disks based on resolved disk observations? DTSTART;TZID=Asia/Shanghai:20170313T120000 DTEND;TZID=Asia/Shanghai:20170313T130000 LAST-MODIFIED:20170218T172355Z LOCATION:DoA, Rm 2907 SUMMARY:How to infer the mass of the planets that are forming in protoplanetary disks based on resolved disk observations? URL;TYPE=URI:/info/1025/4978.htm END:VEVENT BEGIN:VEVENT UID:5185@kiaa.pku.edu.cn DTSTAMP:20170302T085617Z CREATED:20170302T085617Z DESCRIPTION:KIAA Strategic Planning Committee Meeting DTSTART;TZID=Asia/Shanghai:20170315T103000 DTEND;TZID=Asia/Shanghai:20170315T120000 LAST-MODIFIED:20170302T085617Z LOCATION:2nd meeting room SUMMARY:KIAA Strategic Planning Committee Meeting URL;TYPE=URI:/info/1026/5185.htm END:VEVENT BEGIN:VEVENT UID:4975@kiaa.pku.edu.cn DTSTAMP:20170105T145259Z CREATED:20170105T145259Z DESCRIPTION:Universal dark halo scaling relation for the dwarf spheroidal satellites DTSTART;TZID=Asia/Shanghai:20170315T120000 DTEND;TZID=Asia/Shanghai:20170315T130000 LAST-MODIFIED:20170105T145259Z LOCATION:KIAA first floor meeting room SUMMARY:Universal dark halo scaling relation for the dwarf spheroidal satellites URL;TYPE=URI:/info/1025/4975.htm END:VEVENT BEGIN:VEVENT UID:4740@kiaa.pku.edu.cn DTSTAMP:20160919T174049Z CREATED:20160919T174049Z DESCRIPTION:X-shaped bulge of the Milky Way DTSTART;TZID=Asia/Shanghai:20170321T120000 DTEND;TZID=Asia/Shanghai:20170321T130000 LAST-MODIFIED:20160919T174049Z LOCATION:KIAA-PKU SUMMARY:X-shaped bulge of the Milky Way URL;TYPE=URI:/info/1028/4740.htm END:VEVENT BEGIN:VEVENT UID:4773@kiaa.pku.edu.cn DTSTAMP:20170314T112141Z CREATED:20170314T112141Z DESCRIPTION:A disintegrating minor planet transiting the WD 1145+017 DTSTART;TZID=Asia/Shanghai:20170328T120000 DTEND;TZID=Asia/Shanghai:20170328T130000 LAST-MODIFIED:20170314T112141Z LOCATION:KIAA-PKU SUMMARY:A disintegrating minor planet transiting the WD 1145+017 URL;TYPE=URI:/info/1028/4773.htm END:VEVENT BEGIN:VEVENT UID:4814@kiaa.pku.edu.cn DTSTAMP:20170310T170409Z CREATED:20170310T170409Z DESCRIPTION:Understanding the Dawn of Galaxies: Perspectives from the Galaxy Luminosity Function, the Global 21cm Signal and Beyond DTSTART;TZID=Asia/Shanghai:20170328T170000 DTEND;TZID=Asia/Shanghai:20170328T180000 LAST-MODIFIED:20170310T170409Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Understanding the Dawn of Galaxies: Perspectives from the Galaxy Luminosity Function, the Global 21cm Signal and Beyond URL;TYPE=URI:/info/1029/4814.htm END:VEVENT BEGIN:VEVENT UID:4976@kiaa.pku.edu.cn DTSTAMP:20170202T190705Z CREATED:20170202T190705Z DESCRIPTION:Water emission and molecular gas outflows in (ultra)luminous infrared galaxies at low and high redshift DTSTART;TZID=Asia/Shanghai:20170329T120000 DTEND;TZID=Asia/Shanghai:20170329T130000 LAST-MODIFIED:20170202T190705Z LOCATION:Kiaa first floor meeting room SUMMARY:Water emission and molecular gas outflows in (ultra)luminous infrared galaxies at low and high redshift URL;TYPE=URI:/info/1025/4976.htm END:VEVENT BEGIN:VEVENT UID:4678@kiaa.pku.edu.cn DTSTAMP:20160919T121730Z CREATED:20160919T121730Z DESCRIPTION:Modelling galaxy formation and reionization with DRAGONS DTSTART;TZID=Asia/Shanghai:20170330T160000 DTEND;TZID=Asia/Shanghai:20170330T160000 LAST-MODIFIED:20160919T121730Z LOCATION:KIAA-PKU Auditorium SUMMARY:Modelling galaxy formation and reionization with DRAGONS URL;TYPE=URI:/info/1024/4678.htm END:VEVENT BEGIN:VEVENT UID:3893@kiaa.pku.edu.cn DTSTAMP:20170321T101810Z CREATED:20170321T101810Z DESCRIPTION:Lecture to grad students: Modelling Galaxies DTSTART;TZID=Asia/Shanghai:20170331T100000 DTEND;TZID=Asia/Shanghai:20170331T120000 LAST-MODIFIED:20170321T101810Z LOCATION:Rm208, KIAA-PKU SUMMARY:Lecture to grad students: Modelling Galaxies URL;TYPE=URI:/info/1030/3893.htm END:VEVENT BEGIN:VEVENT UID:6677@kiaa.pku.edu.cn DTSTAMP:20170331T091038Z CREATED:20170331T091038Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20170401T091500 DTEND;TZID=Asia/Shanghai:20170402T091500 LAST-MODIFIED:20170331T091038Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6677.htm END:VEVENT BEGIN:VEVENT UID:6676@kiaa.pku.edu.cn DTSTAMP:20170331T090936Z CREATED:20170331T090936Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20170404T080000 DTEND;TZID=Asia/Shanghai:20170404T080000 LAST-MODIFIED:20170331T090936Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6676.htm END:VEVENT BEGIN:VEVENT UID:4656@kiaa.pku.edu.cn DTSTAMP:20170322T015940Z CREATED:20170322T015940Z DESCRIPTION:Solving the mystery of r-process, supernovae or neutron-star mergers? DTSTART;TZID=Asia/Shanghai:20170406T160000 DTEND;TZID=Asia/Shanghai:20170406T170000 LAST-MODIFIED:20170322T015940Z LOCATION:KIAA-PKU Auditorium SUMMARY:Solving the mystery of r-process, supernovae or neutron-star mergers? URL;TYPE=URI:/info/1024/4656.htm END:VEVENT BEGIN:VEVENT UID:4741@kiaa.pku.edu.cn DTSTAMP:20160919T174131Z CREATED:20160919T174131Z DESCRIPTION:Optical observations of a peculiar supernova: ASASSN-15nx DTSTART;TZID=Asia/Shanghai:20170411T120000 DTEND;TZID=Asia/Shanghai:20170411T130000 LAST-MODIFIED:20160919T174131Z LOCATION:KIAA-PKU SUMMARY:Optical observations of a peculiar supernova: ASASSN-15nx URL;TYPE=URI:/info/1028/4741.htm END:VEVENT BEGIN:VEVENT UID:4984@kiaa.pku.edu.cn DTSTAMP:20170227T132222Z CREATED:20170227T132222Z DESCRIPTION:Impact of molecular clouds on galactic disk clumpiness DTSTART;TZID=Asia/Shanghai:20170412T120000 DTEND;TZID=Asia/Shanghai:20170412T130000 LAST-MODIFIED:20170227T132222Z LOCATION:KIAA first floor meeting room SUMMARY:Impact of molecular clouds on galactic disk clumpiness URL;TYPE=URI:/info/1025/4984.htm END:VEVENT BEGIN:VEVENT UID:4658@kiaa.pku.edu.cn DTSTAMP:20170320T101405Z CREATED:20170320T101405Z DESCRIPTION:The Puzzle of Low Ionization Emission in Galaxies DTSTART;TZID=Asia/Shanghai:20170413T160000 DTEND;TZID=Asia/Shanghai:20170413T170000 LAST-MODIFIED:20170320T101405Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Puzzle of Low Ionization Emission in Galaxies URL;TYPE=URI:/info/1024/4658.htm END:VEVENT BEGIN:VEVENT UID:4985@kiaa.pku.edu.cn DTSTAMP:20170227T132304Z CREATED:20170227T132304Z DESCRIPTION:At the edge of galaxy clusters: splashback and accretion shock DTSTART;TZID=Asia/Shanghai:20170414T120000 DTEND;TZID=Asia/Shanghai:20170414T130000 LAST-MODIFIED:20170227T132304Z LOCATION:KIAA first floor meeting room SUMMARY:At the edge of galaxy clusters: splashback and accretion shock URL;TYPE=URI:/info/1025/4985.htm END:VEVENT BEGIN:VEVENT UID:4987@kiaa.pku.edu.cn DTSTAMP:20170331T141110Z CREATED:20170331T141110Z DESCRIPTION:Studying the Milky Way DTSTART;TZID=Asia/Shanghai:20170417T120000 DTEND;TZID=Asia/Shanghai:20170417T130000 LAST-MODIFIED:20170331T141110Z LOCATION:1st meeting room, KIAA SUMMARY:Studying the Milky Way URL;TYPE=URI:/info/1025/4987.htm END:VEVENT BEGIN:VEVENT UID:4743@kiaa.pku.edu.cn DTSTAMP:20160919T174358Z CREATED:20160919T174358Z DESCRIPTION:Strong lensing searches and cosmology DTSTART;TZID=Asia/Shanghai:20170418T120000 DTEND;TZID=Asia/Shanghai:20170418T130000 LAST-MODIFIED:20160919T174358Z LOCATION:KIAA-PKU SUMMARY:Strong lensing searches and cosmology URL;TYPE=URI:/info/1028/4743.htm END:VEVENT BEGIN:VEVENT UID:4815@kiaa.pku.edu.cn DTSTAMP:20170412T155641Z CREATED:20170412T155641Z DESCRIPTION:The QUEST-La Silla AGN variability survey DTSTART;TZID=Asia/Shanghai:20170418T170000 DTEND;TZID=Asia/Shanghai:20170418T180000 LAST-MODIFIED:20170412T155641Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The QUEST-La Silla AGN variability survey URL;TYPE=URI:/info/1029/4815.htm END:VEVENT BEGIN:VEVENT UID:4662@kiaa.pku.edu.cn DTSTAMP:20170316T210412Z CREATED:20170316T210412Z DESCRIPTION:Did LIGO hear the coalescence of primordial black holes? DTSTART;TZID=Asia/Shanghai:20170420T160000 DTEND;TZID=Asia/Shanghai:20170420T170000 LAST-MODIFIED:20170316T210412Z LOCATION:KIAA-PKU Auditorium SUMMARY:Did LIGO hear the coalescence of primordial black holes? URL;TYPE=URI:/info/1024/4662.htm END:VEVENT BEGIN:VEVENT UID:4989@kiaa.pku.edu.cn DTSTAMP:20170407T210459Z CREATED:20170407T210459Z DESCRIPTION:Inner structure of early-type galaxies since z=1.0: a simulation perspective DTSTART;TZID=Asia/Shanghai:20170424T120000 DTEND;TZID=Asia/Shanghai:20170424T130000 LAST-MODIFIED:20170407T210459Z LOCATION:DoA, Rm 2907 SUMMARY:Inner structure of early-type galaxies since z=1.0: a simulation perspective URL;TYPE=URI:/info/1025/4989.htm END:VEVENT BEGIN:VEVENT UID:4992@kiaa.pku.edu.cn DTSTAMP:20170418T115321Z CREATED:20170418T115321Z DESCRIPTION:Cosmological simulations of large scale structure and neutrinos DTSTART;TZID=Asia/Shanghai:20170428T120000 DTEND;TZID=Asia/Shanghai:20170428T130000 LAST-MODIFIED:20170418T115321Z LOCATION:KIAA first floor meeting room SUMMARY:Cosmological simulations of large scale structure and neutrinos URL;TYPE=URI:/info/1025/4992.htm END:VEVENT BEGIN:VEVENT UID:5172@kiaa.pku.edu.cn DTSTAMP:20160907T170522Z CREATED:20160907T170522Z DESCRIPTION:KIAA Science Advisory Committee Meeting DTSTART;TZID=Asia/Shanghai:20170501T093000 DTEND;TZID=Asia/Shanghai:20170502T180000 LAST-MODIFIED:20160907T170522Z LOCATION:1st Meeting Room SUMMARY:KIAA Science Advisory Committee Meeting URL;TYPE=URI:/info/1026/5172.htm END:VEVENT BEGIN:VEVENT UID:5173@kiaa.pku.edu.cn DTSTAMP:20160907T170616Z CREATED:20160907T170616Z DESCRIPTION:KIAA Governing Board Meeting DTSTART;TZID=Asia/Shanghai:20170503T090000 DTEND;TZID=Asia/Shanghai:20170503T170000 LAST-MODIFIED:20160907T170616Z LOCATION:1st Meeting Room SUMMARY:KIAA Governing Board Meeting URL;TYPE=URI:/info/1026/5173.htm END:VEVENT BEGIN:VEVENT UID:6674@kiaa.pku.edu.cn DTSTAMP:20170209T102133Z CREATED:20170209T102133Z DESCRIPTION:KIAA 10th Anniversary Symposium DTSTART;TZID=Asia/Shanghai:20170504T090000 DTEND;TZID=Asia/Shanghai:20170504T180000 LAST-MODIFIED:20170209T102133Z LOCATION:KIAA Auditorium SUMMARY:KIAA 10th Anniversary Symposium URL;TYPE=URI:/info/1089/6674.htm END:VEVENT BEGIN:VEVENT UID:4991@kiaa.pku.edu.cn DTSTAMP:20170410T170826Z CREATED:20170410T170826Z DESCRIPTION:CSI in Type Ia Supernova Remnants DTSTART;TZID=Asia/Shanghai:20170505T120000 DTEND;TZID=Asia/Shanghai:20170505T130000 LAST-MODIFIED:20170410T170826Z LOCATION:1st meeting room,KIAA SUMMARY:CSI in Type Ia Supernova Remnants URL;TYPE=URI:/info/1025/4991.htm END:VEVENT BEGIN:VEVENT UID:4653@kiaa.pku.edu.cn DTSTAMP:20170427T231450Z CREATED:20170427T231450Z DESCRIPTION:Black Holes and Gravitational Waves DTSTART;TZID=Asia/Shanghai:20170505T160000 DTEND;TZID=Asia/Shanghai:20170505T170000 LAST-MODIFIED:20170427T231450Z LOCATION:KIAA-PKU Auditorium SUMMARY:Black Holes and Gravitational Waves URL;TYPE=URI:/info/1024/4653.htm END:VEVENT BEGIN:VEVENT UID:4744@kiaa.pku.edu.cn DTSTAMP:20160919T174507Z CREATED:20160919T174507Z DESCRIPTION:Disk-jet connection in a special subclass of AGN--Narrow-line Seyfert 1 galaxies DTSTART;TZID=Asia/Shanghai:20170509T120000 DTEND;TZID=Asia/Shanghai:20170509T130000 LAST-MODIFIED:20160919T174507Z LOCATION:KIAA-PKU SUMMARY:Disk-jet connection in a special subclass of AGN--Narrow-line Seyfert 1 galaxies URL;TYPE=URI:/info/1028/4744.htm END:VEVENT BEGIN:VEVENT UID:4661@kiaa.pku.edu.cn DTSTAMP:20170317T111214Z CREATED:20170317T111214Z DESCRIPTION:3D Observations of Molecular Gas in Galaxies: From Global Dynamics to Supermassive Black Holes DTSTART;TZID=Asia/Shanghai:20170511T160000 DTEND;TZID=Asia/Shanghai:20170511T170000 LAST-MODIFIED:20170317T111214Z LOCATION:KIAA-PKU Auditorium SUMMARY:3D Observations of Molecular Gas in Galaxies: From Global Dynamics to Supermassive Black Holes URL;TYPE=URI:/info/1024/4661.htm END:VEVENT BEGIN:VEVENT UID:4779@kiaa.pku.edu.cn DTSTAMP:20160919T174546Z CREATED:20160919T174546Z DESCRIPTION:What will happen for pulsar if photon has mass? DTSTART;TZID=Asia/Shanghai:20170516T120000 DTEND;TZID=Asia/Shanghai:20170516T130000 LAST-MODIFIED:20160919T174546Z LOCATION:KIAA-PKU SUMMARY:What will happen for pulsar if photon has mass? URL;TYPE=URI:/info/1028/4779.htm END:VEVENT BEGIN:VEVENT UID:4990@kiaa.pku.edu.cn DTSTAMP:20170410T081703Z CREATED:20170410T081703Z DESCRIPTION:ESASky, ESA’s new science-driven portal for ESA space astronomy missions DTSTART;TZID=Asia/Shanghai:20170519T120000 DTEND;TZID=Asia/Shanghai:20170519T130000 LAST-MODIFIED:20170410T081703Z LOCATION:KIAA, First floor meeting room SUMMARY:ESASky, ESA’s new science-driven portal for ESA space astronomy missions URL;TYPE=URI:/info/1025/4990.htm END:VEVENT BEGIN:VEVENT UID:5184@kiaa.pku.edu.cn DTSTAMP:20170227T090236Z CREATED:20170227T090236Z DESCRIPTION:BHOLE Group 3 Workshop DTSTART;TZID=Asia/Shanghai:20170523T090000 DTEND;TZID=Asia/Shanghai:20170524T180000 LAST-MODIFIED:20170227T090236Z LOCATION:KIAA 1st meeting room SUMMARY:BHOLE Group 3 Workshop URL;TYPE=URI:/info/1026/5184.htm END:VEVENT BEGIN:VEVENT UID:4663@kiaa.pku.edu.cn DTSTAMP:20170223T191845Z CREATED:20170223T191845Z DESCRIPTION:Protoplanetary Disks around Pre-main Sequence Binary Stars DTSTART;TZID=Asia/Shanghai:20170525T160000 DTEND;TZID=Asia/Shanghai:20170525T170000 LAST-MODIFIED:20170223T191845Z LOCATION:KIAA-PKU Auditorium SUMMARY:Protoplanetary Disks around Pre-main Sequence Binary Stars URL;TYPE=URI:/info/1024/4663.htm END:VEVENT BEGIN:VEVENT UID:6678@kiaa.pku.edu.cn DTSTAMP:20170331T091134Z CREATED:20170331T091134Z DESCRIPTION:Dragon Boat Festival holiday DTSTART;TZID=Asia/Shanghai:20170527T091500 DTEND;TZID=Asia/Shanghai:20170528T091500 LAST-MODIFIED:20170331T091134Z LOCATION: SUMMARY:Dragon Boat Festival holiday URL;TYPE=URI:/info/1089/6678.htm END:VEVENT BEGIN:VEVENT UID:6679@kiaa.pku.edu.cn DTSTAMP:20170331T091150Z CREATED:20170331T091150Z DESCRIPTION:Dragon Boat Festival holiday DTSTART;TZID=Asia/Shanghai:20170530T000000 DTEND;TZID=Asia/Shanghai:20170530T000000 LAST-MODIFIED:20170331T091150Z LOCATION: SUMMARY:Dragon Boat Festival holiday URL;TYPE=URI:/info/1089/6679.htm END:VEVENT BEGIN:VEVENT UID:5186@kiaa.pku.edu.cn DTSTAMP:20170316T102440Z CREATED:20170316T102440Z DESCRIPTION:Workshop of Pulsar Timing Array in China DTSTART;TZID=Asia/Shanghai:20170530T090000 DTEND;TZID=Asia/Shanghai:20170531T170000 LAST-MODIFIED:20170316T102440Z LOCATION:KIAA Auditorium SUMMARY:Workshop of Pulsar Timing Array in China URL;TYPE=URI:/info/1026/5186.htm END:VEVENT BEGIN:VEVENT UID:4651@kiaa.pku.edu.cn DTSTAMP:20170523T222215Z CREATED:20170523T222215Z DESCRIPTION:Electromagnetic Counterparts to Gravitational Wave Detections: Bridging the Gap between Theory and Observation DTSTART;TZID=Asia/Shanghai:20170601T160000 DTEND;TZID=Asia/Shanghai:20170601T170000 LAST-MODIFIED:20170523T222215Z LOCATION:KIAA-PKU Auditorium SUMMARY:Electromagnetic Counterparts to Gravitational Wave Detections: Bridging the Gap between Theory and Observation URL;TYPE=URI:/info/1024/4651.htm END:VEVENT BEGIN:VEVENT UID:6683@kiaa.pku.edu.cn DTSTAMP:20170602T084903Z CREATED:20170602T084903Z DESCRIPTION:Undergraduate Thesis Defense DTSTART;TZID=Asia/Shanghai:20170602T080000 DTEND;TZID=Asia/Shanghai:20170602T123000 LAST-MODIFIED:20170602T084903Z LOCATION:KIAA Auditorium SUMMARY:Undergraduate Thesis Defense URL;TYPE=URI:/info/1089/6683.htm END:VEVENT BEGIN:VEVENT UID:4986@kiaa.pku.edu.cn DTSTAMP:20170316T164542Z CREATED:20170316T164542Z DESCRIPTION:Multiscale view of disk formation around low-mass stars DTSTART;TZID=Asia/Shanghai:20170605T120000 DTEND;TZID=Asia/Shanghai:20170605T130000 LAST-MODIFIED:20170316T164542Z LOCATION:DoA, Rm 2907 SUMMARY:Multiscale view of disk formation around low-mass stars URL;TYPE=URI:/info/1025/4986.htm END:VEVENT BEGIN:VEVENT UID:4742@kiaa.pku.edu.cn DTSTAMP:20160919T174316Z CREATED:20160919T174316Z DESCRIPTION:Environmental Quenching of Star-formation Activity DTSTART;TZID=Asia/Shanghai:20170606T120000 DTEND;TZID=Asia/Shanghai:20170606T130000 LAST-MODIFIED:20160919T174316Z LOCATION:KIAA-PKU SUMMARY:Environmental Quenching of Star-formation Activity URL;TYPE=URI:/info/1028/4742.htm END:VEVENT BEGIN:VEVENT UID:3894@kiaa.pku.edu.cn DTSTAMP:20170531T160904Z CREATED:20170531T160904Z DESCRIPTION:Thesis Project Report & Qualification Examination for Grade 2 Grad Students DTSTART;TZID=Asia/Shanghai:20170608T081500 DTEND;TZID=Asia/Shanghai:20170608T123000 LAST-MODIFIED:20170531T160904Z LOCATION:1st meeting room, KIAA SUMMARY:Thesis Project Report & Qualification Examination for Grade 2 Grad Students URL;TYPE=URI:/info/1030/3894.htm END:VEVENT BEGIN:VEVENT UID:3895@kiaa.pku.edu.cn DTSTAMP:20170608T090045Z CREATED:20170608T090045Z DESCRIPTION:Graduate lunch discussion with Prof. Xu Kong DTSTART;TZID=Asia/Shanghai:20170608T120000 DTEND;TZID=Asia/Shanghai:20170608T130000 LAST-MODIFIED:20170608T090045Z LOCATION:1st meetig room, KIAA SUMMARY:Graduate lunch discussion with Prof. Xu Kong URL;TYPE=URI:/info/1030/3895.htm END:VEVENT BEGIN:VEVENT UID:4659@kiaa.pku.edu.cn DTSTAMP:20170319T181442Z CREATED:20170319T181442Z DESCRIPTION:Star formation quenching and mass assembly of galaxies DTSTART;TZID=Asia/Shanghai:20170608T160000 DTEND;TZID=Asia/Shanghai:20170608T170000 LAST-MODIFIED:20170319T181442Z LOCATION:KIAA-PKU Auditorium SUMMARY:Star formation quenching and mass assembly of galaxies URL;TYPE=URI:/info/1024/4659.htm END:VEVENT BEGIN:VEVENT UID:4994@kiaa.pku.edu.cn DTSTAMP:20170602T152538Z CREATED:20170602T152538Z DESCRIPTION:Title: Machine Learning and Automated Analysis of Strong Gravitational Lensing Systems DTSTART;TZID=Asia/Shanghai:20170609T120000 DTEND;TZID=Asia/Shanghai:20170609T130000 LAST-MODIFIED:20170602T152538Z LOCATION:KIAA First floor meeting room SUMMARY:Title: Machine Learning and Automated Analysis of Strong Gravitational Lensing Systems URL;TYPE=URI:/info/1025/4994.htm END:VEVENT BEGIN:VEVENT UID:4772@kiaa.pku.edu.cn DTSTAMP:20170314T113421Z CREATED:20170314T113421Z DESCRIPTION:The Optical--Mid-infrared Extinction Law of the l = 165 Sightline in the Galactic Plane DTSTART;TZID=Asia/Shanghai:20170613T120000 DTEND;TZID=Asia/Shanghai:20170613T130000 LAST-MODIFIED:20170314T113421Z LOCATION:KIAA-PKU SUMMARY:The Optical--Mid-infrared Extinction Law of the l = 165 Sightline in the Galactic Plane URL;TYPE=URI:/info/1028/4772.htm END:VEVENT BEGIN:VEVENT UID:4998@kiaa.pku.edu.cn DTSTAMP:20170612T210501Z CREATED:20170612T210501Z DESCRIPTION:ALMA as a sensitive probe of the stellar IMF across the cosmic time DTSTART;TZID=Asia/Shanghai:20170614T120000 DTEND;TZID=Asia/Shanghai:20170614T130000 LAST-MODIFIED:20170612T210501Z LOCATION:KIAA, First floor meeting room SUMMARY:ALMA as a sensitive probe of the stellar IMF across the cosmic time URL;TYPE=URI:/info/1025/4998.htm END:VEVENT BEGIN:VEVENT UID:4665@kiaa.pku.edu.cn DTSTAMP:20170221T084235Z CREATED:20170221T084235Z DESCRIPTION:Anisotropic Galaxy Clustering in the Isotropic Universe DTSTART;TZID=Asia/Shanghai:20170615T160000 DTEND;TZID=Asia/Shanghai:20170615T170000 LAST-MODIFIED:20170221T084235Z LOCATION:KIAA-PKU Auditorium SUMMARY:Anisotropic Galaxy Clustering in the Isotropic Universe URL;TYPE=URI:/info/1024/4665.htm END:VEVENT BEGIN:VEVENT UID:4774@kiaa.pku.edu.cn DTSTAMP:20170314T111437Z CREATED:20170314T111437Z DESCRIPTION:Was Small Scale Crisis in Lambda CDM solved? DTSTART;TZID=Asia/Shanghai:20170620T120000 DTEND;TZID=Asia/Shanghai:20170620T130000 LAST-MODIFIED:20170314T111437Z LOCATION:KIAA-PKU SUMMARY:Was Small Scale Crisis in Lambda CDM solved? URL;TYPE=URI:/info/1028/4774.htm END:VEVENT BEGIN:VEVENT UID:4657@kiaa.pku.edu.cn DTSTAMP:20170321T163942Z CREATED:20170321T163942Z DESCRIPTION:Gravitational Wave Astronomy with High-Frequency Gravitational Waves DTSTART;TZID=Asia/Shanghai:20170622T160000 DTEND;TZID=Asia/Shanghai:20170622T170000 LAST-MODIFIED:20170321T163942Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gravitational Wave Astronomy with High-Frequency Gravitational Waves URL;TYPE=URI:/info/1024/4657.htm END:VEVENT BEGIN:VEVENT UID:4993@kiaa.pku.edu.cn DTSTAMP:20170424T085359Z CREATED:20170424T085359Z DESCRIPTION:Color gradients and dust attenuation in CANDELS galaxies DTSTART;TZID=Asia/Shanghai:20170623T120000 DTEND;TZID=Asia/Shanghai:20170623T130000 LAST-MODIFIED:20170424T085359Z LOCATION:1st meeting room, KIAA SUMMARY:Color gradients and dust attenuation in CANDELS galaxies URL;TYPE=URI:/info/1025/4993.htm END:VEVENT BEGIN:VEVENT UID:3896@kiaa.pku.edu.cn DTSTAMP:20170622T083001Z CREATED:20170622T083001Z DESCRIPTION:Pulsars - Celestial Clocks DTSTART;TZID=Asia/Shanghai:20170623T160000 DTEND;TZID=Asia/Shanghai:20170623T160000 LAST-MODIFIED:20170622T083001Z LOCATION:KIAA 1st meeting room SUMMARY:Pulsars - Celestial Clocks URL;TYPE=URI:/info/1030/3896.htm END:VEVENT BEGIN:VEVENT UID:4655@kiaa.pku.edu.cn DTSTAMP:20170402T170248Z CREATED:20170402T170248Z DESCRIPTION:Super- and sub-Chandrasekhar limiting mass white dwarfs: Progenitors of peculiar type Ia supernovae and multiple astrophysical implications DTSTART;TZID=Asia/Shanghai:20170629T160000 DTEND;TZID=Asia/Shanghai:20170629T170000 LAST-MODIFIED:20170402T170248Z LOCATION:KIAA-PKU Auditorium SUMMARY:Super- and sub-Chandrasekhar limiting mass white dwarfs: Progenitors of peculiar type Ia supernovae and multiple astrophysical implications URL;TYPE=URI:/info/1024/4655.htm END:VEVENT BEGIN:VEVENT UID:4997@kiaa.pku.edu.cn DTSTAMP:20170608T171831Z CREATED:20170608T171831Z DESCRIPTION:Hydrogen Emission and Absorption in the Halos of the Milky Way and Nearby Galaxies DTSTART;TZID=Asia/Shanghai:20170630T120000 DTEND;TZID=Asia/Shanghai:20170630T130000 LAST-MODIFIED:20170608T171831Z LOCATION:1st meeting room, KIAA SUMMARY:Hydrogen Emission and Absorption in the Halos of the Milky Way and Nearby Galaxies URL;TYPE=URI:/info/1025/4997.htm END:VEVENT BEGIN:VEVENT UID:4999@kiaa.pku.edu.cn DTSTAMP:20170622T113058Z CREATED:20170622T113058Z DESCRIPTION:Stellar feedback and star formation in Galactic high mass star forming regions DTSTART;TZID=Asia/Shanghai:20170704T120000 DTEND;TZID=Asia/Shanghai:20170704T130000 LAST-MODIFIED:20170622T113058Z LOCATION:KIAA First floor meeting room SUMMARY:Stellar feedback and star formation in Galactic high mass star forming regions URL;TYPE=URI:/info/1025/4999.htm END:VEVENT BEGIN:VEVENT UID:4650@kiaa.pku.edu.cn DTSTAMP:20170525T095402Z CREATED:20170525T095402Z DESCRIPTION:Observing Variability of Embedded Protostars: The JCMT Transient Survey DTSTART;TZID=Asia/Shanghai:20170706T160000 DTEND;TZID=Asia/Shanghai:20170706T170000 LAST-MODIFIED:20170525T095402Z LOCATION:KIAA-PKU Auditorium SUMMARY:Observing Variability of Embedded Protostars: The JCMT Transient Survey URL;TYPE=URI:/info/1024/4650.htm END:VEVENT BEGIN:VEVENT UID:4996@kiaa.pku.edu.cn DTSTAMP:20170608T105803Z CREATED:20170608T105803Z DESCRIPTION:Applications of Spiral Density Waves: from Circumstellar disks to Circumplanetary Disks DTSTART;TZID=Asia/Shanghai:20170707T120000 DTEND;TZID=Asia/Shanghai:20170707T130000 LAST-MODIFIED:20170608T105803Z LOCATION:KIAA, First floor meeting room SUMMARY:Applications of Spiral Density Waves: from Circumstellar disks to Circumplanetary Disks URL;TYPE=URI:/info/1025/4996.htm END:VEVENT BEGIN:VEVENT UID:4816@kiaa.pku.edu.cn DTSTAMP:20170630T113021Z CREATED:20170630T113021Z DESCRIPTION:Self Gravity and Physical State of Molecular Gas in Nearby Galaxies DTSTART;TZID=Asia/Shanghai:20170707T170000 DTEND;TZID=Asia/Shanghai:20170707T170000 LAST-MODIFIED:20170630T113021Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Self Gravity and Physical State of Molecular Gas in Nearby Galaxies URL;TYPE=URI:/info/1029/4816.htm END:VEVENT BEGIN:VEVENT UID:4988@kiaa.pku.edu.cn DTSTAMP:20170405T085921Z CREATED:20170405T085921Z DESCRIPTION:The Cosmic Microwave Background, the Hubble Constant, and Cosmological Models DTSTART;TZID=Asia/Shanghai:20170710T120000 DTEND;TZID=Asia/Shanghai:20170710T130000 LAST-MODIFIED:20170405T085921Z LOCATION:1st meeting room, KIAA SUMMARY:The Cosmic Microwave Background, the Hubble Constant, and Cosmological Models URL;TYPE=URI:/info/1025/4988.htm END:VEVENT BEGIN:VEVENT UID:6675@kiaa.pku.edu.cn DTSTAMP:20170321T150001Z CREATED:20170321T150001Z DESCRIPTION:Summer Vacation DTSTART;TZID=Asia/Shanghai:20170712T000000 DTEND;TZID=Asia/Shanghai:20170823T000000 LAST-MODIFIED:20170321T150001Z LOCATION: SUMMARY:Summer Vacation URL;TYPE=URI:/info/1089/6675.htm END:VEVENT BEGIN:VEVENT UID:5000@kiaa.pku.edu.cn DTSTAMP:20170704T152610Z CREATED:20170704T152610Z DESCRIPTION:Microlensing Parallax Observations with Spitzer and Kepler DTSTART;TZID=Asia/Shanghai:20170714T120000 DTEND;TZID=Asia/Shanghai:20170714T130000 LAST-MODIFIED:20170704T152610Z LOCATION:KIAA First floor meeting room SUMMARY:Microlensing Parallax Observations with Spitzer and Kepler URL;TYPE=URI:/info/1025/5000.htm END:VEVENT BEGIN:VEVENT UID:3897@kiaa.pku.edu.cn DTSTAMP:20170714T094722Z CREATED:20170714T094722Z DESCRIPTION:Science Opportunities with new ground based gravitational wave detectors in the Asian region DTSTART;TZID=Asia/Shanghai:20170714T150000 DTEND;TZID=Asia/Shanghai:20170714T150000 LAST-MODIFIED:20170714T094722Z LOCATION:KIAA-PKU SUMMARY:Science Opportunities with new ground based gravitational wave detectors in the Asian region URL;TYPE=URI:/info/1030/3897.htm END:VEVENT BEGIN:VEVENT UID:5001@kiaa.pku.edu.cn DTSTAMP:20170705T142824Z CREATED:20170705T142824Z DESCRIPTION:The Electromagnetic Radiation and Gravitational Waves from the First Black Holes DTSTART;TZID=Asia/Shanghai:20170719T120000 DTEND;TZID=Asia/Shanghai:20170719T130000 LAST-MODIFIED:20170705T142824Z LOCATION:KIAA First floor meeting room SUMMARY:The Electromagnetic Radiation and Gravitational Waves from the First Black Holes URL;TYPE=URI:/info/1025/5001.htm END:VEVENT BEGIN:VEVENT UID:3898@kiaa.pku.edu.cn DTSTAMP:20170718T221551Z CREATED:20170718T221551Z DESCRIPTION:Mapping the Dust Obscured Cosmic Star Formation DTSTART;TZID=Asia/Shanghai:20170719T160000 DTEND;TZID=Asia/Shanghai:20170719T160000 LAST-MODIFIED:20170718T221551Z LOCATION:KIAA 1st meeting room SUMMARY:Mapping the Dust Obscured Cosmic Star Formation URL;TYPE=URI:/info/1030/3898.htm END:VEVENT BEGIN:VEVENT UID:6684@kiaa.pku.edu.cn DTSTAMP:20170711T091508Z CREATED:20170711T091508Z DESCRIPTION:Summer camp DTSTART;TZID=Asia/Shanghai:20170719T160000 DTEND;TZID=Asia/Shanghai:20170723T190000 LAST-MODIFIED:20170711T091508Z LOCATION:1st meeting room,KIAA SUMMARY:Summer camp URL;TYPE=URI:/info/1089/6684.htm END:VEVENT BEGIN:VEVENT UID:4995@kiaa.pku.edu.cn DTSTAMP:20170608T081645Z CREATED:20170608T081645Z DESCRIPTION:Probing giant-planet forming zones around Solar-like stars with CO DTSTART;TZID=Asia/Shanghai:20170725T120000 DTEND;TZID=Asia/Shanghai:20170725T130000 LAST-MODIFIED:20170608T081645Z LOCATION:KIAA First floor meeting room SUMMARY:Probing giant-planet forming zones around Solar-like stars with CO URL;TYPE=URI:/info/1025/4995.htm END:VEVENT BEGIN:VEVENT UID:4649@kiaa.pku.edu.cn DTSTAMP:20170610T121216Z CREATED:20170610T121216Z DESCRIPTION:IceCube and the Discovery of Energetic Cosmic Neutrinos DTSTART;TZID=Asia/Shanghai:20170727T160000 DTEND;TZID=Asia/Shanghai:20170727T170000 LAST-MODIFIED:20170610T121216Z LOCATION:KIAA-PKU Auditorium SUMMARY:IceCube and the Discovery of Energetic Cosmic Neutrinos URL;TYPE=URI:/info/1024/4649.htm END:VEVENT BEGIN:VEVENT UID:5004@kiaa.pku.edu.cn DTSTAMP:20170719T215652Z CREATED:20170719T215652Z DESCRIPTION:Angular correlation studies of the cosmic X-ray background: A new frontier of ICM structure studies DTSTART;TZID=Asia/Shanghai:20170801T120000 DTEND;TZID=Asia/Shanghai:20170801T130000 LAST-MODIFIED:20170719T215652Z LOCATION:KIAA first floor meeting room SUMMARY:Angular correlation studies of the cosmic X-ray background: A new frontier of ICM structure studies URL;TYPE=URI:/info/1025/5004.htm END:VEVENT BEGIN:VEVENT UID:6685@kiaa.pku.edu.cn DTSTAMP:20170724T093628Z CREATED:20170724T093628Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20170802T090000 DTEND;TZID=Asia/Shanghai:20170802T103000 LAST-MODIFIED:20170724T093628Z LOCATION:KIAA SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1089/6685.htm END:VEVENT BEGIN:VEVENT UID:5003@kiaa.pku.edu.cn DTSTAMP:20170717T140746Z CREATED:20170717T140746Z DESCRIPTION:Evolution of galaxies as traced by stellar populations DTSTART;TZID=Asia/Shanghai:20170802T120000 DTEND;TZID=Asia/Shanghai:20170802T130000 LAST-MODIFIED:20170717T140746Z LOCATION:KIAA First floor meeting room SUMMARY:Evolution of galaxies as traced by stellar populations URL;TYPE=URI:/info/1025/5003.htm END:VEVENT BEGIN:VEVENT UID:5182@kiaa.pku.edu.cn DTSTAMP:20161226T144538Z CREATED:20161226T144538Z DESCRIPTION:Workshop on Astroparticle Physics II DTSTART;TZID=Asia/Shanghai:20170817T090000 DTEND;TZID=Asia/Shanghai:20170819T180000 LAST-MODIFIED:20161226T144538Z LOCATION:KIAA Auditorium SUMMARY:Workshop on Astroparticle Physics II URL;TYPE=URI:/info/1026/5182.htm END:VEVENT BEGIN:VEVENT UID:5187@kiaa.pku.edu.cn DTSTAMP:20170317T084856Z CREATED:20170317T084856Z DESCRIPTION:2017 SHAO-PKU bilateral symposium DTSTART;TZID=Asia/Shanghai:20170824T084500 DTEND;TZID=Asia/Shanghai:20170825T180000 LAST-MODIFIED:20170317T084856Z LOCATION:SHAO, Shanghai SUMMARY:2017 SHAO-PKU bilateral symposium URL;TYPE=URI:/info/1026/5187.htm END:VEVENT BEGIN:VEVENT UID:5007@kiaa.pku.edu.cn DTSTAMP:20170824T160512Z CREATED:20170824T160512Z DESCRIPTION:Roles of Environment and Core Stellar Density in Star-formation Quenching DTSTART;TZID=Asia/Shanghai:20170905T120000 DTEND;TZID=Asia/Shanghai:20170905T130000 LAST-MODIFIED:20170824T160512Z LOCATION:1st meeting room, KIAA SUMMARY:Roles of Environment and Core Stellar Density in Star-formation Quenching URL;TYPE=URI:/info/1025/5007.htm END:VEVENT BEGIN:VEVENT UID:3901@kiaa.pku.edu.cn DTSTAMP:20170907T084419Z CREATED:20170907T084419Z DESCRIPTION:Silk Road Project Group Seminar (Tea Seminar) DTSTART;TZID=Asia/Shanghai:20170907T150000 DTEND;TZID=Asia/Shanghai:20170907T170000 LAST-MODIFIED:20170907T084419Z LOCATION:1st meeting room, KIAA-PKU SUMMARY:Silk Road Project Group Seminar (Tea Seminar) URL;TYPE=URI:/info/1030/3901.htm END:VEVENT BEGIN:VEVENT UID:5177@kiaa.pku.edu.cn DTSTAMP:20161010T090411Z CREATED:20161010T090411Z DESCRIPTION:Stellar Populations and the Distance Scale (a conference in honour of Jeremy Mould) DTSTART;TZID=Asia/Shanghai:20170911T090000 DTEND;TZID=Asia/Shanghai:20170915T180000 LAST-MODIFIED:20161010T090411Z LOCATION:Auditorium SUMMARY:Stellar Populations and the Distance Scale (a conference in honour of Jeremy Mould) URL;TYPE=URI:/info/1026/5177.htm END:VEVENT BEGIN:VEVENT UID:3900@kiaa.pku.edu.cn DTSTAMP:20170830T161008Z CREATED:20170830T161008Z DESCRIPTION:Dark Ages to Dark Endings: The Life Cycle of Galaxies in the New Cosmology DTSTART;TZID=Asia/Shanghai:20170913T143000 DTEND;TZID=Asia/Shanghai:20170913T160000 LAST-MODIFIED:20170830T161008Z LOCATION:Room 202, West Building of Physics School. SUMMARY:Dark Ages to Dark Endings: The Life Cycle of Galaxies in the New Cosmology URL;TYPE=URI:/info/1030/3900.htm END:VEVENT BEGIN:VEVENT UID:4817@kiaa.pku.edu.cn DTSTAMP:20170908T144556Z CREATED:20170908T144556Z DESCRIPTION:Studying kinematically decoupled galaxies with MaNGA DTSTART;TZID=Asia/Shanghai:20170917T170000 DTEND;TZID=Asia/Shanghai:20170917T180000 LAST-MODIFIED:20170908T144556Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Studying kinematically decoupled galaxies with MaNGA URL;TYPE=URI:/info/1029/4817.htm END:VEVENT BEGIN:VEVENT UID:5002@kiaa.pku.edu.cn DTSTAMP:20170707T194957Z CREATED:20170707T194957Z DESCRIPTION:What is Nature Astronomy and how do I get published in it ? DTSTART;TZID=Asia/Shanghai:20170918T120000 DTEND;TZID=Asia/Shanghai:20170918T130000 LAST-MODIFIED:20170707T194957Z LOCATION:TBD SUMMARY:What is Nature Astronomy and how do I get published in it ? URL;TYPE=URI:/info/1025/5002.htm END:VEVENT BEGIN:VEVENT UID:4646@kiaa.pku.edu.cn DTSTAMP:20170829T153712Z CREATED:20170829T153712Z DESCRIPTION:The growth of disks and bulges DTSTART;TZID=Asia/Shanghai:20170919T160000 DTEND;TZID=Asia/Shanghai:20170919T170000 LAST-MODIFIED:20170829T153712Z LOCATION:KIAA-PKU Auditorium SUMMARY:The growth of disks and bulges URL;TYPE=URI:/info/1024/4646.htm END:VEVENT BEGIN:VEVENT UID:5005@kiaa.pku.edu.cn DTSTAMP:20170822T202100Z CREATED:20170822T202100Z DESCRIPTION:Dark matter in the Galactic dwarf spheroidal galaxies DTSTART;TZID=Asia/Shanghai:20170925T120000 DTEND;TZID=Asia/Shanghai:20170925T130000 LAST-MODIFIED:20170822T202100Z LOCATION:1st meeting room, KIAA SUMMARY:Dark matter in the Galactic dwarf spheroidal galaxies URL;TYPE=URI:/info/1025/5005.htm END:VEVENT BEGIN:VEVENT UID:5008@kiaa.pku.edu.cn DTSTAMP:20170902T160421Z CREATED:20170902T160421Z DESCRIPTION:Orion: a test bed for studying evolution of protoplanetary disks DTSTART;TZID=Asia/Shanghai:20170927T120000 DTEND;TZID=Asia/Shanghai:20170927T130000 LAST-MODIFIED:20170902T160421Z LOCATION:1st meeting room, KIAA SUMMARY:Orion: a test bed for studying evolution of protoplanetary disks URL;TYPE=URI:/info/1025/5008.htm END:VEVENT BEGIN:VEVENT UID:3899@kiaa.pku.edu.cn DTSTAMP:20170721T100139Z CREATED:20170721T100139Z DESCRIPTION:The importance of telescopes of all sizes, from small to extremely large: the example of exoplanet research DTSTART;TZID=Asia/Shanghai:20170929T110000 DTEND;TZID=Asia/Shanghai:20170929T110000 LAST-MODIFIED:20170721T100139Z LOCATION:Auditorium, KIAA-PKU SUMMARY:The importance of telescopes of all sizes, from small to extremely large: the example of exoplanet research URL;TYPE=URI:/info/1030/3899.htm END:VEVENT BEGIN:VEVENT UID:6680@kiaa.pku.edu.cn DTSTAMP:20170523T121306Z CREATED:20170523T121306Z DESCRIPTION:National Day holiday DTSTART;TZID=Asia/Shanghai:20170930T000000 DTEND;TZID=Asia/Shanghai:20171008T000000 LAST-MODIFIED:20170523T121306Z LOCATION: SUMMARY:National Day holiday URL;TYPE=URI:/info/1089/6680.htm END:VEVENT BEGIN:VEVENT UID:5149@kiaa.pku.edu.cn DTSTAMP:20170924T180136Z CREATED:20170924T180136Z DESCRIPTION:Microstructure of the Ionized ISM from Pulsar Observations DTSTART;TZID=Asia/Shanghai:20171011T120000 DTEND;TZID=Asia/Shanghai:20171011T130000 LAST-MODIFIED:20170924T180136Z LOCATION:1st meeting room at KIAA SUMMARY:Microstructure of the Ionized ISM from Pulsar Observations URL;TYPE=URI:/info/1025/5149.htm END:VEVENT BEGIN:VEVENT UID:4652@kiaa.pku.edu.cn DTSTAMP:20170510T201902Z CREATED:20170510T201902Z DESCRIPTION:Dwarf galaxies and their satellites as extreme probes of LCDM DTSTART;TZID=Asia/Shanghai:20171012T160000 DTEND;TZID=Asia/Shanghai:20171012T170000 LAST-MODIFIED:20170510T201902Z LOCATION:KIAA-PKU Auditorium SUMMARY:Dwarf galaxies and their satellites as extreme probes of LCDM URL;TYPE=URI:/info/1024/4652.htm END:VEVENT BEGIN:VEVENT UID:5188@kiaa.pku.edu.cn DTSTAMP:20170602T091436Z CREATED:20170602T091436Z DESCRIPTION:Meeting: Transients from compact objects DTSTART;TZID=Asia/Shanghai:20171016T090000 DTEND;TZID=Asia/Shanghai:20171020T200000 LAST-MODIFIED:20170602T091436Z LOCATION:1st meeting room, KIAA SUMMARY:Meeting: Transients from compact objects URL;TYPE=URI:/info/1026/5188.htm END:VEVENT BEGIN:VEVENT UID:4770@kiaa.pku.edu.cn DTSTAMP:20171107T133051Z CREATED:20171107T133051Z DESCRIPTION:The secular evolution driven by bars DTSTART;TZID=Asia/Shanghai:20171017T120000 DTEND;TZID=Asia/Shanghai:20171017T130000 LAST-MODIFIED:20171107T133051Z LOCATION:KIAA-PKU SUMMARY:The secular evolution driven by bars URL;TYPE=URI:/info/1028/4770.htm END:VEVENT BEGIN:VEVENT UID:5009@kiaa.pku.edu.cn DTSTAMP:20170915T153955Z CREATED:20170915T153955Z DESCRIPTION:Aligning Visions for Maunakea CANCELLED DTSTART;TZID=Asia/Shanghai:20171018T120000 DTEND;TZID=Asia/Shanghai:20171018T130000 LAST-MODIFIED:20170915T153955Z LOCATION:DoA, Rm 2907 SUMMARY:Aligning Visions for Maunakea CANCELLED URL;TYPE=URI:/info/1025/5009.htm END:VEVENT BEGIN:VEVENT UID:4654@kiaa.pku.edu.cn DTSTAMP:20170419T202640Z CREATED:20170419T202640Z DESCRIPTION:The Nuclear Physics of Neutron Stars DTSTART;TZID=Asia/Shanghai:20171019T160000 DTEND;TZID=Asia/Shanghai:20171019T170000 LAST-MODIFIED:20170419T202640Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Nuclear Physics of Neutron Stars URL;TYPE=URI:/info/1024/4654.htm END:VEVENT BEGIN:VEVENT UID:5148@kiaa.pku.edu.cn DTSTAMP:20171012T140127Z CREATED:20171012T140127Z DESCRIPTION:MG: Simulating chemistry in star forming environments -- KS: Producing distant solar system bodies by mutual scattering of planetary embryos DTSTART;TZID=Asia/Shanghai:20171023T120000 DTEND;TZID=Asia/Shanghai:20171023T130000 LAST-MODIFIED:20171012T140127Z LOCATION:DoA, Rm 2907 SUMMARY:MG: Simulating chemistry in star forming environments -- KS: Producing distant solar system bodies by mutual scattering of planetary embryos URL;TYPE=URI:/info/1025/5148.htm END:VEVENT BEGIN:VEVENT UID:5147@kiaa.pku.edu.cn DTSTAMP:20171013T145952Z CREATED:20171013T145952Z DESCRIPTION:Modelling atomic and molecular gas and the radial profiles in SAMs. DTSTART;TZID=Asia/Shanghai:20171024T120000 DTEND;TZID=Asia/Shanghai:20171024T130000 LAST-MODIFIED:20171013T145952Z LOCATION:KIAA, 1st floor meeting room SUMMARY:Modelling atomic and molecular gas and the radial profiles in SAMs. URL;TYPE=URI:/info/1025/5147.htm END:VEVENT BEGIN:VEVENT UID:3903@kiaa.pku.edu.cn DTSTAMP:20171022T111229Z CREATED:20171022T111229Z DESCRIPTION:Gravitational Wave Seminar: Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources DTSTART;TZID=Asia/Shanghai:20171024T150000 DTEND;TZID=Asia/Shanghai:20171024T170000 LAST-MODIFIED:20171022T111229Z LOCATION:Auditorium Room, Kavli Institute for Astronomy and Astrophysics at Peking University. SUMMARY:Gravitational Wave Seminar: Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources URL;TYPE=URI:/info/1030/3903.htm END:VEVENT BEGIN:VEVENT UID:3902@kiaa.pku.edu.cn DTSTAMP:20171019T085621Z CREATED:20171019T085621Z DESCRIPTION:Meeting between Shri Kulkarni and Students DTSTART;TZID=Asia/Shanghai:20171025T100000 DTEND;TZID=Asia/Shanghai:20171025T100000 LAST-MODIFIED:20171019T085621Z LOCATION:1st meeting room, KIAA-PKU SUMMARY:Meeting between Shri Kulkarni and Students URL;TYPE=URI:/info/1030/3902.htm END:VEVENT BEGIN:VEVENT UID:5150@kiaa.pku.edu.cn DTSTAMP:20170918T131416Z CREATED:20170918T131416Z DESCRIPTION:The formation of the smallest galaxies DTSTART;TZID=Asia/Shanghai:20171025T120000 DTEND;TZID=Asia/Shanghai:20171025T130000 LAST-MODIFIED:20170918T131416Z LOCATION:KIAA first floor meeting room SUMMARY:The formation of the smallest galaxies URL;TYPE=URI:/info/1025/5150.htm END:VEVENT BEGIN:VEVENT UID:4647@kiaa.pku.edu.cn DTSTAMP:20170706T141054Z CREATED:20170706T141054Z DESCRIPTION:High energy neutrino astronomy: What have we learned? DTSTART;TZID=Asia/Shanghai:20171026T160000 DTEND;TZID=Asia/Shanghai:20171026T170000 LAST-MODIFIED:20170706T141054Z LOCATION:KIAA-PKU Auditorium SUMMARY:High energy neutrino astronomy: What have we learned? URL;TYPE=URI:/info/1024/4647.htm END:VEVENT BEGIN:VEVENT UID:5190@kiaa.pku.edu.cn DTSTAMP:20170906T133849Z CREATED:20170906T133849Z DESCRIPTION:Bhole Annuel Meeting DTSTART;TZID=Asia/Shanghai:20171027T083000 DTEND;TZID=Asia/Shanghai:20171027T123000 LAST-MODIFIED:20170906T133849Z LOCATION:KIAA Auditorium SUMMARY:Bhole Annuel Meeting URL;TYPE=URI:/info/1026/5190.htm END:VEVENT BEGIN:VEVENT UID:5006@kiaa.pku.edu.cn DTSTAMP:20170824T135218Z CREATED:20170824T135218Z DESCRIPTION:Discovery of ram-pressure stripped gas around an elliptical galaxy in Abell 2670 DTSTART;TZID=Asia/Shanghai:20171030T120000 DTEND;TZID=Asia/Shanghai:20171030T130000 LAST-MODIFIED:20170824T135218Z LOCATION:DoA, Rm 2907 SUMMARY:Discovery of ram-pressure stripped gas around an elliptical galaxy in Abell 2670 URL;TYPE=URI:/info/1025/5006.htm END:VEVENT BEGIN:VEVENT UID:5152@kiaa.pku.edu.cn DTSTAMP:20170918T083943Z CREATED:20170918T083943Z DESCRIPTION:The properties of the inner disk around HL Tau: Multi-wavelength modeling of the dust emission DTSTART;TZID=Asia/Shanghai:20171031T120000 DTEND;TZID=Asia/Shanghai:20171031T130000 LAST-MODIFIED:20170918T083943Z LOCATION:1st meeting room, KIAA SUMMARY:The properties of the inner disk around HL Tau: Multi-wavelength modeling of the dust emission URL;TYPE=URI:/info/1025/5152.htm END:VEVENT BEGIN:VEVENT UID:5193@kiaa.pku.edu.cn DTSTAMP:20171019T090358Z CREATED:20171019T090358Z DESCRIPTION:Innovation Group Meeting DTSTART;TZID=Asia/Shanghai:20171102T100000 DTEND;TZID=Asia/Shanghai:20171102T113000 LAST-MODIFIED:20171019T090358Z LOCATION: SUMMARY:Innovation Group Meeting URL;TYPE=URI:/info/1026/5193.htm END:VEVENT BEGIN:VEVENT UID:3904@kiaa.pku.edu.cn DTSTAMP:20171024T163849Z CREATED:20171024T163849Z DESCRIPTION:Gravitational Wave Seminar: The future of gravitational wave detection: the low frequency band DTSTART;TZID=Asia/Shanghai:20171102T150000 DTEND;TZID=Asia/Shanghai:20171102T170000 LAST-MODIFIED:20171024T163849Z LOCATION:Auditorium Room SUMMARY:Gravitational Wave Seminar: The future of gravitational wave detection: the low frequency band URL;TYPE=URI:/info/1030/3904.htm END:VEVENT BEGIN:VEVENT UID:4644@kiaa.pku.edu.cn DTSTAMP:20170915T154634Z CREATED:20170915T154634Z DESCRIPTION:Sagittarius A* and the Galactic Pulsar DTSTART;TZID=Asia/Shanghai:20171106T160000 DTEND;TZID=Asia/Shanghai:20171106T170000 LAST-MODIFIED:20170915T154634Z LOCATION:KIAA-PKU Auditorium SUMMARY:Sagittarius A* and the Galactic Pulsar URL;TYPE=URI:/info/1024/4644.htm END:VEVENT BEGIN:VEVENT UID:5189@kiaa.pku.edu.cn DTSTAMP:20170815T094855Z CREATED:20170815T094855Z DESCRIPTION:JCMT TAC meeting DTSTART;TZID=Asia/Shanghai:20171107T090000 DTEND;TZID=Asia/Shanghai:20171108T180000 LAST-MODIFIED:20170815T094855Z LOCATION:2nd meeting room, KIAA SUMMARY:JCMT TAC meeting URL;TYPE=URI:/info/1026/5189.htm END:VEVENT BEGIN:VEVENT UID:4771@kiaa.pku.edu.cn DTSTAMP:20171107T102840Z CREATED:20171107T102840Z DESCRIPTION:Postdoc internal discussion DTSTART;TZID=Asia/Shanghai:20171107T120000 DTEND;TZID=Asia/Shanghai:20171107T130000 LAST-MODIFIED:20171107T102840Z LOCATION:1st meeting room in KIAA SUMMARY:Postdoc internal discussion URL;TYPE=URI:/info/1028/4771.htm END:VEVENT BEGIN:VEVENT UID:5151@kiaa.pku.edu.cn DTSTAMP:20170918T110531Z CREATED:20170918T110531Z DESCRIPTION:High redshift starburst galaxies revealed by South Pole Telescope, ALMA, and gravitational lensing DTSTART;TZID=Asia/Shanghai:20171109T110000 DTEND;TZID=Asia/Shanghai:20171109T120000 LAST-MODIFIED:20170918T110531Z LOCATION:KIAA first floor meeting room SUMMARY:High redshift starburst galaxies revealed by South Pole Telescope, ALMA, and gravitational lensing URL;TYPE=URI:/info/1025/5151.htm END:VEVENT BEGIN:VEVENT UID:3912@kiaa.pku.edu.cn DTSTAMP:20171029T134555Z CREATED:20171029T134555Z DESCRIPTION:Gravitational Wave Seminar: Kilonovae from Neutron Star Mergers DTSTART;TZID=Asia/Shanghai:20171113T150000 DTEND;TZID=Asia/Shanghai:20171113T170000 LAST-MODIFIED:20171029T134555Z LOCATION:Auditorium, KIAA-PKU SUMMARY:Gravitational Wave Seminar: Kilonovae from Neutron Star Mergers URL;TYPE=URI:/info/1030/3912.htm END:VEVENT BEGIN:VEVENT UID:5191@kiaa.pku.edu.cn DTSTAMP:20170907T145752Z CREATED:20170907T145752Z DESCRIPTION:The 2017 KIAA-PKU Astrophysics Forum DTSTART;TZID=Asia/Shanghai:20171114T083000 DTEND;TZID=Asia/Shanghai:20171115T180000 LAST-MODIFIED:20170907T145752Z LOCATION:Auditorium, KIAA SUMMARY:The 2017 KIAA-PKU Astrophysics Forum URL;TYPE=URI:/info/1026/5191.htm END:VEVENT BEGIN:VEVENT UID:6687@kiaa.pku.edu.cn DTSTAMP:20171115T091706Z CREATED:20171115T091706Z DESCRIPTION:KIAA/DoA Family Photo DTSTART;TZID=Asia/Shanghai:20171116T133000 DTEND;TZID=Asia/Shanghai:20171116T133000 LAST-MODIFIED:20171115T091706Z LOCATION:KIAA SUMMARY:KIAA/DoA Family Photo URL;TYPE=URI:/info/1089/6687.htm END:VEVENT BEGIN:VEVENT UID:5192@kiaa.pku.edu.cn DTSTAMP:20171017T100432Z CREATED:20171017T100432Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20171116T140000 DTEND;TZID=Asia/Shanghai:20171116T153000 LAST-MODIFIED:20171017T100432Z LOCATION: SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1026/5192.htm END:VEVENT BEGIN:VEVENT UID:4645@kiaa.pku.edu.cn DTSTAMP:20170907T214358Z CREATED:20170907T214358Z DESCRIPTION:Early Results of the Subaru Hyper Suprime-Cam Survey for High Redshift Galaxies DTSTART;TZID=Asia/Shanghai:20171116T160000 DTEND;TZID=Asia/Shanghai:20171116T170000 LAST-MODIFIED:20170907T214358Z LOCATION:KIAA-PKU Auditorium SUMMARY:Early Results of the Subaru Hyper Suprime-Cam Survey for High Redshift Galaxies URL;TYPE=URI:/info/1024/4645.htm END:VEVENT BEGIN:VEVENT UID:4281@kiaa.pku.edu.cn DTSTAMP:20171119T143028Z CREATED:20171119T143028Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171121T133000 DTEND;TZID=Asia/Shanghai:20171121T140000 LAST-MODIFIED:20171119T143028Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4281.htm END:VEVENT BEGIN:VEVENT UID:4282@kiaa.pku.edu.cn DTSTAMP:20171119T143534Z CREATED:20171119T143534Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171123T133000 DTEND;TZID=Asia/Shanghai:20171123T140000 LAST-MODIFIED:20171119T143534Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4282.htm END:VEVENT BEGIN:VEVENT UID:4643@kiaa.pku.edu.cn DTSTAMP:20171025T234914Z CREATED:20171025T234914Z DESCRIPTION:A Golden Age for Astrometry - Uncovering the Secrets of the Milky Way DTSTART;TZID=Asia/Shanghai:20171123T160000 DTEND;TZID=Asia/Shanghai:20171123T170000 LAST-MODIFIED:20171025T234914Z LOCATION:KIAA-PKU Auditorium SUMMARY:A Golden Age for Astrometry - Uncovering the Secrets of the Milky Way URL;TYPE=URI:/info/1024/4643.htm END:VEVENT BEGIN:VEVENT UID:3905@kiaa.pku.edu.cn DTSTAMP:20171127T131110Z CREATED:20171127T131110Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171128T133000 DTEND;TZID=Asia/Shanghai:20171128T140000 LAST-MODIFIED:20171127T131110Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1030/3905.htm END:VEVENT BEGIN:VEVENT UID:3910@kiaa.pku.edu.cn DTSTAMP:20171118T092535Z CREATED:20171118T092535Z DESCRIPTION:Postdoc Science Day DTSTART;TZID=Asia/Shanghai:20171130T100000 DTEND;TZID=Asia/Shanghai:20171201T160000 LAST-MODIFIED:20171118T092535Z LOCATION:KIAA-PKU SUMMARY:Postdoc Science Day URL;TYPE=URI:/info/1030/3910.htm END:VEVENT BEGIN:VEVENT UID:4642@kiaa.pku.edu.cn DTSTAMP:20171026T210203Z CREATED:20171026T210203Z DESCRIPTION:Mid-J CO Line Emission in LIRGs DTSTART;TZID=Asia/Shanghai:20171130T160000 DTEND;TZID=Asia/Shanghai:20171130T170000 LAST-MODIFIED:20171026T210203Z LOCATION:KIAA-PKU Auditorium SUMMARY:Mid-J CO Line Emission in LIRGs URL;TYPE=URI:/info/1024/4642.htm END:VEVENT BEGIN:VEVENT UID:4283@kiaa.pku.edu.cn DTSTAMP:20171204T091816Z CREATED:20171204T091816Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171205T133000 DTEND;TZID=Asia/Shanghai:20171205T140000 LAST-MODIFIED:20171204T091816Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4283.htm END:VEVENT BEGIN:VEVENT UID:3913@kiaa.pku.edu.cn DTSTAMP:20171118T110600Z CREATED:20171118T110600Z DESCRIPTION:GW seminar: Challenges in Gravitational Wave Data Analysis DTSTART;TZID=Asia/Shanghai:20171205T150000 DTEND;TZID=Asia/Shanghai:20171205T170000 LAST-MODIFIED:20171118T110600Z LOCATION:KIAA-PKU auditorium room SUMMARY:GW seminar: Challenges in Gravitational Wave Data Analysis URL;TYPE=URI:/info/1030/3913.htm END:VEVENT BEGIN:VEVENT UID:5141@kiaa.pku.edu.cn DTSTAMP:20171204T085351Z CREATED:20171204T085351Z DESCRIPTION:On the Spin-axis Dynamics of Planets DTSTART;TZID=Asia/Shanghai:20171206T120000 DTEND;TZID=Asia/Shanghai:20171206T130000 LAST-MODIFIED:20171204T085351Z LOCATION:KIAA, 1st meeting room SUMMARY:On the Spin-axis Dynamics of Planets URL;TYPE=URI:/info/1025/5141.htm END:VEVENT BEGIN:VEVENT UID:4284@kiaa.pku.edu.cn DTSTAMP:20171204T234713Z CREATED:20171204T234713Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171207T133000 DTEND;TZID=Asia/Shanghai:20171207T140000 LAST-MODIFIED:20171204T234713Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4284.htm END:VEVENT BEGIN:VEVENT UID:4639@kiaa.pku.edu.cn DTSTAMP:20171120T150835Z CREATED:20171120T150835Z DESCRIPTION:Multiple Supernova Explosions from A Zombie Star DTSTART;TZID=Asia/Shanghai:20171208T150000 DTEND;TZID=Asia/Shanghai:20171208T160000 LAST-MODIFIED:20171120T150835Z LOCATION:KIAA-PKU Auditorium SUMMARY:Multiple Supernova Explosions from A Zombie Star URL;TYPE=URI:/info/1024/4639.htm END:VEVENT BEGIN:VEVENT UID:5146@kiaa.pku.edu.cn DTSTAMP:20171026T103735Z CREATED:20171026T103735Z DESCRIPTION:Molecular tracers of major starbursts in high-redshift lensed submillimeter galaxies DTSTART;TZID=Asia/Shanghai:20171211T120000 DTEND;TZID=Asia/Shanghai:20171211T130000 LAST-MODIFIED:20171026T103735Z LOCATION:DoA, Rm 2907 SUMMARY:Molecular tracers of major starbursts in high-redshift lensed submillimeter galaxies URL;TYPE=URI:/info/1025/5146.htm END:VEVENT BEGIN:VEVENT UID:4285@kiaa.pku.edu.cn DTSTAMP:20171208T091446Z CREATED:20171208T091446Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171212T133000 DTEND;TZID=Asia/Shanghai:20171212T140000 LAST-MODIFIED:20171208T091446Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4285.htm END:VEVENT BEGIN:VEVENT UID:5143@kiaa.pku.edu.cn DTSTAMP:20171120T130019Z CREATED:20171120T130019Z DESCRIPTION:The Gobbling Monsters within the Hot DOGs DTSTART;TZID=Asia/Shanghai:20171213T120000 DTEND;TZID=Asia/Shanghai:20171213T130000 LAST-MODIFIED:20171120T130019Z LOCATION:KIAA, 1st meeting room SUMMARY:The Gobbling Monsters within the Hot DOGs URL;TYPE=URI:/info/1025/5143.htm END:VEVENT BEGIN:VEVENT UID:4286@kiaa.pku.edu.cn DTSTAMP:20171211T223652Z CREATED:20171211T223652Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171214T133000 DTEND;TZID=Asia/Shanghai:20171214T140000 LAST-MODIFIED:20171211T223652Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4286.htm END:VEVENT BEGIN:VEVENT UID:4648@kiaa.pku.edu.cn DTSTAMP:20170620T164425Z CREATED:20170620T164425Z DESCRIPTION:Shedding Light on the Dark Cosmos through Gravitational Lensing DTSTART;TZID=Asia/Shanghai:20171214T160000 DTEND;TZID=Asia/Shanghai:20171214T170000 LAST-MODIFIED:20170620T164425Z LOCATION:KIAA-PKU Auditorium SUMMARY:Shedding Light on the Dark Cosmos through Gravitational Lensing URL;TYPE=URI:/info/1024/4648.htm END:VEVENT BEGIN:VEVENT UID:5142@kiaa.pku.edu.cn DTSTAMP:20171124T232956Z CREATED:20171124T232956Z DESCRIPTION:Probing the Copernican Principle: Are We Special? DTSTART;TZID=Asia/Shanghai:20171218T120000 DTEND;TZID=Asia/Shanghai:20171218T130000 LAST-MODIFIED:20171124T232956Z LOCATION:DoA, Rm 2907 SUMMARY:Probing the Copernican Principle: Are We Special? URL;TYPE=URI:/info/1025/5142.htm END:VEVENT BEGIN:VEVENT UID:4287@kiaa.pku.edu.cn DTSTAMP:20171217T163356Z CREATED:20171217T163356Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171219T133000 DTEND;TZID=Asia/Shanghai:20171219T140000 LAST-MODIFIED:20171217T163356Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4287.htm END:VEVENT BEGIN:VEVENT UID:3911@kiaa.pku.edu.cn DTSTAMP:20171029T134718Z CREATED:20171029T134718Z DESCRIPTION:Gravitational Wave Seminar: The gravitational capture of stellar-mass compact objects by supermassive and intermediate-mass black holes DTSTART;TZID=Asia/Shanghai:20171219T150000 DTEND;TZID=Asia/Shanghai:20171219T160000 LAST-MODIFIED:20171029T134718Z LOCATION:KIAA-PKU, Auditorium Room SUMMARY:Gravitational Wave Seminar: The gravitational capture of stellar-mass compact objects by supermassive and intermediate-mass black holes URL;TYPE=URI:/info/1030/3911.htm END:VEVENT BEGIN:VEVENT UID:5144@kiaa.pku.edu.cn DTSTAMP:20171115T144946Z CREATED:20171115T144946Z DESCRIPTION:Stellar Populations of Three Ultra Diffuse Galaxies in the Coma Cluster from the MaNGA Survey DTSTART;TZID=Asia/Shanghai:20171220T120000 DTEND;TZID=Asia/Shanghai:20171220T130000 LAST-MODIFIED:20171115T144946Z LOCATION:1st meeting room, KIAA SUMMARY:Stellar Populations of Three Ultra Diffuse Galaxies in the Coma Cluster from the MaNGA Survey URL;TYPE=URI:/info/1025/5144.htm END:VEVENT BEGIN:VEVENT UID:5140@kiaa.pku.edu.cn DTSTAMP:20171219T085509Z CREATED:20171219T085509Z DESCRIPTION:Graduate students lunch discussion with Lijing Shao DTSTART;TZID=Asia/Shanghai:20171220T150000 DTEND;TZID=Asia/Shanghai:20171220T160000 LAST-MODIFIED:20171219T085509Z LOCATION:1st meeting room, KIAA SUMMARY:Graduate students lunch discussion with Lijing Shao URL;TYPE=URI:/info/1025/5140.htm END:VEVENT BEGIN:VEVENT UID:4288@kiaa.pku.edu.cn DTSTAMP:20171219T082132Z CREATED:20171219T082132Z DESCRIPTION:astro-ph DTSTART;TZID=Asia/Shanghai:20171221T103000 DTEND;TZID=Asia/Shanghai:20171221T110000 LAST-MODIFIED:20171219T082132Z LOCATION: SUMMARY:astro-ph URL;TYPE=URI:/info/1027/4288.htm END:VEVENT BEGIN:VEVENT UID:5139@kiaa.pku.edu.cn DTSTAMP:20171219T085706Z CREATED:20171219T085706Z DESCRIPTION:Postdocs' Lunch with SHAO Lijing DTSTART;TZID=Asia/Shanghai:20171221T120000 DTEND;TZID=Asia/Shanghai:20171221T130000 LAST-MODIFIED:20171219T085706Z LOCATION:KIAA 2nd floor meeting room SUMMARY:Postdocs' Lunch with SHAO Lijing URL;TYPE=URI:/info/1025/5139.htm END:VEVENT BEGIN:VEVENT UID:4636@kiaa.pku.edu.cn DTSTAMP:20171218T084757Z CREATED:20171218T084757Z DESCRIPTION:Testing strong-field gravity with pulsars and GWs DTSTART;TZID=Asia/Shanghai:20171221T140000 DTEND;TZID=Asia/Shanghai:20171221T150000 LAST-MODIFIED:20171218T084757Z LOCATION:KIAA-PKU Auditorium SUMMARY:Testing strong-field gravity with pulsars and GWs URL;TYPE=URI:/info/1024/4636.htm END:VEVENT BEGIN:VEVENT UID:4640@kiaa.pku.edu.cn DTSTAMP:20171105T165409Z CREATED:20171105T165409Z DESCRIPTION:Origin of broad-line regions: from torus to accretion disks DTSTART;TZID=Asia/Shanghai:20171221T160000 DTEND;TZID=Asia/Shanghai:20171221T170000 LAST-MODIFIED:20171105T165409Z LOCATION:KIAA-PKU Auditorium SUMMARY:Origin of broad-line regions: from torus to accretion disks URL;TYPE=URI:/info/1024/4640.htm END:VEVENT BEGIN:VEVENT UID:6688@kiaa.pku.edu.cn DTSTAMP:20171218T085550Z CREATED:20171218T085550Z DESCRIPTION:KIAA& DoA Evening Party DTSTART;TZID=Asia/Shanghai:20171222T183000 DTEND;TZID=Asia/Shanghai:20171222T183000 LAST-MODIFIED:20171218T085550Z LOCATION:KIAA Auditorium SUMMARY:KIAA& DoA Evening Party URL;TYPE=URI:/info/1089/6688.htm END:VEVENT BEGIN:VEVENT UID:4289@kiaa.pku.edu.cn DTSTAMP:20171224T104419Z CREATED:20171224T104419Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20171226T133000 DTEND;TZID=Asia/Shanghai:20171226T140000 LAST-MODIFIED:20171224T104419Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4289.htm END:VEVENT BEGIN:VEVENT UID:4290@kiaa.pku.edu.cn DTSTAMP:20171228T091748Z CREATED:20171228T091748Z DESCRIPTION:astro-ph DTSTART;TZID=Asia/Shanghai:20171228T133000 DTEND;TZID=Asia/Shanghai:20171228T140000 LAST-MODIFIED:20171228T091748Z LOCATION: SUMMARY:astro-ph URL;TYPE=URI:/info/1027/4290.htm END:VEVENT BEGIN:VEVENT UID:4641@kiaa.pku.edu.cn DTSTAMP:20171031T022015Z CREATED:20171031T022015Z DESCRIPTION:Close Major-Merger Pairs Since z=1: Evolution of Merger Rate & SFR Enhancement DTSTART;TZID=Asia/Shanghai:20171228T160000 DTEND;TZID=Asia/Shanghai:20171228T170000 LAST-MODIFIED:20171031T022015Z LOCATION:KIAA-PKU Auditorium SUMMARY:Close Major-Merger Pairs Since z=1: Evolution of Merger Rate & SFR Enhancement URL;TYPE=URI:/info/1024/4641.htm END:VEVENT BEGIN:VEVENT UID:5204@kiaa.pku.edu.cn DTSTAMP:20171229T084115Z CREATED:20171229T084115Z DESCRIPTION:Mid-term Report for Undergraduate Thesis DTSTART;TZID=Asia/Shanghai:20171229T083000 DTEND;TZID=Asia/Shanghai:20171229T120000 LAST-MODIFIED:20171229T084115Z LOCATION:KIAA Auditorium SUMMARY:Mid-term Report for Undergraduate Thesis URL;TYPE=URI:/info/1026/5204.htm END:VEVENT BEGIN:VEVENT UID:6682@kiaa.pku.edu.cn DTSTAMP:20170523T163529Z CREATED:20170523T163529Z DESCRIPTION:New Year's Holiday DTSTART;TZID=Asia/Shanghai:20180101T000000 DTEND;TZID=Asia/Shanghai:20180101T000000 LAST-MODIFIED:20170523T163529Z LOCATION: SUMMARY:New Year's Holiday URL;TYPE=URI:/info/1089/6682.htm END:VEVENT BEGIN:VEVENT UID:5145@kiaa.pku.edu.cn DTSTAMP:20171113T113711Z CREATED:20171113T113711Z DESCRIPTION:Cloud Atlas: Rotational Modulations in Planetary Mass/Brown Dwarf Companions DTSTART;TZID=Asia/Shanghai:20180103T120000 DTEND;TZID=Asia/Shanghai:20180103T130000 LAST-MODIFIED:20171113T113711Z LOCATION:KIAA, 1st meeting room SUMMARY:Cloud Atlas: Rotational Modulations in Planetary Mass/Brown Dwarf Companions URL;TYPE=URI:/info/1025/5145.htm END:VEVENT BEGIN:VEVENT UID:6689@kiaa.pku.edu.cn DTSTAMP:20180105T164800Z CREATED:20180105T164800Z DESCRIPTION:Grad Students Annual Reports and PhD Qualification Exam DTSTART;TZID=Asia/Shanghai:20180108T080000 DTEND;TZID=Asia/Shanghai:20180108T180000 LAST-MODIFIED:20180105T164800Z LOCATION:1st meeting room, KIAA SUMMARY:Grad Students Annual Reports and PhD Qualification Exam URL;TYPE=URI:/info/1089/6689.htm END:VEVENT BEGIN:VEVENT UID:4819@kiaa.pku.edu.cn DTSTAMP:20180502T111714Z CREATED:20180502T111714Z DESCRIPTION:Stellar variability and Pre-main-sequence evolution of young stellar objects DTSTART;TZID=Asia/Shanghai:20180110T170000 DTEND;TZID=Asia/Shanghai:20180110T180000 LAST-MODIFIED:20180502T111714Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Stellar variability and Pre-main-sequence evolution of young stellar objects URL;TYPE=URI:/info/1029/4819.htm END:VEVENT BEGIN:VEVENT UID:4818@kiaa.pku.edu.cn DTSTAMP:20180102T084211Z CREATED:20180102T084211Z DESCRIPTION:Graduate Dinner Talk: Stellar variability and Pre-main-sequence evolution of young stellar objects DTSTART;TZID=Asia/Shanghai:20180110T170000 DTEND;TZID=Asia/Shanghai:20180110T180000 LAST-MODIFIED:20180102T084211Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Graduate Dinner Talk: Stellar variability and Pre-main-sequence evolution of young stellar objects URL;TYPE=URI:/info/1029/4818.htm END:VEVENT BEGIN:VEVENT UID:4638@kiaa.pku.edu.cn DTSTAMP:20171207T105753Z CREATED:20171207T105753Z DESCRIPTION:The initial value problem of general relativity and applications in astrophysics DTSTART;TZID=Asia/Shanghai:20180111T160000 DTEND;TZID=Asia/Shanghai:20180111T170000 LAST-MODIFIED:20171207T105753Z LOCATION:KIAA-PKU Auditorium SUMMARY:The initial value problem of general relativity and applications in astrophysics URL;TYPE=URI:/info/1024/4638.htm END:VEVENT BEGIN:VEVENT UID:5132@kiaa.pku.edu.cn DTSTAMP:20180115T084855Z CREATED:20180115T084855Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180115T120000 DTEND;TZID=Asia/Shanghai:20180115T130000 LAST-MODIFIED:20180115T084855Z LOCATION:1st meeting room, KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5132.htm END:VEVENT BEGIN:VEVENT UID:4633@kiaa.pku.edu.cn DTSTAMP:20180102T113149Z CREATED:20180102T113149Z DESCRIPTION:Recent advances in Planet Formation DTSTART;TZID=Asia/Shanghai:20180115T160000 DTEND;TZID=Asia/Shanghai:20180115T170000 LAST-MODIFIED:20180102T113149Z LOCATION:KIAA-PKU Auditorium SUMMARY:Recent advances in Planet Formation URL;TYPE=URI:/info/1024/4633.htm END:VEVENT BEGIN:VEVENT UID:5138@kiaa.pku.edu.cn DTSTAMP:20180102T123453Z CREATED:20180102T123453Z DESCRIPTION:Lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180116T120000 DTEND;TZID=Asia/Shanghai:20180116T130000 LAST-MODIFIED:20180102T123453Z LOCATION:1st floor meeting room SUMMARY:Lunch discussion with postdocs URL;TYPE=URI:/info/1025/5138.htm END:VEVENT BEGIN:VEVENT UID:5131@kiaa.pku.edu.cn DTSTAMP:20180115T085000Z CREATED:20180115T085000Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180116T120000 DTEND;TZID=Asia/Shanghai:20180116T130000 LAST-MODIFIED:20180115T085000Z LOCATION:1st meeting room,KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5131.htm END:VEVENT BEGIN:VEVENT UID:4635@kiaa.pku.edu.cn DTSTAMP:20171228T100713Z CREATED:20171228T100713Z DESCRIPTION:Probing the origins of astroparticles in the multi-messenger era  DTSTART;TZID=Asia/Shanghai:20180116T160000 DTEND;TZID=Asia/Shanghai:20180116T170000 LAST-MODIFIED:20171228T100713Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing the origins of astroparticles in the multi-messenger era  URL;TYPE=URI:/info/1024/4635.htm END:VEVENT BEGIN:VEVENT UID:5130@kiaa.pku.edu.cn DTSTAMP:20180115T085158Z CREATED:20180115T085158Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180117T120000 DTEND;TZID=Asia/Shanghai:20180117T130000 LAST-MODIFIED:20180115T085158Z LOCATION:1st meeting room, KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5130.htm END:VEVENT BEGIN:VEVENT UID:5137@kiaa.pku.edu.cn DTSTAMP:20180102T123620Z CREATED:20180102T123620Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180117T120000 DTEND;TZID=Asia/Shanghai:20180117T130000 LAST-MODIFIED:20180102T123620Z LOCATION:1st floor meeting room SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5137.htm END:VEVENT BEGIN:VEVENT UID:4630@kiaa.pku.edu.cn DTSTAMP:20180105T144410Z CREATED:20180105T144410Z DESCRIPTION:Black hole evolution: from stellar mass to ultra-massive ones DTSTART;TZID=Asia/Shanghai:20180117T160000 DTEND;TZID=Asia/Shanghai:20180117T170000 LAST-MODIFIED:20180105T144410Z LOCATION:KIAA-PKU Auditorium SUMMARY:Black hole evolution: from stellar mass to ultra-massive ones URL;TYPE=URI:/info/1024/4630.htm END:VEVENT BEGIN:VEVENT UID:5136@kiaa.pku.edu.cn DTSTAMP:20180102T123713Z CREATED:20180102T123713Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180118T120000 DTEND;TZID=Asia/Shanghai:20180118T130000 LAST-MODIFIED:20180102T123713Z LOCATION:1st floor meeting room SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5136.htm END:VEVENT BEGIN:VEVENT UID:5129@kiaa.pku.edu.cn DTSTAMP:20180115T085606Z CREATED:20180115T085606Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180118T120000 DTEND;TZID=Asia/Shanghai:20180118T130000 LAST-MODIFIED:20180115T085606Z LOCATION:1st meeting room,KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5129.htm END:VEVENT BEGIN:VEVENT UID:4634@kiaa.pku.edu.cn DTSTAMP:20180102T093405Z CREATED:20180102T093405Z DESCRIPTION:Probing the Cosmos through Gravitational Lensing DTSTART;TZID=Asia/Shanghai:20180118T160000 DTEND;TZID=Asia/Shanghai:20180118T170000 LAST-MODIFIED:20180102T093405Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing the Cosmos through Gravitational Lensing URL;TYPE=URI:/info/1024/4634.htm END:VEVENT BEGIN:VEVENT UID:5135@kiaa.pku.edu.cn DTSTAMP:20180102T123758Z CREATED:20180102T123758Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180119T120000 DTEND;TZID=Asia/Shanghai:20180119T130000 LAST-MODIFIED:20180102T123758Z LOCATION:1st floor meeting room SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5135.htm END:VEVENT BEGIN:VEVENT UID:5134@kiaa.pku.edu.cn DTSTAMP:20180102T123833Z CREATED:20180102T123833Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180122T120000 DTEND;TZID=Asia/Shanghai:20180122T130000 LAST-MODIFIED:20180102T123833Z LOCATION:1st floor meeting room SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5134.htm END:VEVENT BEGIN:VEVENT UID:5128@kiaa.pku.edu.cn DTSTAMP:20180115T085655Z CREATED:20180115T085655Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180122T120000 DTEND;TZID=Asia/Shanghai:20180122T130000 LAST-MODIFIED:20180115T085655Z LOCATION:1st meeting room, KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5128.htm END:VEVENT BEGIN:VEVENT UID:4631@kiaa.pku.edu.cn DTSTAMP:20180105T093105Z CREATED:20180105T093105Z DESCRIPTION:Galaxy Formation through the Dark Ages Until Today DTSTART;TZID=Asia/Shanghai:20180122T160000 DTEND;TZID=Asia/Shanghai:20180122T170000 LAST-MODIFIED:20180105T093105Z LOCATION:KIAA-PKU Auditorium SUMMARY:Galaxy Formation through the Dark Ages Until Today URL;TYPE=URI:/info/1024/4631.htm END:VEVENT BEGIN:VEVENT UID:5133@kiaa.pku.edu.cn DTSTAMP:20180102T123902Z CREATED:20180102T123902Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20180123T120000 DTEND;TZID=Asia/Shanghai:20180123T130000 LAST-MODIFIED:20180102T123902Z LOCATION:1st floor meeting room SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5133.htm END:VEVENT BEGIN:VEVENT UID:5127@kiaa.pku.edu.cn DTSTAMP:20180115T085736Z CREATED:20180115T085736Z DESCRIPTION:Lunch discussion with grad students DTSTART;TZID=Asia/Shanghai:20180123T120000 DTEND;TZID=Asia/Shanghai:20180123T130000 LAST-MODIFIED:20180115T085736Z LOCATION:1st meeting room, KIAA SUMMARY:Lunch discussion with grad students URL;TYPE=URI:/info/1025/5127.htm END:VEVENT BEGIN:VEVENT UID:4632@kiaa.pku.edu.cn DTSTAMP:20180104T165417Z CREATED:20180104T165417Z DESCRIPTION:The Dawn of Star Formation: revealing the initial conditions for massive star formation throughout the Milky Way DTSTART;TZID=Asia/Shanghai:20180123T160000 DTEND;TZID=Asia/Shanghai:20180123T170000 LAST-MODIFIED:20180104T165417Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Dawn of Star Formation: revealing the initial conditions for massive star formation throughout the Milky Way URL;TYPE=URI:/info/1024/4632.htm END:VEVENT BEGIN:VEVENT UID:6681@kiaa.pku.edu.cn DTSTAMP:20170523T163342Z CREATED:20170523T163342Z DESCRIPTION:Winter holidys for faculty & Admin staff DTSTART;TZID=Asia/Shanghai:20180124T000000 DTEND;TZID=Asia/Shanghai:20180214T000000 LAST-MODIFIED:20170523T163342Z LOCATION: SUMMARY:Winter holidys for faculty & Admin staff URL;TYPE=URI:/info/1089/6681.htm END:VEVENT BEGIN:VEVENT UID:6695@kiaa.pku.edu.cn DTSTAMP:20180109T161922Z CREATED:20180109T161922Z DESCRIPTION:Spring Festival Holiday DTSTART;TZID=Asia/Shanghai:20180215T000000 DTEND;TZID=Asia/Shanghai:20180221T000000 LAST-MODIFIED:20180109T161922Z LOCATION: SUMMARY:Spring Festival Holiday URL;TYPE=URI:/info/1089/6695.htm END:VEVENT BEGIN:VEVENT UID:5124@kiaa.pku.edu.cn DTSTAMP:20180304T093147Z CREATED:20180304T093147Z DESCRIPTION:Star Streams as Dark Matter Detectors DTSTART;TZID=Asia/Shanghai:20180306T120000 DTEND;TZID=Asia/Shanghai:20180306T130000 LAST-MODIFIED:20180304T093147Z LOCATION:KIAA 1st meeting room SUMMARY:Star Streams as Dark Matter Detectors URL;TYPE=URI:/info/1025/5124.htm END:VEVENT BEGIN:VEVENT UID:4820@kiaa.pku.edu.cn DTSTAMP:20180502T112032Z CREATED:20180502T112032Z DESCRIPTION:Understanding the galaxy evolution with gaseous halos DTSTART;TZID=Asia/Shanghai:20180306T170000 DTEND;TZID=Asia/Shanghai:20180306T180000 LAST-MODIFIED:20180502T112032Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Understanding the galaxy evolution with gaseous halos URL;TYPE=URI:/info/1029/4820.htm END:VEVENT BEGIN:VEVENT UID:5125@kiaa.pku.edu.cn DTSTAMP:20180301T161718Z CREATED:20180301T161718Z DESCRIPTION:High-mass star formation studies in ALMA era and the TOP-SCOPE survey of Planck cold clumps DTSTART;TZID=Asia/Shanghai:20180309T120000 DTEND;TZID=Asia/Shanghai:20180309T130000 LAST-MODIFIED:20180301T161718Z LOCATION:1st floor meeting room, KIAA SUMMARY:High-mass star formation studies in ALMA era and the TOP-SCOPE survey of Planck cold clumps URL;TYPE=URI:/info/1025/5125.htm END:VEVENT BEGIN:VEVENT UID:4766@kiaa.pku.edu.cn DTSTAMP:20171107T134048Z CREATED:20171107T134048Z DESCRIPTION:The SkyMapper Southern Survey DTSTART;TZID=Asia/Shanghai:20180313T120000 DTEND;TZID=Asia/Shanghai:20180313T130000 LAST-MODIFIED:20171107T134048Z LOCATION:KIAA-PKU SUMMARY:The SkyMapper Southern Survey URL;TYPE=URI:/info/1028/4766.htm END:VEVENT BEGIN:VEVENT UID:4291@kiaa.pku.edu.cn DTSTAMP:20180305T111701Z CREATED:20180305T111701Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180313T133000 DTEND;TZID=Asia/Shanghai:20180313T140000 LAST-MODIFIED:20180305T111701Z LOCATION:KIAA second floor open area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4291.htm END:VEVENT BEGIN:VEVENT UID:4629@kiaa.pku.edu.cn DTSTAMP:20180118T180644Z CREATED:20180118T180644Z DESCRIPTION:Exploring the very early universe with CMB observations DTSTART;TZID=Asia/Shanghai:20180313T160000 DTEND;TZID=Asia/Shanghai:20180313T170000 LAST-MODIFIED:20180118T180644Z LOCATION:KIAA-PKU Auditorium SUMMARY:Exploring the very early universe with CMB observations URL;TYPE=URI:/info/1024/4629.htm END:VEVENT BEGIN:VEVENT UID:4293@kiaa.pku.edu.cn DTSTAMP:20180316T091718Z CREATED:20180316T091718Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180315T133000 DTEND;TZID=Asia/Shanghai:20180315T140000 LAST-MODIFIED:20180316T091718Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4293.htm END:VEVENT BEGIN:VEVENT UID:4821@kiaa.pku.edu.cn DTSTAMP:20180502T112139Z CREATED:20180502T112139Z DESCRIPTION:The origin of ultrahigh energy cosmic ray nuclei DTSTART;TZID=Asia/Shanghai:20180316T170000 DTEND;TZID=Asia/Shanghai:20180316T180000 LAST-MODIFIED:20180502T112139Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The origin of ultrahigh energy cosmic ray nuclei URL;TYPE=URI:/info/1029/4821.htm END:VEVENT BEGIN:VEVENT UID:4769@kiaa.pku.edu.cn DTSTAMP:20171107T133132Z CREATED:20171107T133132Z DESCRIPTION:A type II supernova with a "perfect" linear decline DTSTART;TZID=Asia/Shanghai:20180320T120000 DTEND;TZID=Asia/Shanghai:20180320T130000 LAST-MODIFIED:20171107T133132Z LOCATION:KIAA-PKU SUMMARY:A type II supernova with a "perfect" linear decline URL;TYPE=URI:/info/1028/4769.htm END:VEVENT BEGIN:VEVENT UID:4292@kiaa.pku.edu.cn DTSTAMP:20180316T091535Z CREATED:20180316T091535Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180320T133000 DTEND;TZID=Asia/Shanghai:20180320T140000 LAST-MODIFIED:20180316T091535Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4292.htm END:VEVENT BEGIN:VEVENT UID:5123@kiaa.pku.edu.cn DTSTAMP:20180316T171050Z CREATED:20180316T171050Z DESCRIPTION:Imminent Design Choices for the Thirty Meter Telescope's Wide Field Optical Spectrograph DTSTART;TZID=Asia/Shanghai:20180321T120000 DTEND;TZID=Asia/Shanghai:20180321T130000 LAST-MODIFIED:20180316T171050Z LOCATION:KIAA, 1st meeting room SUMMARY:Imminent Design Choices for the Thirty Meter Telescope's Wide Field Optical Spectrograph URL;TYPE=URI:/info/1025/5123.htm END:VEVENT BEGIN:VEVENT UID:4626@kiaa.pku.edu.cn DTSTAMP:20180312T105759Z CREATED:20180312T105759Z DESCRIPTION:Binary evolution and its applications DTSTART;TZID=Asia/Shanghai:20180322T100000 DTEND;TZID=Asia/Shanghai:20180322T100000 LAST-MODIFIED:20180312T105759Z LOCATION:KIAA-PKU Auditorium SUMMARY:Binary evolution and its applications URL;TYPE=URI:/info/1024/4626.htm END:VEVENT BEGIN:VEVENT UID:4294@kiaa.pku.edu.cn DTSTAMP:20180322T085833Z CREATED:20180322T085833Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180322T133000 DTEND;TZID=Asia/Shanghai:20180322T140000 LAST-MODIFIED:20180322T085833Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4294.htm END:VEVENT BEGIN:VEVENT UID:4822@kiaa.pku.edu.cn DTSTAMP:20180502T112404Z CREATED:20180502T112404Z DESCRIPTION:Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars DTSTART;TZID=Asia/Shanghai:20180323T170000 DTEND;TZID=Asia/Shanghai:20180323T180000 LAST-MODIFIED:20180502T112404Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars URL;TYPE=URI:/info/1029/4822.htm END:VEVENT BEGIN:VEVENT UID:5126@kiaa.pku.edu.cn DTSTAMP:20180206T121400Z CREATED:20180206T121400Z DESCRIPTION:AR Sco: the First White Dwarf Pulsar DTSTART;TZID=Asia/Shanghai:20180326T120000 DTEND;TZID=Asia/Shanghai:20180326T130000 LAST-MODIFIED:20180206T121400Z LOCATION:DOA,Rm 2907 SUMMARY:AR Sco: the First White Dwarf Pulsar URL;TYPE=URI:/info/1025/5126.htm END:VEVENT BEGIN:VEVENT UID:4768@kiaa.pku.edu.cn DTSTAMP:20171107T133540Z CREATED:20171107T133540Z DESCRIPTION:Discussion: Radio jet/outflow in Super-Eddington accreting SMBHs? DTSTART;TZID=Asia/Shanghai:20180327T120000 DTEND;TZID=Asia/Shanghai:20180327T130000 LAST-MODIFIED:20171107T133540Z LOCATION:KIAA-PKU SUMMARY:Discussion: Radio jet/outflow in Super-Eddington accreting SMBHs? URL;TYPE=URI:/info/1028/4768.htm END:VEVENT BEGIN:VEVENT UID:4295@kiaa.pku.edu.cn DTSTAMP:20180327T092548Z CREATED:20180327T092548Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180327T133000 DTEND;TZID=Asia/Shanghai:20180327T140000 LAST-MODIFIED:20180327T092548Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4295.htm END:VEVENT BEGIN:VEVENT UID:4296@kiaa.pku.edu.cn DTSTAMP:20180328T093716Z CREATED:20180328T093716Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180329T133000 DTEND;TZID=Asia/Shanghai:20180329T140000 LAST-MODIFIED:20180328T093716Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4296.htm END:VEVENT BEGIN:VEVENT UID:4627@kiaa.pku.edu.cn DTSTAMP:20180121T143649Z CREATED:20180121T143649Z DESCRIPTION:Ultra-high energy cosmic rays from low-luminosity GRBs DTSTART;TZID=Asia/Shanghai:20180329T160000 DTEND;TZID=Asia/Shanghai:20180329T170000 LAST-MODIFIED:20180121T143649Z LOCATION:KIAA-PKU Auditorium SUMMARY:Ultra-high energy cosmic rays from low-luminosity GRBs URL;TYPE=URI:/info/1024/4627.htm END:VEVENT BEGIN:VEVENT UID:5122@kiaa.pku.edu.cn DTSTAMP:20180319T103030Z CREATED:20180319T103030Z DESCRIPTION:A Tale of Two Bursts DTSTART;TZID=Asia/Shanghai:20180330T120000 DTEND;TZID=Asia/Shanghai:20180330T130000 LAST-MODIFIED:20180319T103030Z LOCATION:KIAA, 1st meeting room SUMMARY:A Tale of Two Bursts URL;TYPE=URI:/info/1025/5122.htm END:VEVENT BEGIN:VEVENT UID:4823@kiaa.pku.edu.cn DTSTAMP:20180502T112538Z CREATED:20180502T112538Z DESCRIPTION:Hierarchical Star Formation in the Magellanic Clouds - a study based on the VMC survey DTSTART;TZID=Asia/Shanghai:20180330T170000 DTEND;TZID=Asia/Shanghai:20180330T180000 LAST-MODIFIED:20180502T112538Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Hierarchical Star Formation in the Magellanic Clouds - a study based on the VMC survey URL;TYPE=URI:/info/1029/4823.htm END:VEVENT BEGIN:VEVENT UID:4297@kiaa.pku.edu.cn DTSTAMP:20180402T102648Z CREATED:20180402T102648Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180403T133000 DTEND;TZID=Asia/Shanghai:20180403T140000 LAST-MODIFIED:20180402T102648Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4297.htm END:VEVENT BEGIN:VEVENT UID:3914@kiaa.pku.edu.cn DTSTAMP:20180328T093125Z CREATED:20180328T093125Z DESCRIPTION:GW Seminar: Numerical Relativity and the Evolution of Compact Binary Spacetimes DTSTART;TZID=Asia/Shanghai:20180403T150000 DTEND;TZID=Asia/Shanghai:20180403T170000 LAST-MODIFIED:20180328T093125Z LOCATION:KIAA auditorium room SUMMARY:GW Seminar: Numerical Relativity and the Evolution of Compact Binary Spacetimes URL;TYPE=URI:/info/1030/3914.htm END:VEVENT BEGIN:VEVENT UID:4625@kiaa.pku.edu.cn DTSTAMP:20180322T171509Z CREATED:20180322T171509Z DESCRIPTION:Circumbinary Accretion: From Supermassive Binary Black Holes to Circumbinary Planets DTSTART;TZID=Asia/Shanghai:20180404T160000 DTEND;TZID=Asia/Shanghai:20180404T170000 LAST-MODIFIED:20180322T171509Z LOCATION:KIAA-PKU Auditorium SUMMARY:Circumbinary Accretion: From Supermassive Binary Black Holes to Circumbinary Planets URL;TYPE=URI:/info/1024/4625.htm END:VEVENT BEGIN:VEVENT UID:6690@kiaa.pku.edu.cn DTSTAMP:20180109T161222Z CREATED:20180109T161222Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20180405T000000 DTEND;TZID=Asia/Shanghai:20180405T000000 LAST-MODIFIED:20180109T161222Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6690.htm END:VEVENT BEGIN:VEVENT UID:5203@kiaa.pku.edu.cn DTSTAMP:20180409T084158Z CREATED:20180409T084158Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20180409T100000 DTEND;TZID=Asia/Shanghai:20180409T120000 LAST-MODIFIED:20180409T084158Z LOCATION:1st meeting room, KIAA SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1026/5203.htm END:VEVENT BEGIN:VEVENT UID:4298@kiaa.pku.edu.cn DTSTAMP:20180402T102806Z CREATED:20180402T102806Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180410T133000 DTEND;TZID=Asia/Shanghai:20180410T140000 LAST-MODIFIED:20180402T102806Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4298.htm END:VEVENT BEGIN:VEVENT UID:4299@kiaa.pku.edu.cn DTSTAMP:20180410T082759Z CREATED:20180410T082759Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180412T133000 DTEND;TZID=Asia/Shanghai:20180412T140000 LAST-MODIFIED:20180410T082759Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4299.htm END:VEVENT BEGIN:VEVENT UID:4623@kiaa.pku.edu.cn DTSTAMP:20180323T172110Z CREATED:20180323T172110Z DESCRIPTION:The halo of the Milky Way DTSTART;TZID=Asia/Shanghai:20180412T160000 DTEND;TZID=Asia/Shanghai:20180412T170000 LAST-MODIFIED:20180323T172110Z LOCATION:KIAA-PKU Auditorium SUMMARY:The halo of the Milky Way URL;TYPE=URI:/info/1024/4623.htm END:VEVENT BEGIN:VEVENT UID:4824@kiaa.pku.edu.cn DTSTAMP:20180502T113241Z CREATED:20180502T113241Z DESCRIPTION:Simulation of spot behavior on the Seven Sisters (Pleiades): do we mislead by K2 lightcurves? DTSTART;TZID=Asia/Shanghai:20180413T170000 DTEND;TZID=Asia/Shanghai:20180413T180000 LAST-MODIFIED:20180502T113241Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Simulation of spot behavior on the Seven Sisters (Pleiades): do we mislead by K2 lightcurves? URL;TYPE=URI:/info/1029/4824.htm END:VEVENT BEGIN:VEVENT UID:4300@kiaa.pku.edu.cn DTSTAMP:20180416T221427Z CREATED:20180416T221427Z DESCRIPTION:Astro-phs DTSTART;TZID=Asia/Shanghai:20180417T133000 DTEND;TZID=Asia/Shanghai:20180417T140000 LAST-MODIFIED:20180416T221427Z LOCATION:KIAA second floor, common area SUMMARY:Astro-phs URL;TYPE=URI:/info/1027/4300.htm END:VEVENT BEGIN:VEVENT UID:4301@kiaa.pku.edu.cn DTSTAMP:20180418T213929Z CREATED:20180418T213929Z DESCRIPTION:Astro-phs DTSTART;TZID=Asia/Shanghai:20180419T133000 DTEND;TZID=Asia/Shanghai:20180419T140000 LAST-MODIFIED:20180418T213929Z LOCATION: SUMMARY:Astro-phs URL;TYPE=URI:/info/1027/4301.htm END:VEVENT BEGIN:VEVENT UID:4622@kiaa.pku.edu.cn DTSTAMP:20180327T095116Z CREATED:20180327T095116Z DESCRIPTION:Introduction to Insight-HXMT: China’s first X-ray Astronomy Satellite DTSTART;TZID=Asia/Shanghai:20180419T160000 DTEND;TZID=Asia/Shanghai:20180419T170000 LAST-MODIFIED:20180327T095116Z LOCATION:KIAA-PKU Auditorium SUMMARY:Introduction to Insight-HXMT: China’s first X-ray Astronomy Satellite URL;TYPE=URI:/info/1024/4622.htm END:VEVENT BEGIN:VEVENT UID:5121@kiaa.pku.edu.cn DTSTAMP:20180328T172010Z CREATED:20180328T172010Z DESCRIPTION:The missing links of neutron star evolution in the eROSITA All-Sky Survey DTSTART;TZID=Asia/Shanghai:20180423T120000 DTEND;TZID=Asia/Shanghai:20180423T130000 LAST-MODIFIED:20180328T172010Z LOCATION:DoA, Rm 2907 SUMMARY:The missing links of neutron star evolution in the eROSITA All-Sky Survey URL;TYPE=URI:/info/1025/5121.htm END:VEVENT BEGIN:VEVENT UID:4767@kiaa.pku.edu.cn DTSTAMP:20171107T133709Z CREATED:20171107T133709Z DESCRIPTION:Evolution of Gas in Spiral Galaxies DTSTART;TZID=Asia/Shanghai:20180424T120000 DTEND;TZID=Asia/Shanghai:20180424T130000 LAST-MODIFIED:20171107T133709Z LOCATION:KIAA-PKU SUMMARY:Evolution of Gas in Spiral Galaxies URL;TYPE=URI:/info/1028/4767.htm END:VEVENT BEGIN:VEVENT UID:4302@kiaa.pku.edu.cn DTSTAMP:20180423T215329Z CREATED:20180423T215329Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180424T133000 DTEND;TZID=Asia/Shanghai:20180424T140000 LAST-MODIFIED:20180423T215329Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4302.htm END:VEVENT BEGIN:VEVENT UID:4825@kiaa.pku.edu.cn DTSTAMP:20180502T113352Z CREATED:20180502T113352Z DESCRIPTION:ALMA survey of protoplanetary disks in Chamaeleon I: Dust and Gas Masses DTSTART;TZID=Asia/Shanghai:20180425T171500 DTEND;TZID=Asia/Shanghai:20180425T181500 LAST-MODIFIED:20180502T113352Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:ALMA survey of protoplanetary disks in Chamaeleon I: Dust and Gas Masses URL;TYPE=URI:/info/1029/4825.htm END:VEVENT BEGIN:VEVENT UID:4303@kiaa.pku.edu.cn DTSTAMP:20180427T094530Z CREATED:20180427T094530Z DESCRIPTION:astro-ph DTSTART;TZID=Asia/Shanghai:20180426T133000 DTEND;TZID=Asia/Shanghai:20180426T140000 LAST-MODIFIED:20180427T094530Z LOCATION: SUMMARY:astro-ph URL;TYPE=URI:/info/1027/4303.htm END:VEVENT BEGIN:VEVENT UID:4624@kiaa.pku.edu.cn DTSTAMP:20180323T171937Z CREATED:20180323T171937Z DESCRIPTION:The Dark Age and Cosmic Dawn DTSTART;TZID=Asia/Shanghai:20180426T160000 DTEND;TZID=Asia/Shanghai:20180426T170000 LAST-MODIFIED:20180323T171937Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Dark Age and Cosmic Dawn URL;TYPE=URI:/info/1024/4624.htm END:VEVENT BEGIN:VEVENT UID:6691@kiaa.pku.edu.cn DTSTAMP:20180109T161344Z CREATED:20180109T161344Z DESCRIPTION:Labor Day Holiday DTSTART;TZID=Asia/Shanghai:20180501T000000 DTEND;TZID=Asia/Shanghai:20180501T000000 LAST-MODIFIED:20180109T161344Z LOCATION: SUMMARY:Labor Day Holiday URL;TYPE=URI:/info/1089/6691.htm END:VEVENT BEGIN:VEVENT UID:4628@kiaa.pku.edu.cn DTSTAMP:20180119T224504Z CREATED:20180119T224504Z DESCRIPTION:Probing Cosmic Reionization with Lyman Alpha Galaxies DTSTART;TZID=Asia/Shanghai:20180503T160000 DTEND;TZID=Asia/Shanghai:20180503T170000 LAST-MODIFIED:20180119T224504Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing Cosmic Reionization with Lyman Alpha Galaxies URL;TYPE=URI:/info/1024/4628.htm END:VEVENT BEGIN:VEVENT UID:4569@kiaa.pku.edu.cn DTSTAMP:20180430T091732Z CREATED:20180430T091732Z DESCRIPTION:Opportunities in next generation multi-object spectroscopy: the science and status of the Maunakea Spectroscopic Explorer (MSE) DTSTART;TZID=Asia/Shanghai:20180507T160000 DTEND;TZID=Asia/Shanghai:20180507T170000 LAST-MODIFIED:20180430T091732Z LOCATION:KIAA-PKU Auditorium SUMMARY:Opportunities in next generation multi-object spectroscopy: the science and status of the Maunakea Spectroscopic Explorer (MSE) URL;TYPE=URI:/info/1024/4569.htm END:VEVENT BEGIN:VEVENT UID:4304@kiaa.pku.edu.cn DTSTAMP:20180507T080305Z CREATED:20180507T080305Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180508T133000 DTEND;TZID=Asia/Shanghai:20180508T140000 LAST-MODIFIED:20180507T080305Z LOCATION:KIAA second floor common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4304.htm END:VEVENT BEGIN:VEVENT UID:5120@kiaa.pku.edu.cn DTSTAMP:20180405T172854Z CREATED:20180405T172854Z DESCRIPTION:What drives the growth of black holes DTSTART;TZID=Asia/Shanghai:20180510T120000 DTEND;TZID=Asia/Shanghai:20180510T130000 LAST-MODIFIED:20180405T172854Z LOCATION:KIAA 1st meeting room SUMMARY:What drives the growth of black holes URL;TYPE=URI:/info/1025/5120.htm END:VEVENT BEGIN:VEVENT UID:4305@kiaa.pku.edu.cn DTSTAMP:20180508T080856Z CREATED:20180508T080856Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180510T133000 DTEND;TZID=Asia/Shanghai:20180510T140000 LAST-MODIFIED:20180508T080856Z LOCATION:KIAA second floor common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4305.htm END:VEVENT BEGIN:VEVENT UID:6697@kiaa.pku.edu.cn DTSTAMP:20180423T094243Z CREATED:20180423T094243Z DESCRIPTION:Gravitational-wave Seminar: GW170817/GRB 170817A/AT2017gfo/afterglow: what did the first NS-NS merger event tell us? DTSTART;TZID=Asia/Shanghai:20180510T150000 DTEND;TZID=Asia/Shanghai:20180510T170000 LAST-MODIFIED:20180423T094243Z LOCATION:KIAA auditorium room SUMMARY:Gravitational-wave Seminar: GW170817/GRB 170817A/AT2017gfo/afterglow: what did the first NS-NS merger event tell us? URL;TYPE=URI:/info/1089/6697.htm END:VEVENT BEGIN:VEVENT UID:4306@kiaa.pku.edu.cn DTSTAMP:20180514T092642Z CREATED:20180514T092642Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180515T133000 DTEND;TZID=Asia/Shanghai:20180515T140000 LAST-MODIFIED:20180514T092642Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4306.htm END:VEVENT BEGIN:VEVENT UID:4637@kiaa.pku.edu.cn DTSTAMP:20171207T125011Z CREATED:20171207T125011Z DESCRIPTION:Imaging snow lines in protoplanetary disks DTSTART;TZID=Asia/Shanghai:20180517T160000 DTEND;TZID=Asia/Shanghai:20180517T170000 LAST-MODIFIED:20171207T125011Z LOCATION:KIAA-PKU Auditorium SUMMARY:Imaging snow lines in protoplanetary disks URL;TYPE=URI:/info/1024/4637.htm END:VEVENT BEGIN:VEVENT UID:4765@kiaa.pku.edu.cn DTSTAMP:20171107T134326Z CREATED:20171107T134326Z DESCRIPTION:What is the Ultra-Diffuse Galaxy? DTSTART;TZID=Asia/Shanghai:20180522T120000 DTEND;TZID=Asia/Shanghai:20180522T130000 LAST-MODIFIED:20171107T134326Z LOCATION:KIAA-PKU SUMMARY:What is the Ultra-Diffuse Galaxy? URL;TYPE=URI:/info/1028/4765.htm END:VEVENT BEGIN:VEVENT UID:4307@kiaa.pku.edu.cn DTSTAMP:20180521T182053Z CREATED:20180521T182053Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180522T133000 DTEND;TZID=Asia/Shanghai:20180522T140000 LAST-MODIFIED:20180521T182053Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4307.htm END:VEVENT BEGIN:VEVENT UID:4567@kiaa.pku.edu.cn DTSTAMP:20180426T161046Z CREATED:20180426T161046Z DESCRIPTION:The Star Formation Law in Dense Molecular Gas DTSTART;TZID=Asia/Shanghai:20180524T160000 DTEND;TZID=Asia/Shanghai:20180524T170000 LAST-MODIFIED:20180426T161046Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Star Formation Law in Dense Molecular Gas URL;TYPE=URI:/info/1024/4567.htm END:VEVENT BEGIN:VEVENT UID:4308@kiaa.pku.edu.cn DTSTAMP:20180527T150924Z CREATED:20180527T150924Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180529T133000 DTEND;TZID=Asia/Shanghai:20180529T140000 LAST-MODIFIED:20180527T150924Z LOCATION:KIAA second floor common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4308.htm END:VEVENT BEGIN:VEVENT UID:4309@kiaa.pku.edu.cn DTSTAMP:20180531T080346Z CREATED:20180531T080346Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180531T133000 DTEND;TZID=Asia/Shanghai:20180531T140000 LAST-MODIFIED:20180531T080346Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4309.htm END:VEVENT BEGIN:VEVENT UID:4568@kiaa.pku.edu.cn DTSTAMP:20180426T161147Z CREATED:20180426T161147Z DESCRIPTION:Top quark and Higgs physics in hadron collisions DTSTART;TZID=Asia/Shanghai:20180531T160000 DTEND;TZID=Asia/Shanghai:20180531T170000 LAST-MODIFIED:20180426T161147Z LOCATION:KIAA-PKU Auditorium SUMMARY:Top quark and Higgs physics in hadron collisions URL;TYPE=URI:/info/1024/4568.htm END:VEVENT BEGIN:VEVENT UID:5117@kiaa.pku.edu.cn DTSTAMP:20180524T152550Z CREATED:20180524T152550Z DESCRIPTION:Fast Radio Bursts - The Next Five Years DTSTART;TZID=Asia/Shanghai:20180601T120000 DTEND;TZID=Asia/Shanghai:20180601T130000 LAST-MODIFIED:20180524T152550Z LOCATION:meeting room of first floor, KIAA SUMMARY:Fast Radio Bursts - The Next Five Years URL;TYPE=URI:/info/1025/5117.htm END:VEVENT BEGIN:VEVENT UID:5114@kiaa.pku.edu.cn DTSTAMP:20180603T103736Z CREATED:20180603T103736Z DESCRIPTION:High-energy gamma rays and neutrinos (> GeV) from the Sun DTSTART;TZID=Asia/Shanghai:20180604T120000 DTEND;TZID=Asia/Shanghai:20180604T130000 LAST-MODIFIED:20180603T103736Z LOCATION:DoA, Rm 2907 SUMMARY:High-energy gamma rays and neutrinos (> GeV) from the Sun URL;TYPE=URI:/info/1025/5114.htm END:VEVENT BEGIN:VEVENT UID:4764@kiaa.pku.edu.cn DTSTAMP:20171107T134450Z CREATED:20171107T134450Z DESCRIPTION:Binary Black Hole Mergers from Globular Clusters DTSTART;TZID=Asia/Shanghai:20180605T120000 DTEND;TZID=Asia/Shanghai:20180605T130000 LAST-MODIFIED:20171107T134450Z LOCATION:KIAA-PKU SUMMARY:Binary Black Hole Mergers from Globular Clusters URL;TYPE=URI:/info/1028/4764.htm END:VEVENT BEGIN:VEVENT UID:4564@kiaa.pku.edu.cn DTSTAMP:20180409T132545Z CREATED:20180409T132545Z DESCRIPTION:X-ray Emission of High-redshift Jetted Active Galactic Nuclei DTSTART;TZID=Asia/Shanghai:20180607T160000 DTEND;TZID=Asia/Shanghai:20180607T170000 LAST-MODIFIED:20180409T132545Z LOCATION:KIAA-PKU Auditorium SUMMARY:X-ray Emission of High-redshift Jetted Active Galactic Nuclei URL;TYPE=URI:/info/1024/4564.htm END:VEVENT BEGIN:VEVENT UID:4310@kiaa.pku.edu.cn DTSTAMP:20180611T092459Z CREATED:20180611T092459Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20180612T133000 DTEND;TZID=Asia/Shanghai:20180612T140000 LAST-MODIFIED:20180611T092459Z LOCATION: SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4310.htm END:VEVENT BEGIN:VEVENT UID:5113@kiaa.pku.edu.cn DTSTAMP:20180611T130056Z CREATED:20180611T130056Z DESCRIPTION:A link between major or intermediate mergers and the formation of galactic discs and of their structures DTSTART;TZID=Asia/Shanghai:20180613T120000 DTEND;TZID=Asia/Shanghai:20180613T130000 LAST-MODIFIED:20180611T130056Z LOCATION:first floor meeting room, KIAA SUMMARY:A link between major or intermediate mergers and the formation of galactic discs and of their structures URL;TYPE=URI:/info/1025/5113.htm END:VEVENT BEGIN:VEVENT UID:4570@kiaa.pku.edu.cn DTSTAMP:20180507T114810Z CREATED:20180507T114810Z DESCRIPTION:Constraining Planet Mass-Scale Objects in Extragalactic Galaxies and Immediate Environment around Supermassive Black Holes with Quasar Microlensing DTSTART;TZID=Asia/Shanghai:20180614T160000 DTEND;TZID=Asia/Shanghai:20180614T170000 LAST-MODIFIED:20180507T114810Z LOCATION:KIAA-PKU Auditorium SUMMARY:Constraining Planet Mass-Scale Objects in Extragalactic Galaxies and Immediate Environment around Supermassive Black Holes with Quasar Microlensing URL;TYPE=URI:/info/1024/4570.htm END:VEVENT BEGIN:VEVENT UID:5115@kiaa.pku.edu.cn DTSTAMP:20180528T102845Z CREATED:20180528T102845Z DESCRIPTION:Supernova Feedback: from Multiphase Interstellar Medium to Galactic Outflows DTSTART;TZID=Asia/Shanghai:20180615T120000 DTEND;TZID=Asia/Shanghai:20180615T130000 LAST-MODIFIED:20180528T102845Z LOCATION:1st floor meeting room, KIAA SUMMARY:Supernova Feedback: from Multiphase Interstellar Medium to Galactic Outflows URL;TYPE=URI:/info/1025/5115.htm END:VEVENT BEGIN:VEVENT UID:6692@kiaa.pku.edu.cn DTSTAMP:20180109T161510Z CREATED:20180109T161510Z DESCRIPTION:Dragon Boat Festival Holiday DTSTART;TZID=Asia/Shanghai:20180616T000000 DTEND;TZID=Asia/Shanghai:20180618T000000 LAST-MODIFIED:20180109T161510Z LOCATION: SUMMARY:Dragon Boat Festival Holiday URL;TYPE=URI:/info/1089/6692.htm END:VEVENT BEGIN:VEVENT UID:5205@kiaa.pku.edu.cn DTSTAMP:20171123T143744Z CREATED:20171123T143744Z DESCRIPTION:KIAA Forum on Gas in Galaxies DTSTART;TZID=Asia/Shanghai:20180618T090000 DTEND;TZID=Asia/Shanghai:20180622T180000 LAST-MODIFIED:20171123T143744Z LOCATION:KIAA Auditorium SUMMARY:KIAA Forum on Gas in Galaxies URL;TYPE=URI:/info/1026/5205.htm END:VEVENT BEGIN:VEVENT UID:5119@kiaa.pku.edu.cn DTSTAMP:20180426T094949Z CREATED:20180426T094949Z DESCRIPTION:Chemical evolution of Milky Way and external galaxies revealed by APOGEE and MaNGA DTSTART;TZID=Asia/Shanghai:20180625T120000 DTEND;TZID=Asia/Shanghai:20180625T130000 LAST-MODIFIED:20180426T094949Z LOCATION:DoA, Rm 2907 SUMMARY:Chemical evolution of Milky Way and external galaxies revealed by APOGEE and MaNGA URL;TYPE=URI:/info/1025/5119.htm END:VEVENT BEGIN:VEVENT UID:4565@kiaa.pku.edu.cn DTSTAMP:20180411T102311Z CREATED:20180411T102311Z DESCRIPTION:The SkyMapper Southern Survey DTSTART;TZID=Asia/Shanghai:20180628T160000 DTEND;TZID=Asia/Shanghai:20180628T170000 LAST-MODIFIED:20180411T102311Z LOCATION:KIAA-PKU Auditorium SUMMARY:The SkyMapper Southern Survey URL;TYPE=URI:/info/1024/4565.htm END:VEVENT BEGIN:VEVENT UID:5112@kiaa.pku.edu.cn DTSTAMP:20180614T202026Z CREATED:20180614T202026Z DESCRIPTION:Massive runaways as probes for stellar physics and dynamics DTSTART;TZID=Asia/Shanghai:20180703T120000 DTEND;TZID=Asia/Shanghai:20180703T130000 LAST-MODIFIED:20180614T202026Z LOCATION:KIAA, 1st meeting room SUMMARY:Massive runaways as probes for stellar physics and dynamics URL;TYPE=URI:/info/1025/5112.htm END:VEVENT BEGIN:VEVENT UID:5107@kiaa.pku.edu.cn DTSTAMP:20180627T202439Z CREATED:20180627T202439Z DESCRIPTION:Electron scattering wings on lines in interacting supernovae DTSTART;TZID=Asia/Shanghai:20180704T120000 DTEND;TZID=Asia/Shanghai:20180704T130000 LAST-MODIFIED:20180627T202439Z LOCATION:KIAA, 1st meeting room SUMMARY:Electron scattering wings on lines in interacting supernovae URL;TYPE=URI:/info/1025/5107.htm END:VEVENT BEGIN:VEVENT UID:4572@kiaa.pku.edu.cn DTSTAMP:20180605T144752Z CREATED:20180605T144752Z DESCRIPTION:ARIMA, TCF and RF: A new statistical approach to exoplanet transit detection DTSTART;TZID=Asia/Shanghai:20180705T160000 DTEND;TZID=Asia/Shanghai:20180705T170000 LAST-MODIFIED:20180605T144752Z LOCATION:KIAA-PKU Auditorium SUMMARY:ARIMA, TCF and RF: A new statistical approach to exoplanet transit detection URL;TYPE=URI:/info/1024/4572.htm END:VEVENT BEGIN:VEVENT UID:5106@kiaa.pku.edu.cn DTSTAMP:20180702T122819Z CREATED:20180702T122819Z DESCRIPTION:Binary Neutron Star Mergers: Learning from the Afterglow of the > August 17th 2017 Event DTSTART;TZID=Asia/Shanghai:20180706T120000 DTEND;TZID=Asia/Shanghai:20180706T130000 LAST-MODIFIED:20180702T122819Z LOCATION:KIAA, 1st meeting room SUMMARY:Binary Neutron Star Mergers: Learning from the Afterglow of the > August 17th 2017 Event URL;TYPE=URI:/info/1025/5106.htm END:VEVENT BEGIN:VEVENT UID:6698@kiaa.pku.edu.cn DTSTAMP:20180706T094950Z CREATED:20180706T094950Z DESCRIPTION:Interview for 2018 Excellent Undergradusates Summer Camp DTSTART;TZID=Asia/Shanghai:20180707T080000 DTEND;TZID=Asia/Shanghai:20180708T153000 LAST-MODIFIED:20180706T094950Z LOCATION:1st meeting room, KIAA SUMMARY:Interview for 2018 Excellent Undergradusates Summer Camp URL;TYPE=URI:/info/1089/6698.htm END:VEVENT BEGIN:VEVENT UID:5111@kiaa.pku.edu.cn DTSTAMP:20180620T104417Z CREATED:20180620T104417Z DESCRIPTION:What can we learn about cosmic-ray sources from the isotropic gamma-ray background? DTSTART;TZID=Asia/Shanghai:20180709T120000 DTEND;TZID=Asia/Shanghai:20180709T130000 LAST-MODIFIED:20180620T104417Z LOCATION:DoA, Rm 2907 SUMMARY:What can we learn about cosmic-ray sources from the isotropic gamma-ray background? URL;TYPE=URI:/info/1025/5111.htm END:VEVENT BEGIN:VEVENT UID:5118@kiaa.pku.edu.cn DTSTAMP:20180509T111631Z CREATED:20180509T111631Z DESCRIPTION:Accreting supermassive black holes in the X-ray band DTSTART;TZID=Asia/Shanghai:20180710T120000 DTEND;TZID=Asia/Shanghai:20180710T130000 LAST-MODIFIED:20180509T111631Z LOCATION:1st floor meeting room, KIAA SUMMARY:Accreting supermassive black holes in the X-ray band URL;TYPE=URI:/info/1025/5118.htm END:VEVENT BEGIN:VEVENT UID:5110@kiaa.pku.edu.cn DTSTAMP:20180622T164431Z CREATED:20180622T164431Z DESCRIPTION:Highlights of DAMPE experiment DTSTART;TZID=Asia/Shanghai:20180711T120000 DTEND;TZID=Asia/Shanghai:20180711T130000 LAST-MODIFIED:20180622T164431Z LOCATION:first floor meeting room, KIAA SUMMARY:Highlights of DAMPE experiment URL;TYPE=URI:/info/1025/5110.htm END:VEVENT BEGIN:VEVENT UID:5105@kiaa.pku.edu.cn DTSTAMP:20180702T202944Z CREATED:20180702T202944Z DESCRIPTION:Highly magnified stars in lensing clusters and a probe for dark matter substructure DTSTART;TZID=Asia/Shanghai:20180713T120000 DTEND;TZID=Asia/Shanghai:20180713T130000 LAST-MODIFIED:20180702T202944Z LOCATION:first floor meeting room, KIAA SUMMARY:Highly magnified stars in lensing clusters and a probe for dark matter substructure URL;TYPE=URI:/info/1025/5105.htm END:VEVENT BEGIN:VEVENT UID:6686@kiaa.pku.edu.cn DTSTAMP:20170929T100651Z CREATED:20170929T100651Z DESCRIPTION:Summer Holiday DTSTART;TZID=Asia/Shanghai:20180716T000000 DTEND;TZID=Asia/Shanghai:20180826T000000 LAST-MODIFIED:20170929T100651Z LOCATION: SUMMARY:Summer Holiday URL;TYPE=URI:/info/1089/6686.htm END:VEVENT BEGIN:VEVENT UID:5116@kiaa.pku.edu.cn DTSTAMP:20180524T153928Z CREATED:20180524T153928Z DESCRIPTION:Monitoring Active Galactic Nuclei with Hbeta Asymmetry with the Wyoming Infrared Observatory DTSTART;TZID=Asia/Shanghai:20180716T120000 DTEND;TZID=Asia/Shanghai:20180716T130000 LAST-MODIFIED:20180524T153928Z LOCATION:DoA, Rm 2907 SUMMARY:Monitoring Active Galactic Nuclei with Hbeta Asymmetry with the Wyoming Infrared Observatory URL;TYPE=URI:/info/1025/5116.htm END:VEVENT BEGIN:VEVENT UID:5104@kiaa.pku.edu.cn DTSTAMP:20180702T210610Z CREATED:20180702T210610Z DESCRIPTION:Demystifying the Diverse IR Continuum SED Shapes among Type-1 AGNs DTSTART;TZID=Asia/Shanghai:20180717T120000 DTEND;TZID=Asia/Shanghai:20180717T130000 LAST-MODIFIED:20180702T210610Z LOCATION:first floor meeting room, KIAA SUMMARY:Demystifying the Diverse IR Continuum SED Shapes among Type-1 AGNs URL;TYPE=URI:/info/1025/5104.htm END:VEVENT BEGIN:VEVENT UID:5109@kiaa.pku.edu.cn DTSTAMP:20180627T091802Z CREATED:20180627T091802Z DESCRIPTION:Alkali metals in exoplanet atmospheres DTSTART;TZID=Asia/Shanghai:20180718T120000 DTEND;TZID=Asia/Shanghai:20180718T130000 LAST-MODIFIED:20180627T091802Z LOCATION:first floor meeting room, KIAA SUMMARY:Alkali metals in exoplanet atmospheres URL;TYPE=URI:/info/1025/5109.htm END:VEVENT BEGIN:VEVENT UID:5103@kiaa.pku.edu.cn DTSTAMP:20180719T182329Z CREATED:20180719T182329Z DESCRIPTION:Toward understanding reionization and Lyman-alpha emitter from green pea galaxies DTSTART;TZID=Asia/Shanghai:20180724T120000 DTEND;TZID=Asia/Shanghai:20180724T130000 LAST-MODIFIED:20180719T182329Z LOCATION:1st floor meeting room, KIAA SUMMARY:Toward understanding reionization and Lyman-alpha emitter from green pea galaxies URL;TYPE=URI:/info/1025/5103.htm END:VEVENT BEGIN:VEVENT UID:5108@kiaa.pku.edu.cn DTSTAMP:20180627T143747Z CREATED:20180627T143747Z DESCRIPTION:Characterisation of gravity and Rossby modes in hundreds of Kepler γ Doradus stars DTSTART;TZID=Asia/Shanghai:20180807T120000 DTEND;TZID=Asia/Shanghai:20180807T130000 LAST-MODIFIED:20180627T143747Z LOCATION:first floor meeting room, KIAA SUMMARY:Characterisation of gravity and Rossby modes in hundreds of Kepler γ Doradus stars URL;TYPE=URI:/info/1025/5108.htm END:VEVENT BEGIN:VEVENT UID:4566@kiaa.pku.edu.cn DTSTAMP:20180416T135737Z CREATED:20180416T135737Z DESCRIPTION:We don’t know how supernovae explode DTSTART;TZID=Asia/Shanghai:20180809T160000 DTEND;TZID=Asia/Shanghai:20180809T170000 LAST-MODIFIED:20180416T135737Z LOCATION:KIAA-PKU Auditorium SUMMARY:We don’t know how supernovae explode URL;TYPE=URI:/info/1024/4566.htm END:VEVENT BEGIN:VEVENT UID:5101@kiaa.pku.edu.cn DTSTAMP:20180823T092840Z CREATED:20180823T092840Z DESCRIPTION:Detecting Rocky Exoplanets with Precise Radial Velocities DTSTART;TZID=Asia/Shanghai:20180905T120000 DTEND;TZID=Asia/Shanghai:20180905T130000 LAST-MODIFIED:20180823T092840Z LOCATION:KIAA, 1st meeting room SUMMARY:Detecting Rocky Exoplanets with Precise Radial Velocities URL;TYPE=URI:/info/1025/5101.htm END:VEVENT BEGIN:VEVENT UID:4763@kiaa.pku.edu.cn DTSTAMP:20180907T125020Z CREATED:20180907T125020Z DESCRIPTION:Galaxy angular momentum - summary of the IAU FM13 meeting DTSTART;TZID=Asia/Shanghai:20180911T120000 DTEND;TZID=Asia/Shanghai:20180911T130000 LAST-MODIFIED:20180907T125020Z LOCATION:KIAA-PKU SUMMARY:Galaxy angular momentum - summary of the IAU FM13 meeting URL;TYPE=URI:/info/1028/4763.htm END:VEVENT BEGIN:VEVENT UID:4575@kiaa.pku.edu.cn DTSTAMP:20180819T000429Z CREATED:20180819T000429Z DESCRIPTION:The Radiation Mechanism of Fast Radio Bursts DTSTART;TZID=Asia/Shanghai:20180913T160000 DTEND;TZID=Asia/Shanghai:20180913T170000 LAST-MODIFIED:20180819T000429Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Radiation Mechanism of Fast Radio Bursts URL;TYPE=URI:/info/1024/4575.htm END:VEVENT BEGIN:VEVENT UID:4580@kiaa.pku.edu.cn DTSTAMP:20180911T160204Z CREATED:20180911T160204Z DESCRIPTION:From relativistic heavy ion collision to antimatter production DTSTART;TZID=Asia/Shanghai:20180914T160000 DTEND;TZID=Asia/Shanghai:20180914T170000 LAST-MODIFIED:20180911T160204Z LOCATION:KIAA-PKU Auditorium SUMMARY:From relativistic heavy ion collision to antimatter production URL;TYPE=URI:/info/1024/4580.htm END:VEVENT BEGIN:VEVENT UID:5194@kiaa.pku.edu.cn DTSTAMP:20180706T085412Z CREATED:20180706T085412Z DESCRIPTION:KIAA Governing Board Meeting DTSTART;TZID=Asia/Shanghai:20180917T084500 DTEND;TZID=Asia/Shanghai:20180917T153000 LAST-MODIFIED:20180706T085412Z LOCATION:KIAA 1st meeting room SUMMARY:KIAA Governing Board Meeting URL;TYPE=URI:/info/1026/5194.htm END:VEVENT BEGIN:VEVENT UID:4579@kiaa.pku.edu.cn DTSTAMP:20180903T140529Z CREATED:20180903T140529Z DESCRIPTION:Cosmology with dwarf galaxies DTSTART;TZID=Asia/Shanghai:20180917T160000 DTEND;TZID=Asia/Shanghai:20180917T170000 LAST-MODIFIED:20180903T140529Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmology with dwarf galaxies URL;TYPE=URI:/info/1024/4579.htm END:VEVENT BEGIN:VEVENT UID:4581@kiaa.pku.edu.cn DTSTAMP:20180912T150030Z CREATED:20180912T150030Z DESCRIPTION:The Impact of Masers in Modern Astrophysics DTSTART;TZID=Asia/Shanghai:20180918T100000 DTEND;TZID=Asia/Shanghai:20180918T110000 LAST-MODIFIED:20180912T150030Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Impact of Masers in Modern Astrophysics URL;TYPE=URI:/info/1024/4581.htm END:VEVENT BEGIN:VEVENT UID:4574@kiaa.pku.edu.cn DTSTAMP:20180806T104314Z CREATED:20180806T104314Z DESCRIPTION:The Evolution and Quenching of Galaxies after z ~ 3 DTSTART;TZID=Asia/Shanghai:20180919T160000 DTEND;TZID=Asia/Shanghai:20180919T170000 LAST-MODIFIED:20180806T104314Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Evolution and Quenching of Galaxies after z ~ 3 URL;TYPE=URI:/info/1024/4574.htm END:VEVENT BEGIN:VEVENT UID:4578@kiaa.pku.edu.cn DTSTAMP:20180830T134325Z CREATED:20180830T134325Z DESCRIPTION:Recent progress of hyper nuclear DTSTART;TZID=Asia/Shanghai:20180920T160000 DTEND;TZID=Asia/Shanghai:20180920T170000 LAST-MODIFIED:20180830T134325Z LOCATION:KIAA-PKU Auditorium SUMMARY:Recent progress of hyper nuclear URL;TYPE=URI:/info/1024/4578.htm END:VEVENT BEGIN:VEVENT UID:6701@kiaa.pku.edu.cn DTSTAMP:20180921T104032Z CREATED:20180921T104032Z DESCRIPTION:2018 PKU-Undergraduate Astronomy Symposium DTSTART;TZID=Asia/Shanghai:20180921T140000 DTEND;TZID=Asia/Shanghai:20180921T170000 LAST-MODIFIED:20180921T104032Z LOCATION:Auditorium KIAA SUMMARY:2018 PKU-Undergraduate Astronomy Symposium URL;TYPE=URI:/info/1089/6701.htm END:VEVENT BEGIN:VEVENT UID:6702@kiaa.pku.edu.cn DTSTAMP:20180921T104135Z CREATED:20180921T104135Z DESCRIPTION:Mid-autumn Gala & Welcome Party for freshman DTSTART;TZID=Asia/Shanghai:20180921T190000 DTEND;TZID=Asia/Shanghai:20180921T190000 LAST-MODIFIED:20180921T104135Z LOCATION:Auditorium SUMMARY:Mid-autumn Gala & Welcome Party for freshman URL;TYPE=URI:/info/1089/6702.htm END:VEVENT BEGIN:VEVENT UID:6693@kiaa.pku.edu.cn DTSTAMP:20180109T161605Z CREATED:20180109T161605Z DESCRIPTION:Mid-autumn Festival Holiday DTSTART;TZID=Asia/Shanghai:20180922T000000 DTEND;TZID=Asia/Shanghai:20180924T000000 LAST-MODIFIED:20180109T161605Z LOCATION: SUMMARY:Mid-autumn Festival Holiday URL;TYPE=URI:/info/1089/6693.htm END:VEVENT BEGIN:VEVENT UID:6703@kiaa.pku.edu.cn DTSTAMP:20180925T101544Z CREATED:20180925T101544Z DESCRIPTION:Interview with the candidate Ph.D. students DTSTART;TZID=Asia/Shanghai:20180926T083000 DTEND;TZID=Asia/Shanghai:20180926T120000 LAST-MODIFIED:20180925T101544Z LOCATION:2nd meeting room, KIAA SUMMARY:Interview with the candidate Ph.D. students URL;TYPE=URI:/info/1089/6703.htm END:VEVENT BEGIN:VEVENT UID:6694@kiaa.pku.edu.cn DTSTAMP:20180109T161659Z CREATED:20180109T161659Z DESCRIPTION:National Day Holiday DTSTART;TZID=Asia/Shanghai:20181001T000000 DTEND;TZID=Asia/Shanghai:20181007T000000 LAST-MODIFIED:20180109T161659Z LOCATION: SUMMARY:National Day Holiday URL;TYPE=URI:/info/1089/6694.htm END:VEVENT BEGIN:VEVENT UID:3907@kiaa.pku.edu.cn DTSTAMP:20180917T115939Z CREATED:20180917T115939Z DESCRIPTION:The Long-Term Stability of Planetary Systems DTSTART;TZID=Asia/Shanghai:20181008T160000 DTEND;TZID=Asia/Shanghai:20181008T173000 LAST-MODIFIED:20180917T115939Z LOCATION:Sunshine Hall(阳光厅)， Yingjie Exchange Center (英杰交流中心). SUMMARY:The Long-Term Stability of Planetary Systems URL;TYPE=URI:/info/1030/3907.htm END:VEVENT BEGIN:VEVENT UID:4311@kiaa.pku.edu.cn DTSTAMP:20180920T094751Z CREATED:20180920T094751Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181009T133000 DTEND;TZID=Asia/Shanghai:20181009T140000 LAST-MODIFIED:20180920T094751Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4311.htm END:VEVENT BEGIN:VEVENT UID:4573@kiaa.pku.edu.cn DTSTAMP:20180723T102642Z CREATED:20180723T102642Z DESCRIPTION:Comets, unseen planets, and the outer fringes of the solar system DTSTART;TZID=Asia/Shanghai:20181009T160000 DTEND;TZID=Asia/Shanghai:20181009T170000 LAST-MODIFIED:20180723T102642Z LOCATION:KIAA-PKU Auditorium SUMMARY:Comets, unseen planets, and the outer fringes of the solar system URL;TYPE=URI:/info/1024/4573.htm END:VEVENT BEGIN:VEVENT UID:4312@kiaa.pku.edu.cn DTSTAMP:20181009T091352Z CREATED:20181009T091352Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181011T133000 DTEND;TZID=Asia/Shanghai:20181011T140000 LAST-MODIFIED:20181009T091352Z LOCATION:KIAA second floor, common area, SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4312.htm END:VEVENT BEGIN:VEVENT UID:4576@kiaa.pku.edu.cn DTSTAMP:20180829T170403Z CREATED:20180829T170403Z DESCRIPTION:Massive black holes along the cosmic history: formation, dynamics and gravitational waves DTSTART;TZID=Asia/Shanghai:20181011T160000 DTEND;TZID=Asia/Shanghai:20181011T170000 LAST-MODIFIED:20180829T170403Z LOCATION:KIAA-PKU Auditorium SUMMARY:Massive black holes along the cosmic history: formation, dynamics and gravitational waves URL;TYPE=URI:/info/1024/4576.htm END:VEVENT BEGIN:VEVENT UID:5102@kiaa.pku.edu.cn DTSTAMP:20180810T111645Z CREATED:20180810T111645Z DESCRIPTION:Searching for radio counterparts in the transient sky DTSTART;TZID=Asia/Shanghai:20181016T120000 DTEND;TZID=Asia/Shanghai:20181016T130000 LAST-MODIFIED:20180810T111645Z LOCATION:KIAA, 1st meeting room SUMMARY:Searching for radio counterparts in the transient sky URL;TYPE=URI:/info/1025/5102.htm END:VEVENT BEGIN:VEVENT UID:4313@kiaa.pku.edu.cn DTSTAMP:20181009T125216Z CREATED:20181009T125216Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181016T133000 DTEND;TZID=Asia/Shanghai:20181016T140000 LAST-MODIFIED:20181009T125216Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4313.htm END:VEVENT BEGIN:VEVENT UID:6704@kiaa.pku.edu.cn DTSTAMP:20181014T115410Z CREATED:20181014T115410Z DESCRIPTION:Mini-workshop on high-redshift universe DTSTART;TZID=Asia/Shanghai:20181016T140000 DTEND;TZID=Asia/Shanghai:20181016T160000 LAST-MODIFIED:20181014T115410Z LOCATION:Second meeting room SUMMARY:Mini-workshop on high-redshift universe URL;TYPE=URI:/info/1089/6704.htm END:VEVENT BEGIN:VEVENT UID:4314@kiaa.pku.edu.cn DTSTAMP:20181015T131741Z CREATED:20181015T131741Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181018T133000 DTEND;TZID=Asia/Shanghai:20181018T140000 LAST-MODIFIED:20181015T131741Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4314.htm END:VEVENT BEGIN:VEVENT UID:4577@kiaa.pku.edu.cn DTSTAMP:20180829T170519Z CREATED:20180829T170519Z DESCRIPTION:Reionization after Planck and before JWST DTSTART;TZID=Asia/Shanghai:20181018T160000 DTEND;TZID=Asia/Shanghai:20181018T170000 LAST-MODIFIED:20180829T170519Z LOCATION:KIAA-PKU Auditorium SUMMARY:Reionization after Planck and before JWST URL;TYPE=URI:/info/1024/4577.htm END:VEVENT BEGIN:VEVENT UID:5094@kiaa.pku.edu.cn DTSTAMP:20181016T111522Z CREATED:20181016T111522Z DESCRIPTION:Massive star formation in the early Universe DTSTART;TZID=Asia/Shanghai:20181023T120000 DTEND;TZID=Asia/Shanghai:20181023T130000 LAST-MODIFIED:20181016T111522Z LOCATION:first floor meeting room, KIAA SUMMARY:Massive star formation in the early Universe URL;TYPE=URI:/info/1025/5094.htm END:VEVENT BEGIN:VEVENT UID:4315@kiaa.pku.edu.cn DTSTAMP:20181022T103025Z CREATED:20181022T103025Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181023T133000 DTEND;TZID=Asia/Shanghai:20181023T140000 LAST-MODIFIED:20181022T103025Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4315.htm END:VEVENT BEGIN:VEVENT UID:4754@kiaa.pku.edu.cn DTSTAMP:20181023T083812Z CREATED:20181023T083812Z DESCRIPTION:The Relative and Absolute LGRB Rate with Metallically and Its Lack of Evolution DTSTART;TZID=Asia/Shanghai:20181025T120000 DTEND;TZID=Asia/Shanghai:20181025T130000 LAST-MODIFIED:20181023T083812Z LOCATION:2nd meeting room, KIAA-PKU SUMMARY:The Relative and Absolute LGRB Rate with Metallically and Its Lack of Evolution URL;TYPE=URI:/info/1028/4754.htm END:VEVENT BEGIN:VEVENT UID:4316@kiaa.pku.edu.cn DTSTAMP:20181022T103131Z CREATED:20181022T103131Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181025T133000 DTEND;TZID=Asia/Shanghai:20181025T140000 LAST-MODIFIED:20181022T103131Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4316.htm END:VEVENT BEGIN:VEVENT UID:4826@kiaa.pku.edu.cn DTSTAMP:20190916T094049Z CREATED:20190916T094049Z DESCRIPTION:Dependence of Spiral Arms Pitch Angle on Wavelength as a Test of Density Wave Theory DTSTART;TZID=Asia/Shanghai:20181025T170000 DTEND;TZID=Asia/Shanghai:20181025T170000 LAST-MODIFIED:20190916T094049Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Dependence of Spiral Arms Pitch Angle on Wavelength as a Test of Density Wave Theory URL;TYPE=URI:/info/1029/4826.htm END:VEVENT BEGIN:VEVENT UID:5197@kiaa.pku.edu.cn DTSTAMP:20181026T081939Z CREATED:20181026T081939Z DESCRIPTION:Family Photo & Faculty Meeting DTSTART;TZID=Asia/Shanghai:20181026T114500 DTEND;TZID=Asia/Shanghai:20181026T114500 LAST-MODIFIED:20181026T081939Z LOCATION:1st meeting room, KIAA SUMMARY:Family Photo & Faculty Meeting URL;TYPE=URI:/info/1026/5197.htm END:VEVENT BEGIN:VEVENT UID:4585@kiaa.pku.edu.cn DTSTAMP:20181014T022607Z CREATED:20181014T022607Z DESCRIPTION:Cosmological implications of the BOSS and eBOSS galaxy surveys DTSTART;TZID=Asia/Shanghai:20181026T160000 DTEND;TZID=Asia/Shanghai:20181026T170000 LAST-MODIFIED:20181014T022607Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmological implications of the BOSS and eBOSS galaxy surveys URL;TYPE=URI:/info/1024/4585.htm END:VEVENT BEGIN:VEVENT UID:5099@kiaa.pku.edu.cn DTSTAMP:20180918T114306Z CREATED:20180918T114306Z DESCRIPTION:Measurement of high redshifts of submillimeter galaxies with the new NOEMA system DTSTART;TZID=Asia/Shanghai:20181029T120000 DTEND;TZID=Asia/Shanghai:20181029T130000 LAST-MODIFIED:20180918T114306Z LOCATION:DoA, Rm 2907 SUMMARY:Measurement of high redshifts of submillimeter galaxies with the new NOEMA system URL;TYPE=URI:/info/1025/5099.htm END:VEVENT BEGIN:VEVENT UID:5100@kiaa.pku.edu.cn DTSTAMP:20180913T094221Z CREATED:20180913T094221Z DESCRIPTION:A Complete Spectroscopic Census of Massively Accreting Cluster Abell 2029. DTSTART;TZID=Asia/Shanghai:20181030T120000 DTEND;TZID=Asia/Shanghai:20181030T130000 LAST-MODIFIED:20180913T094221Z LOCATION:KIAA, 1st meeting room SUMMARY:A Complete Spectroscopic Census of Massively Accreting Cluster Abell 2029. URL;TYPE=URI:/info/1025/5100.htm END:VEVENT BEGIN:VEVENT UID:5098@kiaa.pku.edu.cn DTSTAMP:20180920T135331Z CREATED:20180920T135331Z DESCRIPTION:Radiation-regulated accretion onto seed black holes DTSTART;TZID=Asia/Shanghai:20181101T120000 DTEND;TZID=Asia/Shanghai:20181101T130000 LAST-MODIFIED:20180920T135331Z LOCATION:KIAA, 1st meeting room SUMMARY:Radiation-regulated accretion onto seed black holes URL;TYPE=URI:/info/1025/5098.htm END:VEVENT BEGIN:VEVENT UID:4317@kiaa.pku.edu.cn DTSTAMP:20181031T092802Z CREATED:20181031T092802Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181101T133000 DTEND;TZID=Asia/Shanghai:20181101T140000 LAST-MODIFIED:20181031T092802Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4317.htm END:VEVENT BEGIN:VEVENT UID:4587@kiaa.pku.edu.cn DTSTAMP:20181019T143142Z CREATED:20181019T143142Z DESCRIPTION:Instabilities due to Dust-Gas Interactions in Protoplanetary Disks DTSTART;TZID=Asia/Shanghai:20181101T160000 DTEND;TZID=Asia/Shanghai:20181101T170000 LAST-MODIFIED:20181019T143142Z LOCATION:KIAA-PKU Auditorium SUMMARY:Instabilities due to Dust-Gas Interactions in Protoplanetary Disks URL;TYPE=URI:/info/1024/4587.htm END:VEVENT BEGIN:VEVENT UID:5096@kiaa.pku.edu.cn DTSTAMP:20181007T154032Z CREATED:20181007T154032Z DESCRIPTION:Tracking the incidence of AGN across the galaxy population DTSTART;TZID=Asia/Shanghai:20181102T120000 DTEND;TZID=Asia/Shanghai:20181102T130000 LAST-MODIFIED:20181007T154032Z LOCATION:KIAA, 1st meeting room SUMMARY:Tracking the incidence of AGN across the galaxy population URL;TYPE=URI:/info/1025/5096.htm END:VEVENT BEGIN:VEVENT UID:4590@kiaa.pku.edu.cn DTSTAMP:20181101T085505Z CREATED:20181101T085505Z DESCRIPTION:Formation of Ultra-diffuse Galaxies in the field and in galaxy groups DTSTART;TZID=Asia/Shanghai:20181102T160000 DTEND;TZID=Asia/Shanghai:20181102T170000 LAST-MODIFIED:20181101T085505Z LOCATION:KIAA-PKU Auditorium SUMMARY:Formation of Ultra-diffuse Galaxies in the field and in galaxy groups URL;TYPE=URI:/info/1024/4590.htm END:VEVENT BEGIN:VEVENT UID:5088@kiaa.pku.edu.cn DTSTAMP:20181102T164832Z CREATED:20181102T164832Z DESCRIPTION:Milky Way's Mass and Anisotropy Profiles with LAMOST/SDSS and Gaia DTSTART;TZID=Asia/Shanghai:20181105T120000 DTEND;TZID=Asia/Shanghai:20181105T130000 LAST-MODIFIED:20181102T164832Z LOCATION:DoA, Rm 2907 SUMMARY:Milky Way's Mass and Anisotropy Profiles with LAMOST/SDSS and Gaia URL;TYPE=URI:/info/1025/5088.htm END:VEVENT BEGIN:VEVENT UID:4745@kiaa.pku.edu.cn DTSTAMP:20181019T190259Z CREATED:20181019T190259Z DESCRIPTION:First observational indication of the gravitomagnetic monopole and naked singularity DTSTART;TZID=Asia/Shanghai:20181106T000000 DTEND;TZID=Asia/Shanghai:20181106T130000 LAST-MODIFIED:20181019T190259Z LOCATION:KIAA-PKU SUMMARY:First observational indication of the gravitomagnetic monopole and naked singularity URL;TYPE=URI:/info/1028/4745.htm END:VEVENT BEGIN:VEVENT UID:5095@kiaa.pku.edu.cn DTSTAMP:20181010T110214Z CREATED:20181010T110214Z DESCRIPTION:X-ray Tidal Disruption Events Discovered from the XMM-Newton Pointed Observations DTSTART;TZID=Asia/Shanghai:20181107T120000 DTEND;TZID=Asia/Shanghai:20181107T130000 LAST-MODIFIED:20181010T110214Z LOCATION:KIAA, 1st meeting room SUMMARY:X-ray Tidal Disruption Events Discovered from the XMM-Newton Pointed Observations URL;TYPE=URI:/info/1025/5095.htm END:VEVENT BEGIN:VEVENT UID:4318@kiaa.pku.edu.cn DTSTAMP:20181106T140845Z CREATED:20181106T140845Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181108T133000 DTEND;TZID=Asia/Shanghai:20181108T140000 LAST-MODIFIED:20181106T140845Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4318.htm END:VEVENT BEGIN:VEVENT UID:5196@kiaa.pku.edu.cn DTSTAMP:20180906T104550Z CREATED:20180906T104550Z DESCRIPTION:PKU-KIAA Innovation NSFC Group Kick-off Meeting DTSTART;TZID=Asia/Shanghai:20181112T090000 DTEND;TZID=Asia/Shanghai:20181112T180000 LAST-MODIFIED:20180906T104550Z LOCATION:Auditorium, KIAA SUMMARY:PKU-KIAA Innovation NSFC Group Kick-off Meeting URL;TYPE=URI:/info/1026/5196.htm END:VEVENT BEGIN:VEVENT UID:4582@kiaa.pku.edu.cn DTSTAMP:20180918T153506Z CREATED:20180918T153506Z DESCRIPTION:ALMA views of star forming galaxies at high redshifts DTSTART;TZID=Asia/Shanghai:20181113T160000 DTEND;TZID=Asia/Shanghai:20181113T170000 LAST-MODIFIED:20180918T153506Z LOCATION:KIAA-PKU Auditorium SUMMARY:ALMA views of star forming galaxies at high redshifts URL;TYPE=URI:/info/1024/4582.htm END:VEVENT BEGIN:VEVENT UID:5093@kiaa.pku.edu.cn DTSTAMP:20181022T082940Z CREATED:20181022T082940Z DESCRIPTION:Serendipitous discovery of a dying AGN and searching for more fading/dying AGN(s) DTSTART;TZID=Asia/Shanghai:20181115T120000 DTEND;TZID=Asia/Shanghai:20181115T130000 LAST-MODIFIED:20181022T082940Z LOCATION:KIAA, 1st meeting room SUMMARY:Serendipitous discovery of a dying AGN and searching for more fading/dying AGN(s) URL;TYPE=URI:/info/1025/5093.htm END:VEVENT BEGIN:VEVENT UID:4319@kiaa.pku.edu.cn DTSTAMP:20181113T140857Z CREATED:20181113T140857Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181115T133000 DTEND;TZID=Asia/Shanghai:20181115T140000 LAST-MODIFIED:20181113T140857Z LOCATION:KIAA second floor common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4319.htm END:VEVENT BEGIN:VEVENT UID:4588@kiaa.pku.edu.cn DTSTAMP:20181023T134523Z CREATED:20181023T134523Z DESCRIPTION:Cosmology with X-ray Galaxy Clusters DTSTART;TZID=Asia/Shanghai:20181115T160000 DTEND;TZID=Asia/Shanghai:20181115T170000 LAST-MODIFIED:20181023T134523Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmology with X-ray Galaxy Clusters URL;TYPE=URI:/info/1024/4588.htm END:VEVENT BEGIN:VEVENT UID:6706@kiaa.pku.edu.cn DTSTAMP:20181107T172510Z CREATED:20181107T172510Z DESCRIPTION:GW Tutorial: 1. The Theoretical Basics DTSTART;TZID=Asia/Shanghai:20181119T093000 DTEND;TZID=Asia/Shanghai:20181119T120000 LAST-MODIFIED:20181107T172510Z LOCATION:KIAA first meeting room SUMMARY:GW Tutorial: 1. The Theoretical Basics URL;TYPE=URI:/info/1089/6706.htm END:VEVENT BEGIN:VEVENT UID:4586@kiaa.pku.edu.cn DTSTAMP:20181016T100957Z CREATED:20181016T100957Z DESCRIPTION:A new era of Galactic Archaeology DTSTART;TZID=Asia/Shanghai:20181119T160000 DTEND;TZID=Asia/Shanghai:20181119T170000 LAST-MODIFIED:20181016T100957Z LOCATION:KIAA-PKU Auditorium SUMMARY:A new era of Galactic Archaeology URL;TYPE=URI:/info/1024/4586.htm END:VEVENT BEGIN:VEVENT UID:5091@kiaa.pku.edu.cn DTSTAMP:20181023T130734Z CREATED:20181023T130734Z DESCRIPTION:Final Defence Lunch Talk DTSTART;TZID=Asia/Shanghai:20181121T120000 DTEND;TZID=Asia/Shanghai:20181121T130000 LAST-MODIFIED:20181023T130734Z LOCATION:KIAA, 1st meeting room SUMMARY:Final Defence Lunch Talk URL;TYPE=URI:/info/1025/5091.htm END:VEVENT BEGIN:VEVENT UID:4592@kiaa.pku.edu.cn DTSTAMP:20181114T175032Z CREATED:20181114T175032Z DESCRIPTION:Understanding the trends in the Bulge of the Milky Way DTSTART;TZID=Asia/Shanghai:20181121T160000 DTEND;TZID=Asia/Shanghai:20181121T170000 LAST-MODIFIED:20181114T175032Z LOCATION:KIAA-PKU Auditorium SUMMARY:Understanding the trends in the Bulge of the Milky Way URL;TYPE=URI:/info/1024/4592.htm END:VEVENT BEGIN:VEVENT UID:4746@kiaa.pku.edu.cn DTSTAMP:20181019T190407Z CREATED:20181019T190407Z DESCRIPTION:Galactic winds in star forming galaxies and AGNs: is there evidence for AGN feedback DTSTART;TZID=Asia/Shanghai:20181122T120000 DTEND;TZID=Asia/Shanghai:20181122T130000 LAST-MODIFIED:20181019T190407Z LOCATION:KIAA-PKU SUMMARY:Galactic winds in star forming galaxies and AGNs: is there evidence for AGN feedback URL;TYPE=URI:/info/1028/4746.htm END:VEVENT BEGIN:VEVENT UID:4320@kiaa.pku.edu.cn DTSTAMP:20181121T212319Z CREATED:20181121T212319Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181122T133000 DTEND;TZID=Asia/Shanghai:20181122T140000 LAST-MODIFIED:20181121T212319Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4320.htm END:VEVENT BEGIN:VEVENT UID:4571@kiaa.pku.edu.cn DTSTAMP:20180605T102959Z CREATED:20180605T102959Z DESCRIPTION:Gravitational-wave Astrophysics: BH-BH/NS-NS mergers with LIGO/Virgo DTSTART;TZID=Asia/Shanghai:20181122T160000 DTEND;TZID=Asia/Shanghai:20181122T170000 LAST-MODIFIED:20180605T102959Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gravitational-wave Astrophysics: BH-BH/NS-NS mergers with LIGO/Virgo URL;TYPE=URI:/info/1024/4571.htm END:VEVENT BEGIN:VEVENT UID:5086@kiaa.pku.edu.cn DTSTAMP:20181107T094452Z CREATED:20181107T094452Z DESCRIPTION:Shedding new light on planet formation from ALMA observations of protoplanetary disks DTSTART;TZID=Asia/Shanghai:20181123T120000 DTEND;TZID=Asia/Shanghai:20181123T130000 LAST-MODIFIED:20181107T094452Z LOCATION:KIAA, 1st meeting room SUMMARY:Shedding new light on planet formation from ALMA observations of protoplanetary disks URL;TYPE=URI:/info/1025/5086.htm END:VEVENT BEGIN:VEVENT UID:4747@kiaa.pku.edu.cn DTSTAMP:20181019T190626Z CREATED:20181019T190626Z DESCRIPTION:The Life and Times of the Milky Way DTSTART;TZID=Asia/Shanghai:20181127T120000 DTEND;TZID=Asia/Shanghai:20181127T130000 LAST-MODIFIED:20181019T190626Z LOCATION:KIAA-PKU SUMMARY:The Life and Times of the Milky Way URL;TYPE=URI:/info/1028/4747.htm END:VEVENT BEGIN:VEVENT UID:4827@kiaa.pku.edu.cn DTSTAMP:20190916T094212Z CREATED:20190916T094212Z DESCRIPTION:The physical origin of the death of massive galaxies in the local Universe DTSTART;TZID=Asia/Shanghai:20181127T170000 DTEND;TZID=Asia/Shanghai:20181127T170000 LAST-MODIFIED:20190916T094212Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The physical origin of the death of massive galaxies in the local Universe URL;TYPE=URI:/info/1029/4827.htm END:VEVENT BEGIN:VEVENT UID:4591@kiaa.pku.edu.cn DTSTAMP:20181114T121252Z CREATED:20181114T121252Z DESCRIPTION:Cosmology with Large-scale Structures in the Universe DTSTART;TZID=Asia/Shanghai:20181130T100000 DTEND;TZID=Asia/Shanghai:20181130T110000 LAST-MODIFIED:20181114T121252Z LOCATION:KIAA-PKU Auditorium SUMMARY:Cosmology with Large-scale Structures in the Universe URL;TYPE=URI:/info/1024/4591.htm END:VEVENT BEGIN:VEVENT UID:5195@kiaa.pku.edu.cn DTSTAMP:20180806T111005Z CREATED:20180806T111005Z DESCRIPTION:The 2018 KIAA-PKU Astrophysics Forum DTSTART;TZID=Asia/Shanghai:20181203T090000 DTEND;TZID=Asia/Shanghai:20181204T170000 LAST-MODIFIED:20180806T111005Z LOCATION:Auditorium, KIAA SUMMARY:The 2018 KIAA-PKU Astrophysics Forum URL;TYPE=URI:/info/1026/5195.htm END:VEVENT BEGIN:VEVENT UID:4748@kiaa.pku.edu.cn DTSTAMP:20181019T190715Z CREATED:20181019T190715Z DESCRIPTION:Lunar Occultation: A technique to achieve high angular resolution even with a single 1-m class telescope DTSTART;TZID=Asia/Shanghai:20181206T120000 DTEND;TZID=Asia/Shanghai:20181206T130000 LAST-MODIFIED:20181019T190715Z LOCATION:KIAA-PKU SUMMARY:Lunar Occultation: A technique to achieve high angular resolution even with a single 1-m class telescope URL;TYPE=URI:/info/1028/4748.htm END:VEVENT BEGIN:VEVENT UID:4828@kiaa.pku.edu.cn DTSTAMP:20190916T094250Z CREATED:20190916T094250Z DESCRIPTION:Constraining the Ejecta for the Nonthermal Emission from GW 170817 DTSTART;TZID=Asia/Shanghai:20181207T170000 DTEND;TZID=Asia/Shanghai:20181207T170000 LAST-MODIFIED:20190916T094250Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Constraining the Ejecta for the Nonthermal Emission from GW 170817 URL;TYPE=URI:/info/1029/4828.htm END:VEVENT BEGIN:VEVENT UID:5085@kiaa.pku.edu.cn DTSTAMP:20181130T140417Z CREATED:20181130T140417Z DESCRIPTION:Recent developments in the modelling of the solar chromosphere DTSTART;TZID=Asia/Shanghai:20181210T120000 DTEND;TZID=Asia/Shanghai:20181210T130000 LAST-MODIFIED:20181130T140417Z LOCATION:first floor meeting room, KIAA SUMMARY:Recent developments in the modelling of the solar chromosphere URL;TYPE=URI:/info/1025/5085.htm END:VEVENT BEGIN:VEVENT UID:4749@kiaa.pku.edu.cn DTSTAMP:20181019T190758Z CREATED:20181019T190758Z DESCRIPTION:Globular clusters as a tracer of galaxy formation and evolution: a case study of M85 DTSTART;TZID=Asia/Shanghai:20181211T120000 DTEND;TZID=Asia/Shanghai:20181211T130000 LAST-MODIFIED:20181019T190758Z LOCATION:KIAA-PKU SUMMARY:Globular clusters as a tracer of galaxy formation and evolution: a case study of M85 URL;TYPE=URI:/info/1028/4749.htm END:VEVENT BEGIN:VEVENT UID:4321@kiaa.pku.edu.cn DTSTAMP:20181213T082147Z CREATED:20181213T082147Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20181213T133000 DTEND;TZID=Asia/Shanghai:20181213T140000 LAST-MODIFIED:20181213T082147Z LOCATION:KIAA second floor, common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4321.htm END:VEVENT BEGIN:VEVENT UID:4583@kiaa.pku.edu.cn DTSTAMP:20181006T222401Z CREATED:20181006T222401Z DESCRIPTION:X-raying galactic feedback in nearby disk galaxies DTSTART;TZID=Asia/Shanghai:20181213T160000 DTEND;TZID=Asia/Shanghai:20181213T170000 LAST-MODIFIED:20181006T222401Z LOCATION:KIAA-PKU Auditorium SUMMARY:X-raying galactic feedback in nearby disk galaxies URL;TYPE=URI:/info/1024/4583.htm END:VEVENT BEGIN:VEVENT UID:5090@kiaa.pku.edu.cn DTSTAMP:20181025T105129Z CREATED:20181025T105129Z DESCRIPTION:Scatterings on a sphere DTSTART;TZID=Asia/Shanghai:20181214T120000 DTEND;TZID=Asia/Shanghai:20181214T130000 LAST-MODIFIED:20181025T105129Z LOCATION:first floor meeting room, KIAA SUMMARY:Scatterings on a sphere URL;TYPE=URI:/info/1025/5090.htm END:VEVENT BEGIN:VEVENT UID:5083@kiaa.pku.edu.cn DTSTAMP:20181203T123837Z CREATED:20181203T123837Z DESCRIPTION:Towards a Full MHD Jet Model of Spinning Black Holes DTSTART;TZID=Asia/Shanghai:20181217T120000 DTEND;TZID=Asia/Shanghai:20181217T130000 LAST-MODIFIED:20181203T123837Z LOCATION:DoA, Rm 2907 SUMMARY:Towards a Full MHD Jet Model of Spinning Black Holes URL;TYPE=URI:/info/1025/5083.htm END:VEVENT BEGIN:VEVENT UID:6705@kiaa.pku.edu.cn DTSTAMP:20181105T141726Z CREATED:20181105T141726Z DESCRIPTION:Postdoc Science Day DTSTART;TZID=Asia/Shanghai:20181218T100000 DTEND;TZID=Asia/Shanghai:20181219T170000 LAST-MODIFIED:20181105T141726Z LOCATION:KIAA Auditorium SUMMARY:Postdoc Science Day URL;TYPE=URI:/info/1089/6705.htm END:VEVENT BEGIN:VEVENT UID:4829@kiaa.pku.edu.cn DTSTAMP:20190916T094330Z CREATED:20190916T094330Z DESCRIPTION:An Overview on Fast Radio Burst and FRB Luminosity Function DTSTART;TZID=Asia/Shanghai:20181218T170000 DTEND;TZID=Asia/Shanghai:20181218T170000 LAST-MODIFIED:20190916T094330Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:An Overview on Fast Radio Burst and FRB Luminosity Function URL;TYPE=URI:/info/1029/4829.htm END:VEVENT BEGIN:VEVENT UID:5092@kiaa.pku.edu.cn DTSTAMP:20181022T221403Z CREATED:20181022T221403Z DESCRIPTION:Probing axions with neutron star inspirals observed by Advanced LIGO DTSTART;TZID=Asia/Shanghai:20181220T120000 DTEND;TZID=Asia/Shanghai:20181220T130000 LAST-MODIFIED:20181022T221403Z LOCATION:1st floor meeting room, KIAA SUMMARY:Probing axions with neutron star inspirals observed by Advanced LIGO URL;TYPE=URI:/info/1025/5092.htm END:VEVENT BEGIN:VEVENT UID:4589@kiaa.pku.edu.cn DTSTAMP:20181026T153221Z CREATED:20181026T153221Z DESCRIPTION:Data Oriented GRB Research and the Gravitational Wave GRBs DTSTART;TZID=Asia/Shanghai:20181220T160000 DTEND;TZID=Asia/Shanghai:20181220T170000 LAST-MODIFIED:20181026T153221Z LOCATION:KIAA-PKU Auditorium SUMMARY:Data Oriented GRB Research and the Gravitational Wave GRBs URL;TYPE=URI:/info/1024/4589.htm END:VEVENT BEGIN:VEVENT UID:5087@kiaa.pku.edu.cn DTSTAMP:20181104T101205Z CREATED:20181104T101205Z DESCRIPTION:Extragalactic Cosmic Accelerators Through the Eyes of Ground-Based Gamma-Ray Telescopes DTSTART;TZID=Asia/Shanghai:20181221T120000 DTEND;TZID=Asia/Shanghai:20181221T130000 LAST-MODIFIED:20181104T101205Z LOCATION:first floor meeting room SUMMARY:Extragalactic Cosmic Accelerators Through the Eyes of Ground-Based Gamma-Ray Telescopes URL;TYPE=URI:/info/1025/5087.htm END:VEVENT BEGIN:VEVENT UID:4750@kiaa.pku.edu.cn DTSTAMP:20181019T191016Z CREATED:20181019T191016Z DESCRIPTION:A changing look AGN discovered in LAMOST quasar survey DTSTART;TZID=Asia/Shanghai:20181225T120000 DTEND;TZID=Asia/Shanghai:20181225T130000 LAST-MODIFIED:20181019T191016Z LOCATION:KIAA-PKU SUMMARY:A changing look AGN discovered in LAMOST quasar survey URL;TYPE=URI:/info/1028/4750.htm END:VEVENT BEGIN:VEVENT UID:5084@kiaa.pku.edu.cn DTSTAMP:20181203T090228Z CREATED:20181203T090228Z DESCRIPTION:A New X-Ray Selected Galaxy Cluster Sample from the ROSAT All-Sky Survey DTSTART;TZID=Asia/Shanghai:20181227T120000 DTEND;TZID=Asia/Shanghai:20181227T130000 LAST-MODIFIED:20181203T090228Z LOCATION:first floor meeting room, KIAA SUMMARY:A New X-Ray Selected Galaxy Cluster Sample from the ROSAT All-Sky Survey URL;TYPE=URI:/info/1025/5084.htm END:VEVENT BEGIN:VEVENT UID:5097@kiaa.pku.edu.cn DTSTAMP:20181002T133447Z CREATED:20181002T133447Z DESCRIPTION:Star cluster formation at various scales: from galaxies to giant molecular clouds. DTSTART;TZID=Asia/Shanghai:20181228T120000 DTEND;TZID=Asia/Shanghai:20181228T130000 LAST-MODIFIED:20181002T133447Z LOCATION:KIAA, 1st meeting room SUMMARY:Star cluster formation at various scales: from galaxies to giant molecular clouds. URL;TYPE=URI:/info/1025/5097.htm END:VEVENT BEGIN:VEVENT UID:5089@kiaa.pku.edu.cn DTSTAMP:20181029T104936Z CREATED:20181029T104936Z DESCRIPTION:Differentially rotating quark stars with realistic angular velocity profile DTSTART;TZID=Asia/Shanghai:20181231T120000 DTEND;TZID=Asia/Shanghai:20181231T120000 LAST-MODIFIED:20181029T104936Z LOCATION:DoA, Rm 2907 SUMMARY:Differentially rotating quark stars with realistic angular velocity profile URL;TYPE=URI:/info/1025/5089.htm END:VEVENT BEGIN:VEVENT UID:6707@kiaa.pku.edu.cn DTSTAMP:20181214T120243Z CREATED:20181214T120243Z DESCRIPTION:New Year's Day Holiday DTSTART;TZID=Asia/Shanghai:20190101T000000 DTEND;TZID=Asia/Shanghai:20190101T000000 LAST-MODIFIED:20181214T120243Z LOCATION: SUMMARY:New Year's Day Holiday URL;TYPE=URI:/info/1089/6707.htm END:VEVENT BEGIN:VEVENT UID:4830@kiaa.pku.edu.cn DTSTAMP:20190916T094555Z CREATED:20190916T094555Z DESCRIPTION:Tracing the near-infrared variabilities of embedded young stellar objects DTSTART;TZID=Asia/Shanghai:20190104T170000 DTEND;TZID=Asia/Shanghai:20190104T170000 LAST-MODIFIED:20190916T094555Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Tracing the near-infrared variabilities of embedded young stellar objects URL;TYPE=URI:/info/1029/4830.htm END:VEVENT BEGIN:VEVENT UID:4751@kiaa.pku.edu.cn DTSTAMP:20181019T191124Z CREATED:20181019T191124Z DESCRIPTION:Rotation curves and mass distribution of nearby spiral and dwarf galaxies. DTSTART;TZID=Asia/Shanghai:20190108T120000 DTEND;TZID=Asia/Shanghai:20190108T130000 LAST-MODIFIED:20181019T191124Z LOCATION:KIAA-PKU SUMMARY:Rotation curves and mass distribution of nearby spiral and dwarf galaxies. URL;TYPE=URI:/info/1028/4751.htm END:VEVENT BEGIN:VEVENT UID:6740@kiaa.pku.edu.cn DTSTAMP:20181220T155048Z CREATED:20181220T155048Z DESCRIPTION:Lunch Talk DTSTART;TZID=Asia/Shanghai:20190109T000000 DTEND;TZID=Asia/Shanghai:20190111T000000 LAST-MODIFIED:20181220T155048Z LOCATION: SUMMARY:Lunch Talk URL;TYPE=URI:/info/1089/6740.htm END:VEVENT BEGIN:VEVENT UID:4594@kiaa.pku.edu.cn DTSTAMP:20181227T140734Z CREATED:20181227T140734Z DESCRIPTION:The galaxy-halo connection with strong and weak gravitational lensing DTSTART;TZID=Asia/Shanghai:20190109T160000 DTEND;TZID=Asia/Shanghai:20190109T180000 LAST-MODIFIED:20181227T140734Z LOCATION:KIAA-PKU Auditorium SUMMARY:The galaxy-halo connection with strong and weak gravitational lensing URL;TYPE=URI:/info/1024/4594.htm END:VEVENT BEGIN:VEVENT UID:5010@kiaa.pku.edu.cn DTSTAMP:20181227T141348Z CREATED:20181227T141348Z DESCRIPTION:lunch discussion with graduates DTSTART;TZID=Asia/Shanghai:20190110T120000 DTEND;TZID=Asia/Shanghai:20190110T140000 LAST-MODIFIED:20181227T141348Z LOCATION:the meeting room of the second floor,KIAA SUMMARY:lunch discussion with graduates URL;TYPE=URI:/info/1025/5010.htm END:VEVENT BEGIN:VEVENT UID:5012@kiaa.pku.edu.cn DTSTAMP:20181227T141825Z CREATED:20181227T141825Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20190110T120000 DTEND;TZID=Asia/Shanghai:20190110T140000 LAST-MODIFIED:20181227T141825Z LOCATION:Meeting Room of the first floor, KIAA SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5012.htm END:VEVENT BEGIN:VEVENT UID:4593@kiaa.pku.edu.cn DTSTAMP:20181227T140612Z CREATED:20181227T140612Z DESCRIPTION:Bridging the Milky Way to the universe -- from the perspective of chemical evolution DTSTART;TZID=Asia/Shanghai:20190110T160000 DTEND;TZID=Asia/Shanghai:20190110T180000 LAST-MODIFIED:20181227T140612Z LOCATION:KIAA-PKU Auditorium SUMMARY:Bridging the Milky Way to the universe -- from the perspective of chemical evolution URL;TYPE=URI:/info/1024/4593.htm END:VEVENT BEGIN:VEVENT UID:5013@kiaa.pku.edu.cn DTSTAMP:20181227T142119Z CREATED:20181227T142119Z DESCRIPTION:lunch discussion with graduates DTSTART;TZID=Asia/Shanghai:20190111T120000 DTEND;TZID=Asia/Shanghai:20190111T140000 LAST-MODIFIED:20181227T142119Z LOCATION:Meeting Room of the second floor, KIAA SUMMARY:lunch discussion with graduates URL;TYPE=URI:/info/1025/5013.htm END:VEVENT BEGIN:VEVENT UID:5011@kiaa.pku.edu.cn DTSTAMP:20181227T141615Z CREATED:20181227T141615Z DESCRIPTION:lunch discussion with postdocs DTSTART;TZID=Asia/Shanghai:20190111T120000 DTEND;TZID=Asia/Shanghai:20190111T140000 LAST-MODIFIED:20181227T141615Z LOCATION:Meeting Room of the first floor, KIAA SUMMARY:lunch discussion with postdocs URL;TYPE=URI:/info/1025/5011.htm END:VEVENT BEGIN:VEVENT UID:4584@kiaa.pku.edu.cn DTSTAMP:20181009T002839Z CREATED:20181009T002839Z DESCRIPTION:Neutron stars as fundamental physics laboratories DTSTART;TZID=Asia/Shanghai:20190111T160000 DTEND;TZID=Asia/Shanghai:20190111T170000 LAST-MODIFIED:20181009T002839Z LOCATION:KIAA-PKU Auditorium SUMMARY:Neutron stars as fundamental physics laboratories URL;TYPE=URI:/info/1024/4584.htm END:VEVENT BEGIN:VEVENT UID:5014@kiaa.pku.edu.cn DTSTAMP:20190110T134317Z CREATED:20190110T134317Z DESCRIPTION:Hierarchical Assembly of Brightest Cluster Galaxies DTSTART;TZID=Asia/Shanghai:20190114T120000 DTEND;TZID=Asia/Shanghai:20190114T130000 LAST-MODIFIED:20190110T134317Z LOCATION:KIAA 1st meeting room SUMMARY:Hierarchical Assembly of Brightest Cluster Galaxies URL;TYPE=URI:/info/1025/5014.htm END:VEVENT BEGIN:VEVENT UID:4752@kiaa.pku.edu.cn DTSTAMP:20181019T191220Z CREATED:20181019T191220Z DESCRIPTION:How will the formation history of infall halos affect the satellite galaxies? DTSTART;TZID=Asia/Shanghai:20190118T120000 DTEND;TZID=Asia/Shanghai:20190118T130000 LAST-MODIFIED:20181019T191220Z LOCATION:KIAA-PKU SUMMARY:How will the formation history of infall halos affect the satellite galaxies? URL;TYPE=URI:/info/1028/4752.htm END:VEVENT BEGIN:VEVENT UID:6696@kiaa.pku.edu.cn DTSTAMP:20180301T084033Z CREATED:20180301T084033Z DESCRIPTION:Winter Holiday for Faculty & Admin DTSTART;TZID=Asia/Shanghai:20190120T000000 DTEND;TZID=Asia/Shanghai:20190217T000000 LAST-MODIFIED:20180301T084033Z LOCATION: SUMMARY:Winter Holiday for Faculty & Admin URL;TYPE=URI:/info/1089/6696.htm END:VEVENT BEGIN:VEVENT UID:5082@kiaa.pku.edu.cn DTSTAMP:20181218T121149Z CREATED:20181218T121149Z DESCRIPTION:The early growth of supermassive black holes as seen by Chandra DTSTART;TZID=Asia/Shanghai:20190121T120000 DTEND;TZID=Asia/Shanghai:20190121T130000 LAST-MODIFIED:20181218T121149Z LOCATION:KIAA 1st meeting room SUMMARY:The early growth of supermassive black holes as seen by Chandra URL;TYPE=URI:/info/1025/5082.htm END:VEVENT BEGIN:VEVENT UID:6738@kiaa.pku.edu.cn DTSTAMP:20190227T083411Z CREATED:20190227T083411Z DESCRIPTION:Astro-oh DTSTART;TZID=Asia/Shanghai:20190228T133000 DTEND;TZID=Asia/Shanghai:20190228T140000 LAST-MODIFIED:20190227T083411Z LOCATION:KIAA second floor, common place SUMMARY:Astro-oh URL;TYPE=URI:/info/1089/6738.htm END:VEVENT BEGIN:VEVENT UID:4596@kiaa.pku.edu.cn DTSTAMP:20190218T160509Z CREATED:20190218T160509Z DESCRIPTION:Multiwavelength view of hyperluminous dust-obscured quasars at cosmic noon DTSTART;TZID=Asia/Shanghai:20190228T160000 DTEND;TZID=Asia/Shanghai:20190228T170000 LAST-MODIFIED:20190218T160509Z LOCATION:KIAA-PKU Auditorium SUMMARY:Multiwavelength view of hyperluminous dust-obscured quasars at cosmic noon URL;TYPE=URI:/info/1024/4596.htm END:VEVENT BEGIN:VEVENT UID:4753@kiaa.pku.edu.cn DTSTAMP:20181019T191309Z CREATED:20181019T191309Z DESCRIPTION:Automated accurate decomposition of galaxy images. DTSTART;TZID=Asia/Shanghai:20190305T120000 DTEND;TZID=Asia/Shanghai:20190305T130000 LAST-MODIFIED:20181019T191309Z LOCATION:KIAA-PKU SUMMARY:Automated accurate decomposition of galaxy images. URL;TYPE=URI:/info/1028/4753.htm END:VEVENT BEGIN:VEVENT UID:4322@kiaa.pku.edu.cn DTSTAMP:20190303T172332Z CREATED:20190303T172332Z DESCRIPTION:Astro-ph DTSTART;TZID=Asia/Shanghai:20190305T133000 DTEND;TZID=Asia/Shanghai:20190305T140000 LAST-MODIFIED:20190303T172332Z LOCATION:KIAA second floor common area SUMMARY:Astro-ph URL;TYPE=URI:/info/1027/4322.htm END:VEVENT BEGIN:VEVENT UID:5015@kiaa.pku.edu.cn DTSTAMP:20190222T091316Z CREATED:20190222T091316Z DESCRIPTION:The HKU Laboratory for Space Research: Reaching for the Moon, Mars and the Stars. DTSTART;TZID=Asia/Shanghai:20190306T120000 DTEND;TZID=Asia/Shanghai:20190306T130000 LAST-MODIFIED:20190222T091316Z LOCATION:1st Meeting Room, KIAA SUMMARY:The HKU Laboratory for Space Research: Reaching for the Moon, Mars and the Stars. URL;TYPE=URI:/info/1025/5015.htm END:VEVENT BEGIN:VEVENT UID:4597@kiaa.pku.edu.cn DTSTAMP:20190218T160741Z CREATED:20190218T160741Z DESCRIPTION:The kinematics of globular clusters and planetary nebula in the core of the Fornax Cluster: intracluster light and the search of stellar streams DTSTART;TZID=Asia/Shanghai:20190307T160000 DTEND;TZID=Asia/Shanghai:20190307T170000 LAST-MODIFIED:20190218T160741Z LOCATION:KIAA-PKU Auditorium SUMMARY:The kinematics of globular clusters and planetary nebula in the core of the Fornax Cluster: intracluster light and the search of stellar streams URL;TYPE=URI:/info/1024/4597.htm END:VEVENT BEGIN:VEVENT UID:5016@kiaa.pku.edu.cn DTSTAMP:20190225T204147Z CREATED:20190225T204147Z DESCRIPTION:Several applications of the combination of gravitational waves and their electromagnetic counterparts DTSTART;TZID=Asia/Shanghai:20190311T120000 DTEND;TZID=Asia/Shanghai:20190311T130000 LAST-MODIFIED:20190225T204147Z LOCATION:DoA, Rm 2907 SUMMARY:Several applications of the combination of gravitational waves and their electromagnetic counterparts URL;TYPE=URI:/info/1025/5016.htm END:VEVENT BEGIN:VEVENT UID:5017@kiaa.pku.edu.cn DTSTAMP:20190306T155659Z CREATED:20190306T155659Z DESCRIPTION:Co-evolution of supermassive black holes with galaxies from semi-analytic model DTSTART;TZID=Asia/Shanghai:20190312T120000 DTEND;TZID=Asia/Shanghai:20190312T130000 LAST-MODIFIED:20190306T155659Z LOCATION:KIAA 1st meeting room SUMMARY:Co-evolution of supermassive black holes with galaxies from semi-analytic model URL;TYPE=URI:/info/1025/5017.htm END:VEVENT BEGIN:VEVENT UID:4323@kiaa.pku.edu.cn DTSTAMP:20190311T153141Z CREATED:20190311T153141Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190312T133000 DTEND;TZID=Asia/Shanghai:20190312T140000 LAST-MODIFIED:20190311T153141Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4323.htm END:VEVENT BEGIN:VEVENT UID:4334@kiaa.pku.edu.cn DTSTAMP:20190311T153257Z CREATED:20190311T153257Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190314T133000 DTEND;TZID=Asia/Shanghai:20190314T140000 LAST-MODIFIED:20190311T153257Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4334.htm END:VEVENT BEGIN:VEVENT UID:4598@kiaa.pku.edu.cn DTSTAMP:20190218T160840Z CREATED:20190218T160840Z DESCRIPTION:A comprehensive survey of massive star formation in Cygnus-X DTSTART;TZID=Asia/Shanghai:20190314T160000 DTEND;TZID=Asia/Shanghai:20190314T170000 LAST-MODIFIED:20190218T160840Z LOCATION:KIAA-PKU Auditorium SUMMARY:A comprehensive survey of massive star formation in Cygnus-X URL;TYPE=URI:/info/1024/4598.htm END:VEVENT BEGIN:VEVENT UID:5018@kiaa.pku.edu.cn DTSTAMP:20190311T101529Z CREATED:20190311T101529Z DESCRIPTION:Studies on propagation properties of fast radio bursts DTSTART;TZID=Asia/Shanghai:20190318T120000 DTEND;TZID=Asia/Shanghai:20190318T130000 LAST-MODIFIED:20190311T101529Z LOCATION:first meeting room, KIAA SUMMARY:Studies on propagation properties of fast radio bursts URL;TYPE=URI:/info/1025/5018.htm END:VEVENT BEGIN:VEVENT UID:5019@kiaa.pku.edu.cn DTSTAMP:20190312T161158Z CREATED:20190312T161158Z DESCRIPTION:High-resolution spectroscopic analysis of a large sample of Li-rich giants found by LAMOST DTSTART;TZID=Asia/Shanghai:20190319T120000 DTEND;TZID=Asia/Shanghai:20190319T130000 LAST-MODIFIED:20190312T161158Z LOCATION:first meeting room, KIAA SUMMARY:High-resolution spectroscopic analysis of a large sample of Li-rich giants found by LAMOST URL;TYPE=URI:/info/1025/5019.htm END:VEVENT BEGIN:VEVENT UID:4333@kiaa.pku.edu.cn DTSTAMP:20190311T165623Z CREATED:20190311T165623Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190319T133000 DTEND;TZID=Asia/Shanghai:20190319T140000 LAST-MODIFIED:20190311T165623Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4333.htm END:VEVENT BEGIN:VEVENT UID:5021@kiaa.pku.edu.cn DTSTAMP:20190314T164306Z CREATED:20190314T164306Z DESCRIPTION:Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black holes in galactic nuclei DTSTART;TZID=Asia/Shanghai:20190320T120000 DTEND;TZID=Asia/Shanghai:20190320T130000 LAST-MODIFIED:20190314T164306Z LOCATION:KIAA 1st meeting room SUMMARY:Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black holes in galactic nuclei URL;TYPE=URI:/info/1025/5021.htm END:VEVENT BEGIN:VEVENT UID:6739@kiaa.pku.edu.cn DTSTAMP:20190219T152712Z CREATED:20190219T152712Z DESCRIPTION:Kavli Foundation Visit DTSTART;TZID=Asia/Shanghai:20190321T000000 DTEND;TZID=Asia/Shanghai:20190321T120000 LAST-MODIFIED:20190219T152712Z LOCATION: SUMMARY:Kavli Foundation Visit URL;TYPE=URI:/info/1089/6739.htm END:VEVENT BEGIN:VEVENT UID:4324@kiaa.pku.edu.cn DTSTAMP:20190311T165715Z CREATED:20190311T165715Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190321T133000 DTEND;TZID=Asia/Shanghai:20190321T140000 LAST-MODIFIED:20190311T165715Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4324.htm END:VEVENT BEGIN:VEVENT UID:5023@kiaa.pku.edu.cn DTSTAMP:20190318T090020Z CREATED:20190318T090020Z DESCRIPTION:A New Insight into Forming Jupiter’s Dilute Core DTSTART;TZID=Asia/Shanghai:20190322T120000 DTEND;TZID=Asia/Shanghai:20190322T130000 LAST-MODIFIED:20190318T090020Z LOCATION:1st meeting room, KIAA SUMMARY:A New Insight into Forming Jupiter’s Dilute Core URL;TYPE=URI:/info/1025/5023.htm END:VEVENT BEGIN:VEVENT UID:5022@kiaa.pku.edu.cn DTSTAMP:20190315T100527Z CREATED:20190315T100527Z DESCRIPTION:Host Galaxies of Type I QSOs DTSTART;TZID=Asia/Shanghai:20190325T120000 DTEND;TZID=Asia/Shanghai:20190325T130000 LAST-MODIFIED:20190315T100527Z LOCATION:DoA, Rm 2907 SUMMARY:Host Galaxies of Type I QSOs URL;TYPE=URI:/info/1025/5022.htm END:VEVENT BEGIN:VEVENT UID:4325@kiaa.pku.edu.cn DTSTAMP:20190311T165756Z CREATED:20190311T165756Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190326T133000 DTEND;TZID=Asia/Shanghai:20190326T140000 LAST-MODIFIED:20190311T165756Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4325.htm END:VEVENT BEGIN:VEVENT UID:5025@kiaa.pku.edu.cn DTSTAMP:20190321T102055Z CREATED:20190321T102055Z DESCRIPTION:Disentangling galaxy formation history through a population-orbit superposition model DTSTART;TZID=Asia/Shanghai:20190327T120000 DTEND;TZID=Asia/Shanghai:20190327T130000 LAST-MODIFIED:20190321T102055Z LOCATION:KIAA 1st meeting room SUMMARY:Disentangling galaxy formation history through a population-orbit superposition model URL;TYPE=URI:/info/1025/5025.htm END:VEVENT BEGIN:VEVENT UID:5026@kiaa.pku.edu.cn DTSTAMP:20190321T162556Z CREATED:20190321T162556Z DESCRIPTION:Formation of binary stellar-mass black holes from globular clusters: the impact of host clusters' properties DTSTART;TZID=Asia/Shanghai:20190328T120000 DTEND;TZID=Asia/Shanghai:20190328T130000 LAST-MODIFIED:20190321T162556Z LOCATION:DoA Rm2907 SUMMARY:Formation of binary stellar-mass black holes from globular clusters: the impact of host clusters' properties URL;TYPE=URI:/info/1025/5026.htm END:VEVENT BEGIN:VEVENT UID:4326@kiaa.pku.edu.cn DTSTAMP:20190311T165927Z CREATED:20190311T165927Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190328T133000 DTEND;TZID=Asia/Shanghai:20190328T140000 LAST-MODIFIED:20190311T165927Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4326.htm END:VEVENT BEGIN:VEVENT UID:4600@kiaa.pku.edu.cn DTSTAMP:20190220T111050Z CREATED:20190220T111050Z DESCRIPTION:Testing general relativity using X-ray reflection spectroscopy DTSTART;TZID=Asia/Shanghai:20190329T153000 DTEND;TZID=Asia/Shanghai:20190329T163000 LAST-MODIFIED:20190220T111050Z LOCATION:KIAA-PKU Auditorium SUMMARY:Testing general relativity using X-ray reflection spectroscopy URL;TYPE=URI:/info/1024/4600.htm END:VEVENT BEGIN:VEVENT UID:4327@kiaa.pku.edu.cn DTSTAMP:20190311T170016Z CREATED:20190311T170016Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190402T133000 DTEND;TZID=Asia/Shanghai:20190402T140000 LAST-MODIFIED:20190311T170016Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4327.htm END:VEVENT BEGIN:VEVENT UID:4610@kiaa.pku.edu.cn DTSTAMP:20190402T133100Z CREATED:20190402T133100Z DESCRIPTION:Extracting Physics from Gravitational Waves (1/2) DTSTART;TZID=Asia/Shanghai:20190403T100000 DTEND;TZID=Asia/Shanghai:20190403T100000 LAST-MODIFIED:20190402T133100Z LOCATION:K208, KIAA-PKU SUMMARY:Extracting Physics from Gravitational Waves (1/2) URL;TYPE=URI:/info/1024/4610.htm END:VEVENT BEGIN:VEVENT UID:4328@kiaa.pku.edu.cn DTSTAMP:20190311T171414Z CREATED:20190311T171414Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190404T133000 DTEND;TZID=Asia/Shanghai:20190404T140000 LAST-MODIFIED:20190311T171414Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4328.htm END:VEVENT BEGIN:VEVENT UID:4613@kiaa.pku.edu.cn DTSTAMP:20190304T173036Z CREATED:20190304T173036Z DESCRIPTION:Gravitational Lensing of Gravitational Waves DTSTART;TZID=Asia/Shanghai:20190404T160000 DTEND;TZID=Asia/Shanghai:20190404T170000 LAST-MODIFIED:20190304T173036Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gravitational Lensing of Gravitational Waves URL;TYPE=URI:/info/1024/4613.htm END:VEVENT BEGIN:VEVENT UID:6708@kiaa.pku.edu.cn DTSTAMP:20181214T123437Z CREATED:20181214T123437Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20190405T000000 DTEND;TZID=Asia/Shanghai:20190405T000000 LAST-MODIFIED:20181214T123437Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6708.htm END:VEVENT BEGIN:VEVENT UID:4609@kiaa.pku.edu.cn DTSTAMP:20190402T133217Z CREATED:20190402T133217Z DESCRIPTION:Extracting Physics from Gravitational Waves (2/2) DTSTART;TZID=Asia/Shanghai:20190405T100000 DTEND;TZID=Asia/Shanghai:20190405T100000 LAST-MODIFIED:20190402T133217Z LOCATION:1st floor meeting room, KIAA-PKU SUMMARY:Extracting Physics from Gravitational Waves (2/2) URL;TYPE=URI:/info/1024/4609.htm END:VEVENT BEGIN:VEVENT UID:4332@kiaa.pku.edu.cn DTSTAMP:20190311T171611Z CREATED:20190311T171611Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190409T133000 DTEND;TZID=Asia/Shanghai:20190409T140000 LAST-MODIFIED:20190311T171611Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4332.htm END:VEVENT BEGIN:VEVENT UID:4831@kiaa.pku.edu.cn DTSTAMP:20190916T094725Z CREATED:20190916T094725Z DESCRIPTION:The Co-evolution between Quasars and Their Host Galaxies at High Redshift DTSTART;TZID=Asia/Shanghai:20190410T170000 DTEND;TZID=Asia/Shanghai:20190410T170000 LAST-MODIFIED:20190916T094725Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The Co-evolution between Quasars and Their Host Galaxies at High Redshift URL;TYPE=URI:/info/1029/4831.htm END:VEVENT BEGIN:VEVENT UID:5027@kiaa.pku.edu.cn DTSTAMP:20190404T150123Z CREATED:20190404T150123Z DESCRIPTION:Multiwavelength Study of the TeV halo of Geminga DTSTART;TZID=Asia/Shanghai:20190411T120000 DTEND;TZID=Asia/Shanghai:20190411T130000 LAST-MODIFIED:20190404T150123Z LOCATION:1st floor meeting room, KIAA SUMMARY:Multiwavelength Study of the TeV halo of Geminga URL;TYPE=URI:/info/1025/5027.htm END:VEVENT BEGIN:VEVENT UID:4331@kiaa.pku.edu.cn DTSTAMP:20190311T171734Z CREATED:20190311T171734Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190411T133000 DTEND;TZID=Asia/Shanghai:20190411T140000 LAST-MODIFIED:20190311T171734Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4331.htm END:VEVENT BEGIN:VEVENT UID:4621@kiaa.pku.edu.cn DTSTAMP:20190220T111209Z CREATED:20190220T111209Z DESCRIPTION:The habitability of tidally-locked exoplanets: a climatic view DTSTART;TZID=Asia/Shanghai:20190411T160000 DTEND;TZID=Asia/Shanghai:20190411T170000 LAST-MODIFIED:20190220T111209Z LOCATION:KIAA-PKU Auditorium SUMMARY:The habitability of tidally-locked exoplanets: a climatic view URL;TYPE=URI:/info/1024/4621.htm END:VEVENT BEGIN:VEVENT UID:5029@kiaa.pku.edu.cn DTSTAMP:20190406T214229Z CREATED:20190406T214229Z DESCRIPTION:Stochastic background of gravitational waves DTSTART;TZID=Asia/Shanghai:20190412T120000 DTEND;TZID=Asia/Shanghai:20190412T130000 LAST-MODIFIED:20190406T214229Z LOCATION:1st floor meeting room, KIAA SUMMARY:Stochastic background of gravitational waves URL;TYPE=URI:/info/1025/5029.htm END:VEVENT BEGIN:VEVENT UID:4330@kiaa.pku.edu.cn DTSTAMP:20190311T172110Z CREATED:20190311T172110Z DESCRIPTION:astro-ph discussions DTSTART;TZID=Asia/Shanghai:20190416T133000 DTEND;TZID=Asia/Shanghai:20190416T140000 LAST-MODIFIED:20190311T172110Z LOCATION: SUMMARY:astro-ph discussions URL;TYPE=URI:/info/1027/4330.htm END:VEVENT BEGIN:VEVENT UID:5020@kiaa.pku.edu.cn DTSTAMP:20190314T101849Z CREATED:20190314T101849Z DESCRIPTION:DarkSPIDER: a tool to constrain Dark Matter particle candidates with astrophysical observations DTSTART;TZID=Asia/Shanghai:20190417T120000 DTEND;TZID=Asia/Shanghai:20190417T130000 LAST-MODIFIED:20190314T101849Z LOCATION:KIAA 1st meeting room SUMMARY:DarkSPIDER: a tool to constrain Dark Matter particle candidates with astrophysical observations URL;TYPE=URI:/info/1025/5020.htm END:VEVENT BEGIN:VEVENT UID:4599@kiaa.pku.edu.cn DTSTAMP:20190218T160959Z CREATED:20190218T160959Z DESCRIPTION:Probing gamma-ray sky with Fermi DTSTART;TZID=Asia/Shanghai:20190418T160000 DTEND;TZID=Asia/Shanghai:20190418T170000 LAST-MODIFIED:20190218T160959Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing gamma-ray sky with Fermi URL;TYPE=URI:/info/1024/4599.htm END:VEVENT BEGIN:VEVENT UID:5033@kiaa.pku.edu.cn DTSTAMP:20190415T085058Z CREATED:20190415T085058Z DESCRIPTION:Too fast, too furious: rapid formation of hot planets by gravitational instability DTSTART;TZID=Asia/Shanghai:20190419T120000 DTEND;TZID=Asia/Shanghai:20190419T130000 LAST-MODIFIED:20190415T085058Z LOCATION:KIAA 1st meeting room SUMMARY:Too fast, too furious: rapid formation of hot planets by gravitational instability URL;TYPE=URI:/info/1025/5033.htm END:VEVENT BEGIN:VEVENT UID:5031@kiaa.pku.edu.cn DTSTAMP:20190409T095122Z CREATED:20190409T095122Z DESCRIPTION:High-mass X-ray binaries in nearby galaxies DTSTART;TZID=Asia/Shanghai:20190423T120000 DTEND;TZID=Asia/Shanghai:20190423T130000 LAST-MODIFIED:20190409T095122Z LOCATION:1st floor meeting room, KIAA SUMMARY:High-mass X-ray binaries in nearby galaxies URL;TYPE=URI:/info/1025/5031.htm END:VEVENT BEGIN:VEVENT UID:4762@kiaa.pku.edu.cn DTSTAMP:20190306T211112Z CREATED:20190306T211112Z DESCRIPTION:X-shaped Radio Galaxies DTSTART;TZID=Asia/Shanghai:20190424T120000 DTEND;TZID=Asia/Shanghai:20190424T120000 LAST-MODIFIED:20190306T211112Z LOCATION:KIAA-PKU SUMMARY:X-shaped Radio Galaxies URL;TYPE=URI:/info/1028/4762.htm END:VEVENT BEGIN:VEVENT UID:4595@kiaa.pku.edu.cn DTSTAMP:20190110T170108Z CREATED:20190110T170108Z DESCRIPTION:The Assembly of Galaxies at the Highest Redshifts DTSTART;TZID=Asia/Shanghai:20190425T160000 DTEND;TZID=Asia/Shanghai:20190425T170000 LAST-MODIFIED:20190110T170108Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Assembly of Galaxies at the Highest Redshifts URL;TYPE=URI:/info/1024/4595.htm END:VEVENT BEGIN:VEVENT UID:5032@kiaa.pku.edu.cn DTSTAMP:20190411T161034Z CREATED:20190411T161034Z DESCRIPTION:The Optical to Mid-Infrared Extinction Law--An Adjustment to the Classic Rv=3.1 Extinction Law DTSTART;TZID=Asia/Shanghai:20190426T120000 DTEND;TZID=Asia/Shanghai:20190426T130000 LAST-MODIFIED:20190411T161034Z LOCATION:1st floor meeting room, KIAA SUMMARY:The Optical to Mid-Infrared Extinction Law--An Adjustment to the Classic Rv=3.1 Extinction Law URL;TYPE=URI:/info/1025/5032.htm END:VEVENT BEGIN:VEVENT UID:6699@kiaa.pku.edu.cn DTSTAMP:20180905T110711Z CREATED:20180905T110711Z DESCRIPTION:Labor Day Holiday DTSTART;TZID=Asia/Shanghai:20190429T000000 DTEND;TZID=Asia/Shanghai:20190503T000000 LAST-MODIFIED:20180905T110711Z LOCATION: SUMMARY:Labor Day Holiday URL;TYPE=URI:/info/1089/6699.htm END:VEVENT BEGIN:VEVENT UID:5040@kiaa.pku.edu.cn DTSTAMP:20190504T214128Z CREATED:20190504T214128Z DESCRIPTION:Massive black hole triplets: implications for PTA and LISA DTSTART;TZID=Asia/Shanghai:20190510T120000 DTEND;TZID=Asia/Shanghai:20190510T130000 LAST-MODIFIED:20190504T214128Z LOCATION:first meeting room, KIAA SUMMARY:Massive black hole triplets: implications for PTA and LISA URL;TYPE=URI:/info/1025/5040.htm END:VEVENT BEGIN:VEVENT UID:4761@kiaa.pku.edu.cn DTSTAMP:20190306T211236Z CREATED:20190306T211236Z DESCRIPTION:The growth of spheroidal components in numerical simulations DTSTART;TZID=Asia/Shanghai:20190514T120000 DTEND;TZID=Asia/Shanghai:20190514T120000 LAST-MODIFIED:20190306T211236Z LOCATION:KIAA-PKU SUMMARY:The growth of spheroidal components in numerical simulations URL;TYPE=URI:/info/1028/4761.htm END:VEVENT BEGIN:VEVENT UID:4620@kiaa.pku.edu.cn DTSTAMP:20190220T112443Z CREATED:20190220T112443Z DESCRIPTION:Gravitational wave astronomy around 0.1-10 Hz DTSTART;TZID=Asia/Shanghai:20190516T160000 DTEND;TZID=Asia/Shanghai:20190516T170000 LAST-MODIFIED:20190220T112443Z LOCATION:KIAA-PKU Auditorium SUMMARY:Gravitational wave astronomy around 0.1-10 Hz URL;TYPE=URI:/info/1024/4620.htm END:VEVENT BEGIN:VEVENT UID:5037@kiaa.pku.edu.cn DTSTAMP:20190429T103800Z CREATED:20190429T103800Z DESCRIPTION:PARSEC-COLIBRI stellar evolution models DTSTART;TZID=Asia/Shanghai:20190517T120000 DTEND;TZID=Asia/Shanghai:20190517T130000 LAST-MODIFIED:20190429T103800Z LOCATION:KIAA 1st meeting room SUMMARY:PARSEC-COLIBRI stellar evolution models URL;TYPE=URI:/info/1025/5037.htm END:VEVENT BEGIN:VEVENT UID:4615@kiaa.pku.edu.cn DTSTAMP:20190225T171217Z CREATED:20190225T171217Z DESCRIPTION:Chemical evolution of galaxies DTSTART;TZID=Asia/Shanghai:20190520T160000 DTEND;TZID=Asia/Shanghai:20190520T170000 LAST-MODIFIED:20190225T171217Z LOCATION:KIAA-PKU Auditorium SUMMARY:Chemical evolution of galaxies URL;TYPE=URI:/info/1024/4615.htm END:VEVENT BEGIN:VEVENT UID:4760@kiaa.pku.edu.cn DTSTAMP:20190306T211351Z CREATED:20190306T211351Z DESCRIPTION:Towards Mira distance scale in the LSST-JWST era DTSTART;TZID=Asia/Shanghai:20190521T120000 DTEND;TZID=Asia/Shanghai:20190521T120000 LAST-MODIFIED:20190306T211351Z LOCATION:KIAA-PKU SUMMARY:Towards Mira distance scale in the LSST-JWST era URL;TYPE=URI:/info/1028/4760.htm END:VEVENT BEGIN:VEVENT UID:5030@kiaa.pku.edu.cn DTSTAMP:20190408T134509Z CREATED:20190408T134509Z DESCRIPTION:The Snowball Bifurcation on Tidally Locked Planets DTSTART;TZID=Asia/Shanghai:20190522T120000 DTEND;TZID=Asia/Shanghai:20190522T130000 LAST-MODIFIED:20190408T134509Z LOCATION:KIAA 1st meeting room SUMMARY:The Snowball Bifurcation on Tidally Locked Planets URL;TYPE=URI:/info/1025/5030.htm END:VEVENT BEGIN:VEVENT UID:4608@kiaa.pku.edu.cn DTSTAMP:20190416T101358Z CREATED:20190416T101358Z DESCRIPTION:The early life of millisecond magnetars DTSTART;TZID=Asia/Shanghai:20190522T160000 DTEND;TZID=Asia/Shanghai:20190522T170000 LAST-MODIFIED:20190416T101358Z LOCATION:KIAA-PKU Auditorium SUMMARY:The early life of millisecond magnetars URL;TYPE=URI:/info/1024/4608.htm END:VEVENT BEGIN:VEVENT UID:4832@kiaa.pku.edu.cn DTSTAMP:20190916T095418Z CREATED:20190916T095418Z DESCRIPTION:The Infrared Emission and Opening Angle of the Torus in Quasars DTSTART;TZID=Asia/Shanghai:20190522T170000 DTEND;TZID=Asia/Shanghai:20190522T170000 LAST-MODIFIED:20190916T095418Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:The Infrared Emission and Opening Angle of the Torus in Quasars URL;TYPE=URI:/info/1029/4832.htm END:VEVENT BEGIN:VEVENT UID:4619@kiaa.pku.edu.cn DTSTAMP:20190220T112750Z CREATED:20190220T112750Z DESCRIPTION:Early Star Forming Galaxies and Cosmic Reionization DTSTART;TZID=Asia/Shanghai:20190523T160000 DTEND;TZID=Asia/Shanghai:20190523T170000 LAST-MODIFIED:20190220T112750Z LOCATION:KIAA-PKU Auditorium SUMMARY:Early Star Forming Galaxies and Cosmic Reionization URL;TYPE=URI:/info/1024/4619.htm END:VEVENT BEGIN:VEVENT UID:6736@kiaa.pku.edu.cn DTSTAMP:20190521T145720Z CREATED:20190521T145720Z DESCRIPTION:final postdoc defense of DR. Wang Shu DTSTART;TZID=Asia/Shanghai:20190527T160000 DTEND;TZID=Asia/Shanghai:20190527T170000 LAST-MODIFIED:20190521T145720Z LOCATION: SUMMARY:final postdoc defense of DR. Wang Shu URL;TYPE=URI:/info/1089/6736.htm END:VEVENT BEGIN:VEVENT UID:4759@kiaa.pku.edu.cn DTSTAMP:20190306T211509Z CREATED:20190306T211509Z DESCRIPTION:Strong MgII and FeII systems at high-z and their possible associated galaxies DTSTART;TZID=Asia/Shanghai:20190528T120000 DTEND;TZID=Asia/Shanghai:20190528T120000 LAST-MODIFIED:20190306T211509Z LOCATION:KIAA-PKU SUMMARY:Strong MgII and FeII systems at high-z and their possible associated galaxies URL;TYPE=URI:/info/1028/4759.htm END:VEVENT BEGIN:VEVENT UID:5034@kiaa.pku.edu.cn DTSTAMP:20190419T000740Z CREATED:20190419T000740Z DESCRIPTION:Detection of the Circumgalactic Medium of Nearby Galaxies via Emission Lines DTSTART;TZID=Asia/Shanghai:20190529T120000 DTEND;TZID=Asia/Shanghai:20190529T130000 LAST-MODIFIED:20190419T000740Z LOCATION:KIAA 1st meeting room SUMMARY:Detection of the Circumgalactic Medium of Nearby Galaxies via Emission Lines URL;TYPE=URI:/info/1025/5034.htm END:VEVENT BEGIN:VEVENT UID:4618@kiaa.pku.edu.cn DTSTAMP:20190220T112924Z CREATED:20190220T112924Z DESCRIPTION:Elementary Particles and Future Colliders DTSTART;TZID=Asia/Shanghai:20190530T160000 DTEND;TZID=Asia/Shanghai:20190530T170000 LAST-MODIFIED:20190220T112924Z LOCATION:KIAA-PKU Auditorium SUMMARY:Elementary Particles and Future Colliders URL;TYPE=URI:/info/1024/4618.htm END:VEVENT BEGIN:VEVENT UID:6737@kiaa.pku.edu.cn DTSTAMP:20190510T091018Z CREATED:20190510T091018Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20190531T120000 DTEND;TZID=Asia/Shanghai:20190531T140000 LAST-MODIFIED:20190510T091018Z LOCATION:1st meeting room SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1089/6737.htm END:VEVENT BEGIN:VEVENT UID:5041@kiaa.pku.edu.cn DTSTAMP:20190507T143128Z CREATED:20190507T143128Z DESCRIPTION:Exploring accretion and jet in Narrow-Line Seyfert 1 galaxies DTSTART;TZID=Asia/Shanghai:20190603T120000 DTEND;TZID=Asia/Shanghai:20190603T130000 LAST-MODIFIED:20190507T143128Z LOCATION:first meeting room, KIAA SUMMARY:Exploring accretion and jet in Narrow-Line Seyfert 1 galaxies URL;TYPE=URI:/info/1025/5041.htm END:VEVENT BEGIN:VEVENT UID:5038@kiaa.pku.edu.cn DTSTAMP:20190429T171033Z CREATED:20190429T171033Z DESCRIPTION:Light Echoes Around Type Ia Supernova 2014J - From Near and Far DTSTART;TZID=Asia/Shanghai:20190605T120000 DTEND;TZID=Asia/Shanghai:20190605T130000 LAST-MODIFIED:20190429T171033Z LOCATION:KIAA 1st meeting room SUMMARY:Light Echoes Around Type Ia Supernova 2014J - From Near and Far URL;TYPE=URI:/info/1025/5038.htm END:VEVENT BEGIN:VEVENT UID:4617@kiaa.pku.edu.cn DTSTAMP:20190220T113024Z CREATED:20190220T113024Z DESCRIPTION:Closeby Habitable Exoplanet Survey DTSTART;TZID=Asia/Shanghai:20190606T160000 DTEND;TZID=Asia/Shanghai:20190606T170000 LAST-MODIFIED:20190220T113024Z LOCATION:KIAA-PKU Auditorium SUMMARY:Closeby Habitable Exoplanet Survey URL;TYPE=URI:/info/1024/4617.htm END:VEVENT BEGIN:VEVENT UID:6743@kiaa.pku.edu.cn DTSTAMP:20181214T124353Z CREATED:20181214T124353Z DESCRIPTION:Dragon Boat Festival Holiday DTSTART;TZID=Asia/Shanghai:20190607T000000 DTEND;TZID=Asia/Shanghai:20190607T000000 LAST-MODIFIED:20181214T124353Z LOCATION: SUMMARY:Dragon Boat Festival Holiday URL;TYPE=URI:/info/1089/6743.htm END:VEVENT BEGIN:VEVENT UID:5024@kiaa.pku.edu.cn DTSTAMP:20190318T113441Z CREATED:20190318T113441Z DESCRIPTION:Wind mass transfer in AGB binaries DTSTART;TZID=Asia/Shanghai:20190610T114500 DTEND;TZID=Asia/Shanghai:20190610T114500 LAST-MODIFIED:20190318T113441Z LOCATION:1st meeting room, KIAA SUMMARY:Wind mass transfer in AGB binaries URL;TYPE=URI:/info/1025/5024.htm END:VEVENT BEGIN:VEVENT UID:6735@kiaa.pku.edu.cn DTSTAMP:20190606T172015Z CREATED:20190606T172015Z DESCRIPTION:The 2nd-year Graduate students' thesis project report DTSTART;TZID=Asia/Shanghai:20190610T130000 DTEND;TZID=Asia/Shanghai:20190610T170000 LAST-MODIFIED:20190606T172015Z LOCATION: SUMMARY:The 2nd-year Graduate students' thesis project report URL;TYPE=URI:/info/1089/6735.htm END:VEVENT BEGIN:VEVENT UID:4755@kiaa.pku.edu.cn DTSTAMP:20190306T211655Z CREATED:20190306T211655Z DESCRIPTION:ProFound: source extraction and application to modern survey data DTSTART;TZID=Asia/Shanghai:20190611T120000 DTEND;TZID=Asia/Shanghai:20190611T120000 LAST-MODIFIED:20190306T211655Z LOCATION:KIAA-PKU SUMMARY:ProFound: source extraction and application to modern survey data URL;TYPE=URI:/info/1028/4755.htm END:VEVENT BEGIN:VEVENT UID:5028@kiaa.pku.edu.cn DTSTAMP:20190404T150246Z CREATED:20190404T150246Z DESCRIPTION:GRAVITY science highlights and technical challenge/advance in near-infrared interferometry DTSTART;TZID=Asia/Shanghai:20190612T120000 DTEND;TZID=Asia/Shanghai:20190612T130000 LAST-MODIFIED:20190404T150246Z LOCATION:1st floor meeting room, KIAA SUMMARY:GRAVITY science highlights and technical challenge/advance in near-infrared interferometry URL;TYPE=URI:/info/1025/5028.htm END:VEVENT BEGIN:VEVENT UID:4836@kiaa.pku.edu.cn DTSTAMP:20190916T095457Z CREATED:20190916T095457Z DESCRIPTION:Experience Sharing on Postdoc Position Application DTSTART;TZID=Asia/Shanghai:20190612T170000 DTEND;TZID=Asia/Shanghai:20190612T170000 LAST-MODIFIED:20190916T095457Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Experience Sharing on Postdoc Position Application URL;TYPE=URI:/info/1029/4836.htm END:VEVENT BEGIN:VEVENT UID:4614@kiaa.pku.edu.cn DTSTAMP:20190301T170920Z CREATED:20190301T170920Z DESCRIPTION:The Potential Habitability of Rocky Planets around Red Dwarfs: Stellar Drivers for Atmospheric Chemistry and Stability DTSTART;TZID=Asia/Shanghai:20190613T160000 DTEND;TZID=Asia/Shanghai:20190613T170000 LAST-MODIFIED:20190301T170920Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Potential Habitability of Rocky Planets around Red Dwarfs: Stellar Drivers for Atmospheric Chemistry and Stability URL;TYPE=URI:/info/1024/4614.htm END:VEVENT BEGIN:VEVENT UID:5039@kiaa.pku.edu.cn DTSTAMP:20190429T171148Z CREATED:20190429T171148Z DESCRIPTION:Exploring the missing links in massive star explosions DTSTART;TZID=Asia/Shanghai:20190614T120000 DTEND;TZID=Asia/Shanghai:20190614T130000 LAST-MODIFIED:20190429T171148Z LOCATION:KIAA 1st meeting room SUMMARY:Exploring the missing links in massive star explosions URL;TYPE=URI:/info/1025/5039.htm END:VEVENT BEGIN:VEVENT UID:5035@kiaa.pku.edu.cn DTSTAMP:20190423T140931Z CREATED:20190423T140931Z DESCRIPTION:The Role of Environment in Radio Galaxies DTSTART;TZID=Asia/Shanghai:20190619T120000 DTEND;TZID=Asia/Shanghai:20190619T130000 LAST-MODIFIED:20190423T140931Z LOCATION:KIAA 1st meeting room SUMMARY:The Role of Environment in Radio Galaxies URL;TYPE=URI:/info/1025/5035.htm END:VEVENT BEGIN:VEVENT UID:4616@kiaa.pku.edu.cn DTSTAMP:20190220T113617Z CREATED:20190220T113617Z DESCRIPTION:Further insights into box/peanut bulge formation DTSTART;TZID=Asia/Shanghai:20190620T160000 DTEND;TZID=Asia/Shanghai:20190620T170000 LAST-MODIFIED:20190220T113617Z LOCATION:KIAA-PKU Auditorium SUMMARY:Further insights into box/peanut bulge formation URL;TYPE=URI:/info/1024/4616.htm END:VEVENT BEGIN:VEVENT UID:5043@kiaa.pku.edu.cn DTSTAMP:20190603T095232Z CREATED:20190603T095232Z DESCRIPTION:The SALT/SAAO Transient Programme in the LSST Era DTSTART;TZID=Asia/Shanghai:20190624T120000 DTEND;TZID=Asia/Shanghai:20190624T130000 LAST-MODIFIED:20190603T095232Z LOCATION:KIAA 1st meeting room SUMMARY:The SALT/SAAO Transient Programme in the LSST Era URL;TYPE=URI:/info/1025/5043.htm END:VEVENT BEGIN:VEVENT UID:5042@kiaa.pku.edu.cn DTSTAMP:20190530T120408Z CREATED:20190530T120408Z DESCRIPTION:Astrophysical applications of star cluster dynamics DTSTART;TZID=Asia/Shanghai:20190625T120000 DTEND;TZID=Asia/Shanghai:20190625T130000 LAST-MODIFIED:20190530T120408Z LOCATION:KIAA 1st meeting room SUMMARY:Astrophysical applications of star cluster dynamics URL;TYPE=URI:/info/1025/5042.htm END:VEVENT BEGIN:VEVENT UID:5045@kiaa.pku.edu.cn DTSTAMP:20190610T150132Z CREATED:20190610T150132Z DESCRIPTION:The optically thick rotating magnetic wind from a massive white dwarf merger product DTSTART;TZID=Asia/Shanghai:20190626T120000 DTEND;TZID=Asia/Shanghai:20190626T130000 LAST-MODIFIED:20190610T150132Z LOCATION:1st meeting room, KIAA SUMMARY:The optically thick rotating magnetic wind from a massive white dwarf merger product URL;TYPE=URI:/info/1025/5045.htm END:VEVENT BEGIN:VEVENT UID:4612@kiaa.pku.edu.cn DTSTAMP:20190318T131939Z CREATED:20190318T131939Z DESCRIPTION:Merger and mass ejection of neutron-star binaries in numerical relativity DTSTART;TZID=Asia/Shanghai:20190627T160000 DTEND;TZID=Asia/Shanghai:20190627T170000 LAST-MODIFIED:20190318T131939Z LOCATION:KIAA-PKU Auditorium SUMMARY:Merger and mass ejection of neutron-star binaries in numerical relativity URL;TYPE=URI:/info/1024/4612.htm END:VEVENT BEGIN:VEVENT UID:5036@kiaa.pku.edu.cn DTSTAMP:20190426T085431Z CREATED:20190426T085431Z DESCRIPTION:Dynamical evidence for a dark substructure in the Milky Way halo DTSTART;TZID=Asia/Shanghai:20190628T120000 DTEND;TZID=Asia/Shanghai:20190628T130000 LAST-MODIFIED:20190426T085431Z LOCATION:KIAA 1st meeting room SUMMARY:Dynamical evidence for a dark substructure in the Milky Way halo URL;TYPE=URI:/info/1025/5036.htm END:VEVENT BEGIN:VEVENT UID:5046@kiaa.pku.edu.cn DTSTAMP:20190611T131220Z CREATED:20190611T131220Z DESCRIPTION:Hadron-quark phase transition in neutron stars DTSTART;TZID=Asia/Shanghai:20190701T120000 DTEND;TZID=Asia/Shanghai:20190701T130000 LAST-MODIFIED:20190611T131220Z LOCATION:DoA, Rm 2907 SUMMARY:Hadron-quark phase transition in neutron stars URL;TYPE=URI:/info/1025/5046.htm END:VEVENT BEGIN:VEVENT UID:5044@kiaa.pku.edu.cn DTSTAMP:20190605T162232Z CREATED:20190605T162232Z DESCRIPTION:Cosmic compass - First tomography of an outer 3D sub-Gauss field via atomic alignment DTSTART;TZID=Asia/Shanghai:20190702T120000 DTEND;TZID=Asia/Shanghai:20190702T130000 LAST-MODIFIED:20190605T162232Z LOCATION:KIAA 1st meeting room SUMMARY:Cosmic compass - First tomography of an outer 3D sub-Gauss field via atomic alignment URL;TYPE=URI:/info/1025/5044.htm END:VEVENT BEGIN:VEVENT UID:4611@kiaa.pku.edu.cn DTSTAMP:20190318T132028Z CREATED:20190318T132028Z DESCRIPTION:Merging Supermassive Black Hole Binaries DTSTART;TZID=Asia/Shanghai:20190704T160000 DTEND;TZID=Asia/Shanghai:20190704T170000 LAST-MODIFIED:20190318T132028Z LOCATION:KIAA-PKU Auditorium SUMMARY:Merging Supermassive Black Hole Binaries URL;TYPE=URI:/info/1024/4611.htm END:VEVENT BEGIN:VEVENT UID:5081@kiaa.pku.edu.cn DTSTAMP:20190612T111837Z CREATED:20190612T111837Z DESCRIPTION:Accretion state transition in active galactic nuclei: observational evidences DTSTART;TZID=Asia/Shanghai:20190705T120000 DTEND;TZID=Asia/Shanghai:20190705T130000 LAST-MODIFIED:20190612T111837Z LOCATION:1st meeting room, KIAA SUMMARY:Accretion state transition in active galactic nuclei: observational evidences URL;TYPE=URI:/info/1025/5081.htm END:VEVENT BEGIN:VEVENT UID:6700@kiaa.pku.edu.cn DTSTAMP:20180905T110929Z CREATED:20180905T110929Z DESCRIPTION:Summer Holiday DTSTART;TZID=Asia/Shanghai:20190708T000000 DTEND;TZID=Asia/Shanghai:20190825T000000 LAST-MODIFIED:20180905T110929Z LOCATION: SUMMARY:Summer Holiday URL;TYPE=URI:/info/1089/6700.htm END:VEVENT BEGIN:VEVENT UID:5080@kiaa.pku.edu.cn DTSTAMP:20190619T102047Z CREATED:20190619T102047Z DESCRIPTION:VVV MICROLENSING EVENTS, CURRENT STATUS AND FUTURE WORK DTSTART;TZID=Asia/Shanghai:20190709T120000 DTEND;TZID=Asia/Shanghai:20190709T130000 LAST-MODIFIED:20190619T102047Z LOCATION:KIAA 1st meeting room SUMMARY:VVV MICROLENSING EVENTS, CURRENT STATUS AND FUTURE WORK URL;TYPE=URI:/info/1025/5080.htm END:VEVENT BEGIN:VEVENT UID:5078@kiaa.pku.edu.cn DTSTAMP:20190625T142347Z CREATED:20190625T142347Z DESCRIPTION:Accretion towards SgrA* SMBH in the Milky Way DTSTART;TZID=Asia/Shanghai:20190712T120000 DTEND;TZID=Asia/Shanghai:20190712T130000 LAST-MODIFIED:20190625T142347Z LOCATION:KIAA 1st meeting room SUMMARY:Accretion towards SgrA* SMBH in the Milky Way URL;TYPE=URI:/info/1025/5078.htm END:VEVENT BEGIN:VEVENT UID:4607@kiaa.pku.edu.cn DTSTAMP:20190531T113507Z CREATED:20190531T113507Z DESCRIPTION:The Breakout of Astrophysical Shocks DTSTART;TZID=Asia/Shanghai:20190712T160000 DTEND;TZID=Asia/Shanghai:20190712T170000 LAST-MODIFIED:20190531T113507Z LOCATION:KIAA 1st Meeting Room SUMMARY:The Breakout of Astrophysical Shocks URL;TYPE=URI:/info/1024/4607.htm END:VEVENT BEGIN:VEVENT UID:5079@kiaa.pku.edu.cn DTSTAMP:20190625T115200Z CREATED:20190625T115200Z DESCRIPTION:Pebble-driven planet formation around stars of different masses DTSTART;TZID=Asia/Shanghai:20190715T120000 DTEND;TZID=Asia/Shanghai:20190715T130000 LAST-MODIFIED:20190625T115200Z LOCATION:KIAA 1st meeting room SUMMARY:Pebble-driven planet formation around stars of different masses URL;TYPE=URI:/info/1025/5079.htm END:VEVENT BEGIN:VEVENT UID:6734@kiaa.pku.edu.cn DTSTAMP:20190712T112211Z CREATED:20190712T112211Z DESCRIPTION:Science Camp DTSTART;TZID=Asia/Shanghai:20190716T133000 DTEND;TZID=Asia/Shanghai:20190716T150000 LAST-MODIFIED:20190712T112211Z LOCATION:KIAA Auditorium SUMMARY:Science Camp URL;TYPE=URI:/info/1089/6734.htm END:VEVENT BEGIN:VEVENT UID:6733@kiaa.pku.edu.cn DTSTAMP:20190712T112320Z CREATED:20190712T112320Z DESCRIPTION:Science Camp DTSTART;TZID=Asia/Shanghai:20190718T133000 DTEND;TZID=Asia/Shanghai:20190718T153000 LAST-MODIFIED:20190712T112320Z LOCATION:KIAA Auditorium SUMMARY:Science Camp URL;TYPE=URI:/info/1089/6733.htm END:VEVENT BEGIN:VEVENT UID:4606@kiaa.pku.edu.cn DTSTAMP:20190725T094809Z CREATED:20190725T094809Z DESCRIPTION:Dark and luminous matter in galaxies (in a new golden age for HI galaxy surveys with the SKA) DTSTART;TZID=Asia/Shanghai:20190801T160000 DTEND;TZID=Asia/Shanghai:20190801T170000 LAST-MODIFIED:20190725T094809Z LOCATION:KIAA-PKU Auditorium SUMMARY:Dark and luminous matter in galaxies (in a new golden age for HI galaxy surveys with the SKA) URL;TYPE=URI:/info/1024/4606.htm END:VEVENT BEGIN:VEVENT UID:5073@kiaa.pku.edu.cn DTSTAMP:20190815T090914Z CREATED:20190815T090914Z DESCRIPTION:Blazar OJ287 and its nano-Hertz GW emitting massive BH binary central engine DTSTART;TZID=Asia/Shanghai:20190822T120000 DTEND;TZID=Asia/Shanghai:20190822T130000 LAST-MODIFIED:20190815T090914Z LOCATION:1st meeting room, KIAA SUMMARY:Blazar OJ287 and its nano-Hertz GW emitting massive BH binary central engine URL;TYPE=URI:/info/1025/5073.htm END:VEVENT BEGIN:VEVENT UID:5074@kiaa.pku.edu.cn DTSTAMP:20190806T152500Z CREATED:20190806T152500Z DESCRIPTION:The mass relations between supermassive Black Holes and their host galaxies at 1<z<2 with HST-WFC3 DTSTART;TZID=Asia/Shanghai:20190823T120000 DTEND;TZID=Asia/Shanghai:20190823T130000 LAST-MODIFIED:20190806T152500Z LOCATION:1st meeting room, KIAA SUMMARY:The mass relations between supermassive Black Holes and their host galaxies at 1<z<2 with HST-WFC3 URL;TYPE=URI:/info/1025/5074.htm END:VEVENT BEGIN:VEVENT UID:5076@kiaa.pku.edu.cn DTSTAMP:20190720T093725Z CREATED:20190720T093725Z DESCRIPTION:Dissecting the Baryon Cycle and Star Formation with Space-based Slitless Spectroscopy DTSTART;TZID=Asia/Shanghai:20190830T120000 DTEND;TZID=Asia/Shanghai:20190830T130000 LAST-MODIFIED:20190720T093725Z LOCATION:1st meeting room, KIAA SUMMARY:Dissecting the Baryon Cycle and Star Formation with Space-based Slitless Spectroscopy URL;TYPE=URI:/info/1025/5076.htm END:VEVENT BEGIN:VEVENT UID:5077@kiaa.pku.edu.cn DTSTAMP:20190705T170547Z CREATED:20190705T170547Z DESCRIPTION:Formation of Galaxy Clusters — from the Core to the Outskirts DTSTART;TZID=Asia/Shanghai:20190904T120000 DTEND;TZID=Asia/Shanghai:20190904T130000 LAST-MODIFIED:20190705T170547Z LOCATION:KIAA 1st Meeting Room SUMMARY:Formation of Galaxy Clusters — from the Core to the Outskirts URL;TYPE=URI:/info/1025/5077.htm END:VEVENT BEGIN:VEVENT UID:5198@kiaa.pku.edu.cn DTSTAMP:20190508T153037Z CREATED:20190508T153037Z DESCRIPTION:KIAA Forum on Gas in Galaxies DTSTART;TZID=Asia/Shanghai:20190909T090000 DTEND;TZID=Asia/Shanghai:20190913T173000 LAST-MODIFIED:20190508T153037Z LOCATION:KIAA Auditorium SUMMARY:KIAA Forum on Gas in Galaxies URL;TYPE=URI:/info/1026/5198.htm END:VEVENT BEGIN:VEVENT UID:6742@kiaa.pku.edu.cn DTSTAMP:20181214T124520Z CREATED:20181214T124520Z DESCRIPTION:Mid-Autumn Festival Holiday DTSTART;TZID=Asia/Shanghai:20190913T000000 DTEND;TZID=Asia/Shanghai:20190913T000000 LAST-MODIFIED:20181214T124520Z LOCATION: SUMMARY:Mid-Autumn Festival Holiday URL;TYPE=URI:/info/1089/6742.htm END:VEVENT BEGIN:VEVENT UID:5070@kiaa.pku.edu.cn DTSTAMP:20190827T232755Z CREATED:20190827T232755Z DESCRIPTION:The Physics of Superluminous Supernovae DTSTART;TZID=Asia/Shanghai:20190917T120000 DTEND;TZID=Asia/Shanghai:20190917T130000 LAST-MODIFIED:20190827T232755Z LOCATION:1st meeting room, KIAA SUMMARY:The Physics of Superluminous Supernovae URL;TYPE=URI:/info/1025/5070.htm END:VEVENT BEGIN:VEVENT UID:5067@kiaa.pku.edu.cn DTSTAMP:20190911T200345Z CREATED:20190911T200345Z DESCRIPTION:Postdoc Defence DTSTART;TZID=Asia/Shanghai:20190919T140000 DTEND;TZID=Asia/Shanghai:20190919T150000 LAST-MODIFIED:20190911T200345Z LOCATION:1st meeting room, KIAA SUMMARY:Postdoc Defence URL;TYPE=URI:/info/1025/5067.htm END:VEVENT BEGIN:VEVENT UID:4602@kiaa.pku.edu.cn DTSTAMP:20190826T092935Z CREATED:20190826T092935Z DESCRIPTION:Mapping the stars, gas and dust in nearby galaxies DTSTART;TZID=Asia/Shanghai:20190919T160000 DTEND;TZID=Asia/Shanghai:20190919T170000 LAST-MODIFIED:20190826T092935Z LOCATION:KIAA-PKU Auditorium SUMMARY:Mapping the stars, gas and dust in nearby galaxies URL;TYPE=URI:/info/1024/4602.htm END:VEVENT BEGIN:VEVENT UID:5068@kiaa.pku.edu.cn DTSTAMP:20190910T114734Z CREATED:20190910T114734Z DESCRIPTION:The multiple eruptions of Eta Carinae DTSTART;TZID=Asia/Shanghai:20190920T120000 DTEND;TZID=Asia/Shanghai:20190920T130000 LAST-MODIFIED:20190910T114734Z LOCATION:KIAA 1st meeting room SUMMARY:The multiple eruptions of Eta Carinae URL;TYPE=URI:/info/1025/5068.htm END:VEVENT BEGIN:VEVENT UID:6731@kiaa.pku.edu.cn DTSTAMP:20190919T114404Z CREATED:20190919T114404Z DESCRIPTION:Undergraduate Research Symposium DTSTART;TZID=Asia/Shanghai:20190920T130000 DTEND;TZID=Asia/Shanghai:20190920T170000 LAST-MODIFIED:20190919T114404Z LOCATION:KIAA Auditorium SUMMARY:Undergraduate Research Symposium URL;TYPE=URI:/info/1089/6731.htm END:VEVENT BEGIN:VEVENT UID:6730@kiaa.pku.edu.cn DTSTAMP:20190919T114637Z CREATED:20190919T114637Z DESCRIPTION:Party to welcome the new students and to celebrate the National Day DTSTART;TZID=Asia/Shanghai:20190920T190000 DTEND;TZID=Asia/Shanghai:20190920T210000 LAST-MODIFIED:20190919T114637Z LOCATION:KIAA Auditorium SUMMARY:Party to welcome the new students and to celebrate the National Day URL;TYPE=URI:/info/1089/6730.htm END:VEVENT BEGIN:VEVENT UID:5072@kiaa.pku.edu.cn DTSTAMP:20190820T085534Z CREATED:20190820T085534Z DESCRIPTION:What is beyond the “visible” galaxy? DTSTART;TZID=Asia/Shanghai:20190924T120000 DTEND;TZID=Asia/Shanghai:20190924T130000 LAST-MODIFIED:20190820T085534Z LOCATION:KIAA 1st meeting room SUMMARY:What is beyond the “visible” galaxy? URL;TYPE=URI:/info/1025/5072.htm END:VEVENT BEGIN:VEVENT UID:4329@kiaa.pku.edu.cn DTSTAMP:20190923T094744Z CREATED:20190923T094744Z DESCRIPTION:Astro-PH DTSTART;TZID=Asia/Shanghai:20190924T133000 DTEND;TZID=Asia/Shanghai:20190924T133000 LAST-MODIFIED:20190923T094744Z LOCATION:Kiaa second floor, common area SUMMARY:Astro-PH URL;TYPE=URI:/info/1027/4329.htm END:VEVENT BEGIN:VEVENT UID:5069@kiaa.pku.edu.cn DTSTAMP:20190902T151247Z CREATED:20190902T151247Z DESCRIPTION:The SkyMapper Southern Survey: data reduction and pipeline DTSTART;TZID=Asia/Shanghai:20190925T120000 DTEND;TZID=Asia/Shanghai:20190925T130000 LAST-MODIFIED:20190902T151247Z LOCATION:KIAA 1st Meeting Room SUMMARY:The SkyMapper Southern Survey: data reduction and pipeline URL;TYPE=URI:/info/1025/5069.htm END:VEVENT BEGIN:VEVENT UID:4603@kiaa.pku.edu.cn DTSTAMP:20190826T093205Z CREATED:20190826T093205Z DESCRIPTION:Formation of massive stellar binaries in the early universe DTSTART;TZID=Asia/Shanghai:20190926T160000 DTEND;TZID=Asia/Shanghai:20190926T170000 LAST-MODIFIED:20190826T093205Z LOCATION:KIAA-PKU Auditorium SUMMARY:Formation of massive stellar binaries in the early universe URL;TYPE=URI:/info/1024/4603.htm END:VEVENT BEGIN:VEVENT UID:5066@kiaa.pku.edu.cn DTSTAMP:20190912T101723Z CREATED:20190912T101723Z DESCRIPTION:A crucial but unexplored chromosphere line for measuring stellar helium abundances DTSTART;TZID=Asia/Shanghai:20190927T120000 DTEND;TZID=Asia/Shanghai:20190927T130000 LAST-MODIFIED:20190912T101723Z LOCATION:1st meeting room, KIAA SUMMARY:A crucial but unexplored chromosphere line for measuring stellar helium abundances URL;TYPE=URI:/info/1025/5066.htm END:VEVENT BEGIN:VEVENT UID:4835@kiaa.pku.edu.cn DTSTAMP:20190925T190047Z CREATED:20190925T190047Z DESCRIPTION:GRAVITY Near-Infrared Interferometry and High Spatial Resolution AGN Science DTSTART;TZID=Asia/Shanghai:20190927T171500 DTEND;TZID=Asia/Shanghai:20190927T181500 LAST-MODIFIED:20190925T190047Z LOCATION:1st Meeting Room, KIAA-PKU SUMMARY:GRAVITY Near-Infrared Interferometry and High Spatial Resolution AGN Science URL;TYPE=URI:/info/1029/4835.htm END:VEVENT BEGIN:VEVENT UID:6741@kiaa.pku.edu.cn DTSTAMP:20181214T124715Z CREATED:20181214T124715Z DESCRIPTION:National Day Holiday DTSTART;TZID=Asia/Shanghai:20190930T000000 DTEND;TZID=Asia/Shanghai:20191006T000000 LAST-MODIFIED:20181214T124715Z LOCATION: SUMMARY:National Day Holiday URL;TYPE=URI:/info/1089/6741.htm END:VEVENT BEGIN:VEVENT UID:4492@kiaa.pku.edu.cn DTSTAMP:20191008T120907Z CREATED:20191008T120907Z DESCRIPTION:Modelling Stellar Populations of Star Clusters DTSTART;TZID=Asia/Shanghai:20191011T150000 DTEND;TZID=Asia/Shanghai:20191011T160000 LAST-MODIFIED:20191008T120907Z LOCATION:KIAA-PKU Auditorium SUMMARY:Modelling Stellar Populations of Star Clusters URL;TYPE=URI:/info/1024/4492.htm END:VEVENT BEGIN:VEVENT UID:5071@kiaa.pku.edu.cn DTSTAMP:20190821T110042Z CREATED:20190821T110042Z DESCRIPTION:A self-consistent constraint on the maximum mass of neutron star according to GW170817 DTSTART;TZID=Asia/Shanghai:20191014T121500 DTEND;TZID=Asia/Shanghai:20191014T131500 LAST-MODIFIED:20190821T110042Z LOCATION:DoA, Rm 2907 SUMMARY:A self-consistent constraint on the maximum mass of neutron star according to GW170817 URL;TYPE=URI:/info/1025/5071.htm END:VEVENT BEGIN:VEVENT UID:5075@kiaa.pku.edu.cn DTSTAMP:20190723T104447Z CREATED:20190723T104447Z DESCRIPTION:Challenge to the Black Hole Model of quasars and Active Galactic Nuclei DTSTART;TZID=Asia/Shanghai:20191015T120000 DTEND;TZID=Asia/Shanghai:20191015T120000 LAST-MODIFIED:20190723T104447Z LOCATION:1st meeting room, KIAA SUMMARY:Challenge to the Black Hole Model of quasars and Active Galactic Nuclei URL;TYPE=URI:/info/1025/5075.htm END:VEVENT BEGIN:VEVENT UID:4604@kiaa.pku.edu.cn DTSTAMP:20190826T093538Z CREATED:20190826T093538Z DESCRIPTION:How to Make High-mass Stars DTSTART;TZID=Asia/Shanghai:20191017T160000 DTEND;TZID=Asia/Shanghai:20191017T170000 LAST-MODIFIED:20190826T093538Z LOCATION:KIAA-PKU Auditorium SUMMARY:How to Make High-mass Stars URL;TYPE=URI:/info/1024/4604.htm END:VEVENT BEGIN:VEVENT UID:5202@kiaa.pku.edu.cn DTSTAMP:20190508T153206Z CREATED:20190508T153206Z DESCRIPTION:Cosmic Evolution of Quasars: from the First Light to Local Relics DTSTART;TZID=Asia/Shanghai:20191021T090000 DTEND;TZID=Asia/Shanghai:20191025T180000 LAST-MODIFIED:20190508T153206Z LOCATION:KIAA Auditorium SUMMARY:Cosmic Evolution of Quasars: from the First Light to Local Relics URL;TYPE=URI:/info/1026/5202.htm END:VEVENT BEGIN:VEVENT UID:5065@kiaa.pku.edu.cn DTSTAMP:20191015T105556Z CREATED:20191015T105556Z DESCRIPTION:Milimeter gap contrast as a probe for turbulence level in protoplanetary disks DTSTART;TZID=Asia/Shanghai:20191028T121500 DTEND;TZID=Asia/Shanghai:20191028T124500 LAST-MODIFIED:20191015T105556Z LOCATION:DoA, Rm 2907 SUMMARY:Milimeter gap contrast as a probe for turbulence level in protoplanetary disks URL;TYPE=URI:/info/1025/5065.htm END:VEVENT BEGIN:VEVENT UID:5048@kiaa.pku.edu.cn DTSTAMP:20191021T143539Z CREATED:20191021T143539Z DESCRIPTION:HI gas and satellites studies using Illustris-TNG DTSTART;TZID=Asia/Shanghai:20191028T123000 DTEND;TZID=Asia/Shanghai:20191028T130000 LAST-MODIFIED:20191021T143539Z LOCATION:DoA, Rm 2907 SUMMARY:HI gas and satellites studies using Illustris-TNG URL;TYPE=URI:/info/1025/5048.htm END:VEVENT BEGIN:VEVENT UID:5200@kiaa.pku.edu.cn DTSTAMP:20191010T093145Z CREATED:20191010T093145Z DESCRIPTION:Faculty Meeting DTSTART;TZID=Asia/Shanghai:20191030T120000 DTEND;TZID=Asia/Shanghai:20191030T120000 LAST-MODIFIED:20191010T093145Z LOCATION: SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1026/5200.htm END:VEVENT BEGIN:VEVENT UID:4493@kiaa.pku.edu.cn DTSTAMP:20191025T090228Z CREATED:20191025T090228Z DESCRIPTION:First binary black hole coalescences DTSTART;TZID=Asia/Shanghai:20191031T160000 DTEND;TZID=Asia/Shanghai:20191031T170000 LAST-MODIFIED:20191025T090228Z LOCATION:KIAA-PKU Auditorium SUMMARY:First binary black hole coalescences URL;TYPE=URI:/info/1024/4493.htm END:VEVENT BEGIN:VEVENT UID:4488@kiaa.pku.edu.cn DTSTAMP:20190826T093646Z CREATED:20190826T093646Z DESCRIPTION:Stochastic particle acceleration in high-energy phenomena DTSTART;TZID=Asia/Shanghai:20191107T160000 DTEND;TZID=Asia/Shanghai:20191107T170000 LAST-MODIFIED:20190826T093646Z LOCATION:KIAA-PKU Auditorium SUMMARY:Stochastic particle acceleration in high-energy phenomena URL;TYPE=URI:/info/1024/4488.htm END:VEVENT BEGIN:VEVENT UID:4489@kiaa.pku.edu.cn DTSTAMP:20190830T140351Z CREATED:20190830T140351Z DESCRIPTION:Multi-wavelength Properties of First Galaxies & Radiative Transfer Simulation of Direct Collapse Scenario DTSTART;TZID=Asia/Shanghai:20191108T150000 DTEND;TZID=Asia/Shanghai:20191108T160000 LAST-MODIFIED:20190830T140351Z LOCATION:KIAA-PKU Auditorium SUMMARY:Multi-wavelength Properties of First Galaxies & Radiative Transfer Simulation of Direct Collapse Scenario URL;TYPE=URI:/info/1024/4489.htm END:VEVENT BEGIN:VEVENT UID:5050@kiaa.pku.edu.cn DTSTAMP:20191103T104425Z CREATED:20191103T104425Z DESCRIPTION:Kelvin-Helmholtz instability in dusty rings of protoplanetary disks DTSTART;TZID=Asia/Shanghai:20191111T121500 DTEND;TZID=Asia/Shanghai:20191111T124500 LAST-MODIFIED:20191103T104425Z LOCATION:DoA, Rm 2907 SUMMARY:Kelvin-Helmholtz instability in dusty rings of protoplanetary disks URL;TYPE=URI:/info/1025/5050.htm END:VEVENT BEGIN:VEVENT UID:4601@kiaa.pku.edu.cn DTSTAMP:20190826T090407Z CREATED:20190826T090407Z DESCRIPTION:Connecting the Bright and Dark Sides of Massive Galaxies DTSTART;TZID=Asia/Shanghai:20191114T160000 DTEND;TZID=Asia/Shanghai:20191114T170000 LAST-MODIFIED:20190826T090407Z LOCATION:KIAA-PKU Auditorium SUMMARY:Connecting the Bright and Dark Sides of Massive Galaxies URL;TYPE=URI:/info/1024/4601.htm END:VEVENT BEGIN:VEVENT UID:5047@kiaa.pku.edu.cn DTSTAMP:20191016T135723Z CREATED:20191016T135723Z DESCRIPTION:Li abundance anomaly in red giants stars and recent efforts to understand DTSTART;TZID=Asia/Shanghai:20191118T121500 DTEND;TZID=Asia/Shanghai:20191118T130000 LAST-MODIFIED:20191016T135723Z LOCATION:DoA, Rm 2907 SUMMARY:Li abundance anomaly in red giants stars and recent efforts to understand URL;TYPE=URI:/info/1025/5047.htm END:VEVENT BEGIN:VEVENT UID:4833@kiaa.pku.edu.cn DTSTAMP:20191225T200536Z CREATED:20191225T200536Z DESCRIPTION:Statistical Properties of Classical and Pseudo Bulges in the Local Universe DTSTART;TZID=Asia/Shanghai:20191122T171500 DTEND;TZID=Asia/Shanghai:20191122T181500 LAST-MODIFIED:20191225T200536Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Statistical Properties of Classical and Pseudo Bulges in the Local Universe URL;TYPE=URI:/info/1029/4833.htm END:VEVENT BEGIN:VEVENT UID:5049@kiaa.pku.edu.cn DTSTAMP:20191029T104903Z CREATED:20191029T104903Z DESCRIPTION:Research on red subdwarfs DTSTART;TZID=Asia/Shanghai:20191125T121500 DTEND;TZID=Asia/Shanghai:20191125T131500 LAST-MODIFIED:20191029T104903Z LOCATION:DoA, Rm 2907 SUMMARY:Research on red subdwarfs URL;TYPE=URI:/info/1025/5049.htm END:VEVENT BEGIN:VEVENT UID:5201@kiaa.pku.edu.cn DTSTAMP:20190919T110404Z CREATED:20190919T110404Z DESCRIPTION:KIAA Forum 2019: The Future of Gravitational Wave Astrophysics DTSTART;TZID=Asia/Shanghai:20191128T083000 DTEND;TZID=Asia/Shanghai:20191129T170000 LAST-MODIFIED:20190919T110404Z LOCATION:KIAA Auditorium SUMMARY:KIAA Forum 2019: The Future of Gravitational Wave Astrophysics URL;TYPE=URI:/info/1026/5201.htm END:VEVENT BEGIN:VEVENT UID:5053@kiaa.pku.edu.cn DTSTAMP:20191113T155759Z CREATED:20191113T155759Z DESCRIPTION:Constraints on Axionlike Particles from gamma ray observations DTSTART;TZID=Asia/Shanghai:20191202T121500 DTEND;TZID=Asia/Shanghai:20191202T130000 LAST-MODIFIED:20191113T155759Z LOCATION:DoA, Rm 2907 SUMMARY:Constraints on Axionlike Particles from gamma ray observations URL;TYPE=URI:/info/1025/5053.htm END:VEVENT BEGIN:VEVENT UID:4495@kiaa.pku.edu.cn DTSTAMP:20191129T162810Z CREATED:20191129T162810Z DESCRIPTION:Consistent Microphysics in Astrophysical Simulations: Why we need it, how we make it, and where we use it DTSTART;TZID=Asia/Shanghai:20191204T160000 DTEND;TZID=Asia/Shanghai:20191204T170000 LAST-MODIFIED:20191129T162810Z LOCATION:KIAA-PKU Auditorium SUMMARY:Consistent Microphysics in Astrophysical Simulations: Why we need it, how we make it, and where we use it URL;TYPE=URI:/info/1024/4495.htm END:VEVENT BEGIN:VEVENT UID:4490@kiaa.pku.edu.cn DTSTAMP:20190903T095432Z CREATED:20190903T095432Z DESCRIPTION:AGN feedback in a galaxy scale DTSTART;TZID=Asia/Shanghai:20191205T150000 DTEND;TZID=Asia/Shanghai:20191205T160000 LAST-MODIFIED:20190903T095432Z LOCATION:KIAA-PKU Auditorium SUMMARY:AGN feedback in a galaxy scale URL;TYPE=URI:/info/1024/4490.htm END:VEVENT BEGIN:VEVENT UID:5052@kiaa.pku.edu.cn DTSTAMP:20191112T162658Z CREATED:20191112T162658Z DESCRIPTION:Globular Cluster Systems in M85, M87, and Virgo DTSTART;TZID=Asia/Shanghai:20191209T121500 DTEND;TZID=Asia/Shanghai:20191209T131500 LAST-MODIFIED:20191112T162658Z LOCATION:DoA, Rm 2907 SUMMARY:Globular Cluster Systems in M85, M87, and Virgo URL;TYPE=URI:/info/1025/5052.htm END:VEVENT BEGIN:VEVENT UID:3908@kiaa.pku.edu.cn DTSTAMP:20191119T095738Z CREATED:20191119T095738Z DESCRIPTION:Postdoc Science Days DTSTART;TZID=Asia/Shanghai:20191210T100000 DTEND;TZID=Asia/Shanghai:20191211T170000 LAST-MODIFIED:20191119T095738Z LOCATION:Auditorium SUMMARY:Postdoc Science Days URL;TYPE=URI:/info/1030/3908.htm END:VEVENT BEGIN:VEVENT UID:4605@kiaa.pku.edu.cn DTSTAMP:20190806T124049Z CREATED:20190806T124049Z DESCRIPTION:The Cosmic Ray-Dominated Circumgalactic Medium DTSTART;TZID=Asia/Shanghai:20191212T160000 DTEND;TZID=Asia/Shanghai:20191212T170000 LAST-MODIFIED:20190806T124049Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Cosmic Ray-Dominated Circumgalactic Medium URL;TYPE=URI:/info/1024/4605.htm END:VEVENT BEGIN:VEVENT UID:5051@kiaa.pku.edu.cn DTSTAMP:20191105T223728Z CREATED:20191105T223728Z DESCRIPTION:Constraining the accretion of Gas-giant planets from observed Hα line DTSTART;TZID=Asia/Shanghai:20191216T121500 DTEND;TZID=Asia/Shanghai:20191216T130000 LAST-MODIFIED:20191105T223728Z LOCATION:DoA, Rm 2907 SUMMARY:Constraining the accretion of Gas-giant planets from observed Hα line URL;TYPE=URI:/info/1025/5051.htm END:VEVENT BEGIN:VEVENT UID:5199@kiaa.pku.edu.cn DTSTAMP:20191111T134712Z CREATED:20191111T134712Z DESCRIPTION:JWST Training Workshop DTSTART;TZID=Asia/Shanghai:20191217T130000 DTEND;TZID=Asia/Shanghai:20191219T120000 LAST-MODIFIED:20191111T134712Z LOCATION: SUMMARY:JWST Training Workshop URL;TYPE=URI:/info/1026/5199.htm END:VEVENT BEGIN:VEVENT UID:4491@kiaa.pku.edu.cn DTSTAMP:20190916T160839Z CREATED:20190916T160839Z DESCRIPTION:Megamasers & AGN, Starburst DTSTART;TZID=Asia/Shanghai:20191219T160000 DTEND;TZID=Asia/Shanghai:20191219T170000 LAST-MODIFIED:20190916T160839Z LOCATION:KIAA-PKU Auditorium SUMMARY:Megamasers & AGN, Starburst URL;TYPE=URI:/info/1024/4491.htm END:VEVENT BEGIN:VEVENT UID:6727@kiaa.pku.edu.cn DTSTAMP:20191216T090012Z CREATED:20191216T090012Z DESCRIPTION:New Year's Eve Party DTSTART;TZID=Asia/Shanghai:20191220T183000 DTEND;TZID=Asia/Shanghai:20191220T203000 LAST-MODIFIED:20191216T090012Z LOCATION:KIAA Auditorium SUMMARY:New Year's Eve Party URL;TYPE=URI:/info/1089/6727.htm END:VEVENT BEGIN:VEVENT UID:5054@kiaa.pku.edu.cn DTSTAMP:20191211T154733Z CREATED:20191211T154733Z DESCRIPTION:Properties of Host Galaxies of Type 2 Quasars & Bar Fractions in IllustrisTNG DTSTART;TZID=Asia/Shanghai:20191223T121500 DTEND;TZID=Asia/Shanghai:20191223T130000 LAST-MODIFIED:20191211T154733Z LOCATION:DoA, Rm 2907 SUMMARY:Properties of Host Galaxies of Type 2 Quasars & Bar Fractions in IllustrisTNG URL;TYPE=URI:/info/1025/5054.htm END:VEVENT BEGIN:VEVENT UID:4756@kiaa.pku.edu.cn DTSTAMP:20191220T001907Z CREATED:20191220T001907Z DESCRIPTION:Star Formation Activities in Dusty Galaxies DTSTART;TZID=Asia/Shanghai:20191224T120000 DTEND;TZID=Asia/Shanghai:20191224T130000 LAST-MODIFIED:20191220T001907Z LOCATION:KIAA-PKU SUMMARY:Star Formation Activities in Dusty Galaxies URL;TYPE=URI:/info/1028/4756.htm END:VEVENT BEGIN:VEVENT UID:4494@kiaa.pku.edu.cn DTSTAMP:20191105T134158Z CREATED:20191105T134158Z DESCRIPTION:How spiral galaxies arise and thrive over cosmic time DTSTART;TZID=Asia/Shanghai:20191226T160000 DTEND;TZID=Asia/Shanghai:20191226T170000 LAST-MODIFIED:20191105T134158Z LOCATION:KIAA-PKU Auditorium SUMMARY:How spiral galaxies arise and thrive over cosmic time URL;TYPE=URI:/info/1024/4494.htm END:VEVENT BEGIN:VEVENT UID:6728@kiaa.pku.edu.cn DTSTAMP:20191206T091411Z CREATED:20191206T091411Z DESCRIPTION:Mid-term defense of Undergraduate Graduation Thesis DTSTART;TZID=Asia/Shanghai:20191227T140000 DTEND;TZID=Asia/Shanghai:20191227T140000 LAST-MODIFIED:20191206T091411Z LOCATION:KIAA-PKU Auditorium SUMMARY:Mid-term defense of Undergraduate Graduation Thesis URL;TYPE=URI:/info/1089/6728.htm END:VEVENT BEGIN:VEVENT UID:4834@kiaa.pku.edu.cn DTSTAMP:20191225T200355Z CREATED:20191225T200355Z DESCRIPTION:Fast radio burst science DTSTART;TZID=Asia/Shanghai:20191227T171500 DTEND;TZID=Asia/Shanghai:20191227T181500 LAST-MODIFIED:20191225T200355Z LOCATION:1st Seminar Room, KIAA-PKU SUMMARY:Fast radio burst science URL;TYPE=URI:/info/1029/4834.htm END:VEVENT BEGIN:VEVENT UID:5055@kiaa.pku.edu.cn DTSTAMP:20191212T151435Z CREATED:20191212T151435Z DESCRIPTION:Cosmological Inference using Gravitational Wave Standard Sirens DTSTART;TZID=Asia/Shanghai:20191230T121500 DTEND;TZID=Asia/Shanghai:20191230T130000 LAST-MODIFIED:20191212T151435Z LOCATION:DoA, Rm 2907 SUMMARY:Cosmological Inference using Gravitational Wave Standard Sirens URL;TYPE=URI:/info/1025/5055.htm END:VEVENT BEGIN:VEVENT UID:4757@kiaa.pku.edu.cn DTSTAMP:20191225T140739Z CREATED:20191225T140739Z DESCRIPTION:Correlation of structure and stellar properties of galaxies DTSTART;TZID=Asia/Shanghai:20191231T120000 DTEND;TZID=Asia/Shanghai:20191231T130000 LAST-MODIFIED:20191225T140739Z LOCATION:KIAA-PKU SUMMARY:Correlation of structure and stellar properties of galaxies URL;TYPE=URI:/info/1028/4757.htm END:VEVENT BEGIN:VEVENT UID:6717@kiaa.pku.edu.cn DTSTAMP:20191225T145837Z CREATED:20191225T145837Z DESCRIPTION:New Year Day Holiday DTSTART;TZID=Asia/Shanghai:20200101T000000 DTEND;TZID=Asia/Shanghai:20200101T000000 LAST-MODIFIED:20191225T145837Z LOCATION: SUMMARY:New Year Day Holiday URL;TYPE=URI:/info/1089/6717.htm END:VEVENT BEGIN:VEVENT UID:6729@kiaa.pku.edu.cn DTSTAMP:20191128T101618Z CREATED:20191128T101618Z DESCRIPTION:Faculty candidate interviews DTSTART;TZID=Asia/Shanghai:20200103T090000 DTEND;TZID=Asia/Shanghai:20200109T170000 LAST-MODIFIED:20191128T101618Z LOCATION: SUMMARY:Faculty candidate interviews URL;TYPE=URI:/info/1089/6729.htm END:VEVENT BEGIN:VEVENT UID:4499@kiaa.pku.edu.cn DTSTAMP:20200102T141353Z CREATED:20200102T141353Z DESCRIPTION:Towards an era of precise and synergistic exoplanetolog DTSTART;TZID=Asia/Shanghai:20200103T100000 DTEND;TZID=Asia/Shanghai:20200103T110000 LAST-MODIFIED:20200102T141353Z LOCATION:KIAA-PKU Auditorium SUMMARY:Towards an era of precise and synergistic exoplanetolog URL;TYPE=URI:/info/1024/4499.htm END:VEVENT BEGIN:VEVENT UID:6718@kiaa.pku.edu.cn DTSTAMP:20200102T165449Z CREATED:20200102T165449Z DESCRIPTION:Lunch discussion with Miao Li DTSTART;TZID=Asia/Shanghai:20200103T120000 DTEND;TZID=Asia/Shanghai:20200103T120000 LAST-MODIFIED:20200102T165449Z LOCATION: SUMMARY:Lunch discussion with Miao Li URL;TYPE=URI:/info/1089/6718.htm END:VEVENT BEGIN:VEVENT UID:6723@kiaa.pku.edu.cn DTSTAMP:20200102T170528Z CREATED:20200102T170528Z DESCRIPTION:Lunch discussion with Fabo Feng DTSTART;TZID=Asia/Shanghai:20200103T120000 DTEND;TZID=Asia/Shanghai:20200103T120000 LAST-MODIFIED:20200102T170528Z LOCATION: SUMMARY:Lunch discussion with Fabo Feng URL;TYPE=URI:/info/1089/6723.htm END:VEVENT BEGIN:VEVENT UID:4498@kiaa.pku.edu.cn DTSTAMP:20200102T141038Z CREATED:20200102T141038Z DESCRIPTION:Probing growth of structure & star-formation history in the Universe DTSTART;TZID=Asia/Shanghai:20200103T150000 DTEND;TZID=Asia/Shanghai:20200103T160000 LAST-MODIFIED:20200102T141038Z LOCATION:KIAA-PKU Auditorium SUMMARY:Probing growth of structure & star-formation history in the Universe URL;TYPE=URI:/info/1024/4498.htm END:VEVENT BEGIN:VEVENT UID:4496@kiaa.pku.edu.cn DTSTAMP:20200102T140608Z CREATED:20200102T140608Z DESCRIPTION:Standing on the shoulders of Kepler DTSTART;TZID=Asia/Shanghai:20200104T100000 DTEND;TZID=Asia/Shanghai:20200104T110000 LAST-MODIFIED:20200102T140608Z LOCATION:KIAA-PKU Auditorium SUMMARY:Standing on the shoulders of Kepler URL;TYPE=URI:/info/1024/4496.htm END:VEVENT BEGIN:VEVENT UID:6719@kiaa.pku.edu.cn DTSTAMP:20200102T170656Z CREATED:20200102T170656Z DESCRIPTION:Lunch discussion with Miao Li DTSTART;TZID=Asia/Shanghai:20200104T120000 DTEND;TZID=Asia/Shanghai:20200104T120000 LAST-MODIFIED:20200102T170656Z LOCATION: SUMMARY:Lunch discussion with Miao Li URL;TYPE=URI:/info/1089/6719.htm END:VEVENT BEGIN:VEVENT UID:6726@kiaa.pku.edu.cn DTSTAMP:20200102T165702Z CREATED:20200102T165702Z DESCRIPTION:Lunch discussion with Haoyi-Wu DTSTART;TZID=Asia/Shanghai:20200104T120000 DTEND;TZID=Asia/Shanghai:20200104T120000 LAST-MODIFIED:20200102T165702Z LOCATION: SUMMARY:Lunch discussion with Haoyi-Wu URL;TYPE=URI:/info/1089/6726.htm END:VEVENT BEGIN:VEVENT UID:4497@kiaa.pku.edu.cn DTSTAMP:20200102T140710Z CREATED:20200102T140710Z DESCRIPTION:The Nature and Impact of Supernovae Feedback in Galaxy Formation DTSTART;TZID=Asia/Shanghai:20200104T150000 DTEND;TZID=Asia/Shanghai:20200104T160000 LAST-MODIFIED:20200102T140710Z LOCATION:KIAA-PKU Auditorium SUMMARY:The Nature and Impact of Supernovae Feedback in Galaxy Formation URL;TYPE=URI:/info/1024/4497.htm END:VEVENT BEGIN:VEVENT UID:6720@kiaa.pku.edu.cn DTSTAMP:20200102T170810Z CREATED:20200102T170810Z DESCRIPTION:Coffee with Haoyi Wu DTSTART;TZID=Asia/Shanghai:20200105T100000 DTEND;TZID=Asia/Shanghai:20200105T100000 LAST-MODIFIED:20200102T170810Z LOCATION: SUMMARY:Coffee with Haoyi Wu URL;TYPE=URI:/info/1089/6720.htm END:VEVENT BEGIN:VEVENT UID:6725@kiaa.pku.edu.cn DTSTAMP:20200102T170002Z CREATED:20200102T170002Z DESCRIPTION:Coffee with Wei Zhu DTSTART;TZID=Asia/Shanghai:20200105T100000 DTEND;TZID=Asia/Shanghai:20200105T100000 LAST-MODIFIED:20200102T170002Z LOCATION: SUMMARY:Coffee with Wei Zhu URL;TYPE=URI:/info/1089/6725.htm END:VEVENT BEGIN:VEVENT UID:6724@kiaa.pku.edu.cn DTSTAMP:20200102T170121Z CREATED:20200102T170121Z DESCRIPTION:Lunch discussion with Fabo Feng DTSTART;TZID=Asia/Shanghai:20200105T100000 DTEND;TZID=Asia/Shanghai:20200105T100000 LAST-MODIFIED:20200102T170121Z LOCATION: SUMMARY:Lunch discussion with Fabo Feng URL;TYPE=URI:/info/1089/6724.htm END:VEVENT BEGIN:VEVENT UID:6721@kiaa.pku.edu.cn DTSTAMP:20200102T170929Z CREATED:20200102T170929Z DESCRIPTION:Lunch discussion with Wei Zhu DTSTART;TZID=Asia/Shanghai:20200105T120000 DTEND;TZID=Asia/Shanghai:20200105T120000 LAST-MODIFIED:20200102T170929Z LOCATION: SUMMARY:Lunch discussion with Wei Zhu URL;TYPE=URI:/info/1089/6721.htm END:VEVENT BEGIN:VEVENT UID:4758@kiaa.pku.edu.cn DTSTAMP:20191227T192629Z CREATED:20191227T192629Z DESCRIPTION:The youngest and more massive Super Stellar Clusters as cosmic laboratories. DTSTART;TZID=Asia/Shanghai:20200107T120000 DTEND;TZID=Asia/Shanghai:20200107T130000 LAST-MODIFIED:20191227T192629Z LOCATION:KIAA-PKU SUMMARY:The youngest and more massive Super Stellar Clusters as cosmic laboratories. URL;TYPE=URI:/info/1028/4758.htm END:VEVENT BEGIN:VEVENT UID:6716@kiaa.pku.edu.cn DTSTAMP:20191225T144946Z CREATED:20191225T144946Z DESCRIPTION:Annual progress report & PhD thesis proposal DTSTART;TZID=Asia/Shanghai:20200109T130000 DTEND;TZID=Asia/Shanghai:20200110T170000 LAST-MODIFIED:20191225T144946Z LOCATION:KIAA 1st meeting room SUMMARY:Annual progress report & PhD thesis proposal URL;TYPE=URI:/info/1089/6716.htm END:VEVENT BEGIN:VEVENT UID:6732@kiaa.pku.edu.cn DTSTAMP:20190902T085558Z CREATED:20190902T085558Z DESCRIPTION:Winter Vacation DTSTART;TZID=Asia/Shanghai:20200113T000000 DTEND;TZID=Asia/Shanghai:20200216T235959 LAST-MODIFIED:20190902T085558Z LOCATION: SUMMARY:Winter Vacation URL;TYPE=URI:/info/1089/6732.htm END:VEVENT BEGIN:VEVENT UID:5056@kiaa.pku.edu.cn DTSTAMP:20191219T110745Z CREATED:20191219T110745Z DESCRIPTION:TeV gamma-rays as a new window onto the physics of gamma-ray bursts and related topics DTSTART;TZID=Asia/Shanghai:20200113T120000 DTEND;TZID=Asia/Shanghai:20200113T124500 LAST-MODIFIED:20191219T110745Z LOCATION:KIAA, 1st meeting room SUMMARY:TeV gamma-rays as a new window onto the physics of gamma-ray bursts and related topics URL;TYPE=URI:/info/1025/5056.htm END:VEVENT BEGIN:VEVENT UID:5064@kiaa.pku.edu.cn DTSTAMP:20200103T140932Z CREATED:20200103T140932Z DESCRIPTION:ALMA tutorial DTSTART;TZID=Asia/Shanghai:20200114T100000 DTEND;TZID=Asia/Shanghai:20200114T160000 LAST-MODIFIED:20200103T140932Z LOCATION:1st meeting room. SUMMARY:ALMA tutorial URL;TYPE=URI:/info/1025/5064.htm END:VEVENT BEGIN:VEVENT UID:4500@kiaa.pku.edu.cn DTSTAMP:20200108T090225Z CREATED:20200108T090225Z DESCRIPTION:How was neutral hydrogen in our Galaxy discovered? DTSTART;TZID=Asia/Shanghai:20200117T160000 DTEND;TZID=Asia/Shanghai:20200117T170000 LAST-MODIFIED:20200108T090225Z LOCATION:KIAA-PKU Auditorium SUMMARY:How was neutral hydrogen in our Galaxy discovered? URL;TYPE=URI:/info/1024/4500.htm END:VEVENT BEGIN:VEVENT UID:5063@kiaa.pku.edu.cn DTSTAMP:20200206T213733Z CREATED:20200206T213733Z DESCRIPTION:Stellar lifetime with different stellar compositions DTSTART;TZID=Asia/Shanghai:20200210T150000 DTEND;TZID=Asia/Shanghai:20200210T153000 LAST-MODIFIED:20200206T213733Z LOCATION:https://zoom.com.cn/j/585325753 SUMMARY:Stellar lifetime with different stellar compositions URL;TYPE=URI:/info/1025/5063.htm END:VEVENT BEGIN:VEVENT UID:5062@kiaa.pku.edu.cn DTSTAMP:20200210T185033Z CREATED:20200210T185033Z DESCRIPTION:On the influence of environment on satellite galaxies in semi-analytic model DTSTART;TZID=Asia/Shanghai:20200217T150000 DTEND;TZID=Asia/Shanghai:20200217T153000 LAST-MODIFIED:20200210T185033Z LOCATION:Join Zoom Meeting https://zoom.com.cn/j/784318949 Meeting ID: 784 318 949 SUMMARY:On the influence of environment on satellite galaxies in semi-analytic model URL;TYPE=URI:/info/1025/5062.htm END:VEVENT BEGIN:VEVENT UID:5061@kiaa.pku.edu.cn DTSTAMP:20200214T103153Z CREATED:20200214T103153Z DESCRIPTION:Hammurabi X: simulating Galactic synchrotron emission with random magnetic fields DTSTART;TZID=Asia/Shanghai:20200224T140000 DTEND;TZID=Asia/Shanghai:20200224T143000 LAST-MODIFIED:20200214T103153Z LOCATION:Join Zoom Meeting https://zoom.com.cn/j/696757317 Meeting ID: 696 757 317 SUMMARY:Hammurabi X: simulating Galactic synchrotron emission with random magnetic fields URL;TYPE=URI:/info/1025/5061.htm END:VEVENT BEGIN:VEVENT UID:5057@kiaa.pku.edu.cn DTSTAMP:20200224T151522Z CREATED:20200224T151522Z DESCRIPTION:Detection of near-core rotations using the pulsations of Kepler gamma Doradus stars DTSTART;TZID=Asia/Shanghai:20200304T140000 DTEND;TZID=Asia/Shanghai:20200304T143000 LAST-MODIFIED:20200224T151522Z LOCATION:Zoom Meeting ID: 230 422 334 SUMMARY:Detection of near-core rotations using the pulsations of Kepler gamma Doradus stars URL;TYPE=URI:/info/1025/5057.htm END:VEVENT BEGIN:VEVENT UID:5059@kiaa.pku.edu.cn DTSTAMP:20200227T152133Z CREATED:20200227T152133Z DESCRIPTION:Southern Pulsar Census and Polarimetric Studies with the MWA DTSTART;TZID=Asia/Shanghai:20200311T140000 DTEND;TZID=Asia/Shanghai:20200311T143000 LAST-MODIFIED:20200227T152133Z LOCATION:Meeting ID: 211 310 579 SUMMARY:Southern Pulsar Census and Polarimetric Studies with the MWA URL;TYPE=URI:/info/1025/5059.htm END:VEVENT BEGIN:VEVENT UID:5058@kiaa.pku.edu.cn DTSTAMP:20200224T152748Z CREATED:20200224T152748Z DESCRIPTION:Molecular Oxygen detected in Mrk231 DTSTART;TZID=Asia/Shanghai:20200318T140000 DTEND;TZID=Asia/Shanghai:20200318T143000 LAST-MODIFIED:20200224T152748Z LOCATION:Zoom Meeting ID: 836 243 760 SUMMARY:Molecular Oxygen detected in Mrk231 URL;TYPE=URI:/info/1025/5058.htm END:VEVENT BEGIN:VEVENT UID:5060@kiaa.pku.edu.cn DTSTAMP:20200317T130204Z CREATED:20200317T130204Z DESCRIPTION:Discovery of two nearby post-T Tauri stellar associations DTSTART;TZID=Asia/Shanghai:20200325T140000 DTEND;TZID=Asia/Shanghai:20200325T143000 LAST-MODIFIED:20200317T130204Z LOCATION:Zoom Meeting ID: 460 656 365 SUMMARY:Discovery of two nearby post-T Tauri stellar associations URL;TYPE=URI:/info/1025/5060.htm END:VEVENT BEGIN:VEVENT UID:6746@kiaa.pku.edu.cn DTSTAMP:20191216T101926Z CREATED:20191216T101926Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20200404T000000 DTEND;TZID=Asia/Shanghai:20200404T000000 LAST-MODIFIED:20191216T101926Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6746.htm END:VEVENT BEGIN:VEVENT UID:6745@kiaa.pku.edu.cn DTSTAMP:20191216T102001Z CREATED:20191216T102001Z DESCRIPTION:Qingming Festival Holiday DTSTART;TZID=Asia/Shanghai:20200406T000000 DTEND;TZID=Asia/Shanghai:20200406T000000 LAST-MODIFIED:20191216T102001Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/6745.htm END:VEVENT BEGIN:VEVENT UID:6744@kiaa.pku.edu.cn DTSTAMP:20200402T152813Z CREATED:20200402T152813Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20200408T140000 DTEND;TZID=Asia/Shanghai:20200408T143000 LAST-MODIFIED:20200402T152813Z LOCATION:zOOM Meeting ID: 473 454 626 SUMMARY:Probing the Cosmic Star-Formation History Revealed by Blind Searches for Far-Infrared Emission Line Galaxies URL;TYPE=URI:/info/1025/6744.htm END:VEVENT BEGIN:VEVENT UID:6839@kiaa.pku.edu.cn DTSTAMP:20200413T152813Z CREATED:20200413T152813Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20200415T140000 DTEND;TZID=Asia/Shanghai:20200415T143000 LAST-MODIFIED:20200413T152813Z LOCATION:Zoom Meeting ID: 909 214 806 SUMMARY:Virtual Observatory: From Idea to Research Mode URL;TYPE=URI:/info/1025/6839.htm END:VEVENT BEGIN:VEVENT UID:6840@kiaa.pku.edu.cn DTSTAMP:20200410T152504Z CREATED:20200410T152504Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20200422T140000 DTEND;TZID=Asia/Shanghai:20200422T143000 LAST-MODIFIED:20200410T152504Z LOCATION:Zoom Meeting ID: 330 287 857 SUMMARY:Fast Radio Burst: From the Source Engine To the Geometry URL;TYPE=URI:/info/1025/6840.htm END:VEVENT BEGIN:VEVENT UID:6953@kiaa.pku.edu.cn DTSTAMP:20200410T121842Z CREATED:20200410T121842Z DESCRIPTION:Planetary nebulae (PNe) are descendants of the low- and intermediate-mass stars (about 1–8 solar masses), which account for the absolute majority (>90%) of stellar populations in the universe.  As an major category of the interstellar media, PNe are one of the few classes of celestial objects that are active in almost every part of the electromagnetic spectrum; they have proven to be ideal lab... DTSTART;TZID=Asia/Shanghai:20200429T140000 DTEND;TZID=Asia/Shanghai:20200429T143000 LAST-MODIFIED:20200410T121842Z LOCATION:ZOOM Meeting ID: 423 427 281 SUMMARY:Planetary Nebulae as Probes of the Stellar and Galactic Evolution URL;TYPE=URI:/info/1025/6953.htm END:VEVENT BEGIN:VEVENT UID:6954@kiaa.pku.edu.cn DTSTAMP:20200409T161842Z CREATED:20200409T161842Z DESCRIPTION: DTSTART;TZID=Asia/Shanghai:20200513T140000 DTEND;TZID=Asia/Shanghai:20200513T143000 LAST-MODIFIED:20200409T161842Z LOCATION:Zoom Meeting ID: 633 6286 4314 SUMMARY:TBD URL;TYPE=URI:/info/1025/6954.htm END:VEVENT BEGIN:VEVENT UID:6952@kiaa.pku.edu.cn DTSTAMP:20200424T183247Z CREATED:20200424T183247Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20200520T140000 DTEND;TZID=Asia/Shanghai:20200520T143000 LAST-MODIFIED:20200424T183247Z LOCATION:Zoom Meeting ID: 646 2952 0793 SUMMARY:TBD URL;TYPE=URI:/info/1025/6952.htm END:VEVENT BEGIN:VEVENT UID:6951@kiaa.pku.edu.cn DTSTAMP:20200428T153243Z CREATED:20200428T153243Z DESCRIPTION:abstract:The inner 500 pc of our Galaxy contains a large amount of dense molecular gas, known as the Central Molecular Zone (CMZ). However, its star formation is observed to be about 10 time less efficient as compared with the prediction from the dense gas star formation relations that are well established toward nearby clouds and external galaxies. This challenges our current understanding of ... DTSTART;TZID=Asia/Shanghai:20200527T140003 DTEND;TZID=Asia/Shanghai:20200527T143003 LAST-MODIFIED:20200428T153243Z LOCATION:Meeting ID: 731 2099 7847, Password: astroPKU SUMMARY:Deciphering Star Formation Enigmas in the Central Molecular Zone URL;TYPE=URI:/info/1025/6951.htm END:VEVENT BEGIN:VEVENT UID:7005@kiaa.pku.edu.cn DTSTAMP:20200610T110429Z CREATED:20200610T110429Z DESCRIPTION:The Milky Way (MW) mass profile is crucial to the Galactic dynamics and many astrophysical studies at various scales. Here we estimate the mass and concentration of the MW halo using the kinematic data of its satellite galaxies, including the latest measurements from Gaia DR2; we also demonstrate how to verify the galaxy formation model in cosmological simulations with observed satellite kinema... DTSTART;TZID=Asia/Shanghai:20200603T140000 DTEND;TZID=Asia/Shanghai:20200603T143000 LAST-MODIFIED:20200610T110429Z LOCATION:Meeting ID: 731 2099 7847, Password: astroPKU SUMMARY:Constraining the Milky Way Mass Profile with Phase-space Distribution of Satellite Galaxies URL;TYPE=URI:/info/1025/7005.htm END:VEVENT BEGIN:VEVENT UID:7006@kiaa.pku.edu.cn DTSTAMP:20200610T153719Z CREATED:20200610T153719Z DESCRIPTION:The binary properties of open clusters place crucial constraints on star formation theory and cluster dynamical evolution. We build a comprehensive Bayesian framework that models the color-magnitude d... DTSTART;TZID=Asia/Shanghai:20200610T140000 DTEND;TZID=Asia/Shanghai:20200610T153000 LAST-MODIFIED:20200610T153719Z LOCATION:zoom Meeting ID: 731 2099 7847. Password: astroPKU SUMMARY:The binary stars in the open cluster NGC3532 and evidence for the dynamical interaction URL;TYPE=URI:/info/1025/7006.htm END:VEVENT BEGIN:VEVENT UID:7007@kiaa.pku.edu.cn DTSTAMP:20200610T153719Z CREATED:20200610T153719Z DESCRIPTION:The speaker will present their latest results which demonstrate that as disc galaxies accumulate more mass, their central stellar mass density increases, bulge type transforms, stellar population ages... DTSTART;TZID=Asia/Shanghai:20200611T140000 DTEND;TZID=Asia/Shanghai:20200611T143000 LAST-MODIFIED:20200610T153719Z LOCATION:Meeting ID: 731 2099 7847, Password: astroPKU SUMMARY:Correlation of bulge transformation in disc galaxies with the gradual decrease in their stellar activity URL;TYPE=URI:/info/1025/7007.htm END:VEVENT BEGIN:VEVENT UID:7008@kiaa.pku.edu.cn DTSTAMP:20200610T153719Z CREATED:20200610T153719Z DESCRIPTION:Abstract:Big bang nucleosynthesis (BBN) is one of the three key pieces of evidence of the hot big bang model, providing a robust tool in order to probe the physics of the early Universe. Theoretical calculations of light element abundances (namely, D,4He, and 7Li) in the standard BBN (SBBN) model are well characterized. In this talk, I will focus on our recent study of non-SBBN models, one mode... DTSTART;TZID=Asia/Shanghai:20200617T140000 DTEND;TZID=Asia/Shanghai:20200617T143000 LAST-MODIFIED:20200610T153719Z LOCATION:Meeting ID: 731 2099 7847， Password: astroPKU SUMMARY:Non-Standard Big Bang Nucleosynthesis URL;TYPE=URI:/info/1025/7008.htm END:VEVENT BEGIN:VEVENT UID:7009@kiaa.pku.edu.cn DTSTAMP:20200610T153719Z CREATED:20200610T153719Z DESCRIPTION:Abstract: Twenty-two decades since Laplace's nebular hypothesis, more than a century after Barnard's revealing dark clouds, nearly 50 years after the ‘great’ discovery of CO, and a full decade of suddenly ubiquitous filaments, star formation as a sub-field of astronomy remains predominantly phenomenological, as evidenced by a glaring lack of predictive theories. For example, the elegant self-... DTSTART;TZID=Asia/Shanghai:20200624T140000 DTEND;TZID=Asia/Shanghai:20200624T150000 LAST-MODIFIED:20200610T153719Z LOCATION:Meeting ID: 731 2099 7847， Password: astroPKU SUMMARY:How to 'Solve' Star Formation ? URL;TYPE=URI:/info/1025/7009.htm END:VEVENT BEGIN:VEVENT UID:7032@kiaa.pku.edu.cn DTSTAMP:20200619T122325Z CREATED:20200619T122325Z DESCRIPTION:Dragon Boat Festival Holida DTSTART;TZID=Asia/Shanghai:20200625T000000 DTEND;TZID=Asia/Shanghai:20200627T000000 LAST-MODIFIED:20200619T122325Z LOCATION: SUMMARY:Dragon Boat Festival Holiday URL;TYPE=URI:/info/1089/7032.htm END:VEVENT BEGIN:VEVENT UID:7010@kiaa.pku.edu.cn DTSTAMP:20200610T153719Z CREATED:20200610T153719Z DESCRIPTION:Abstract:The stellar initial mass distribution function (IMF) is the most crucial assumption when interpreting the astronomy observations of stellar systems. Evidence has shown that the IMF is not universal nor invariant. In this talk, I will introduce the IGIMF theory that explains and predicts the IMF variation as a function of star formation intensity and gas metallicity. The galaxy-wide IMF... DTSTART;TZID=Asia/Shanghai:20200701T140000 DTEND;TZID=Asia/Shanghai:20200701T143000 LAST-MODIFIED:20200610T153719Z LOCATION:Meeting ID: 731 2099 7847, Password: astroPKU SUMMARY:Variable stellar initial mass function and its implications on galaxy chemical evolution URL;TYPE=URI:/info/1025/7010.htm END:VEVENT BEGIN:VEVENT UID:7030@kiaa.pku.edu.cn DTSTAMP:20200619T121728Z CREATED:20200619T121728Z DESCRIPTION:Summer Vacatio DTSTART;TZID=Asia/Shanghai:20200706T000000 DTEND;TZID=Asia/Shanghai:20200830T000000 LAST-MODIFIED:20200619T121728Z LOCATION: SUMMARY:Summer Vacation URL;TYPE=URI:/info/1089/7030.htm END:VEVENT BEGIN:VEVENT UID:7081@kiaa.pku.edu.cn DTSTAMP:20200708T103709Z CREATED:20200708T103709Z DESCRIPTION:Abstract:Based on the MaNGA IFU survey, we have studied the dynamical effects, which is strongly suspected to be led by bars, on the star formation distribution across disks during the quenching of a typical late-type galaxy. Low-luminosity AGN also affects star formation during the passive evolution, not only from that fainter galaxies tend to have higher fraction of AGN, but also from an empi... DTSTART;TZID=Asia/Shanghai:20200708T140009 DTEND;TZID=Asia/Shanghai:20200708T143009 LAST-MODIFIED:20200708T103709Z LOCATION:Meeting ID: 731 2099 7847 Password: astroPKU SUMMARY:Passive Evolution of Nearby Disks--Impact of Dynamical Processes and AGNs URL;TYPE=URI:/info/1025/7081.htm END:VEVENT BEGIN:VEVENT UID:7090@kiaa.pku.edu.cn DTSTAMP:20200711T142747Z CREATED:20200711T142747Z DESCRIPTION:abstract:The joint detection of gravitational wave (GW) and electromagnetic radiation from the binary neutron star merger event GW170817A marks a breakthrough in the field of multi-messenger astronomy. The short gamma-ray burst (sGRB) GRB170817A, associated with this binary neutron star merger event, has an isotropic-equivalent gamma-ray radiation luminosity of 1.6*1047 erg/s, which is much low... DTSTART;TZID=Asia/Shanghai:20200715T140000 DTEND;TZID=Asia/Shanghai:20200715T143000 LAST-MODIFIED:20200711T142747Z LOCATION:Zoom Meeting ID: 731 2099 7847 Password: astroPKU SUMMARY:Study on the jet structure and correlation of short gamma-ray bursts URL;TYPE=URI:/info/1025/7090.htm END:VEVENT BEGIN:VEVENT UID:7110@kiaa.pku.edu.cn DTSTAMP:20200817T185054Z CREATED:20200817T185054Z DESCRIPTION:Abstract:Galaxy mergers are expected to produce multiple supermassive black holes (SMBHs) in close-separation, but the detection of such SMBHs has been difficult. We found a red active galactic nucleus (AGN) of 2MASS J165939.7 + 183436 (1659+1834), as a prospective merging SMBH candidate owing to its merging features in Hubble Space Telescope imaging and double-peaked broad emission lines (BELs... DTSTART;TZID=Asia/Shanghai:20200821T130000 DTEND;TZID=Asia/Shanghai:20200821T133000 LAST-MODIFIED:20200817T185054Z LOCATION:Zoom Meeting ID: 731 2099 7847 Passcode: astroPKU SUMMARY:A merging SMBH candidate found in red active galactic nuclei URL;TYPE=URI:/info/1025/7110.htm END:VEVENT BEGIN:VEVENT UID:7271@kiaa.pku.edu.cn DTSTAMP:20200914T115113Z CREATED:20200914T115113Z DESCRIPTION:Abstract:  Few-body dynamics is an important process that controls the evolution of dense stellar systems such as young star clusters, massive globular clusters (GCs), ultra-compact dwarfs (UCDs) and nuclear star clusters (NSCs). It is also a key process to produce exotic objects including blue stragglers, X-ray binaries and Gravitational wave progenitors. To understand how star clusters and ex... DTSTART;TZID=Asia/Shanghai:20200915T100000 DTEND;TZID=Asia/Shanghai:20200915T110000 LAST-MODIFIED:20200914T115113Z LOCATION:https://zoom.us/j/94933300110 SUMMARY:Few-body problem in dense stellar systems URL;TYPE=URI:/info/1024/7271.htm END:VEVENT BEGIN:VEVENT UID:7280@kiaa.pku.edu.cn DTSTAMP:20200915T114855Z CREATED:20200915T114855Z DESCRIPTION:Abstract:Using kinematical and new structural data of a sample of  27 Giant HII regions (GHIIR) and 103 HII galaxies (HIIG), I explore the relations between their size, surface brightness, ionized gas velocity dispersion,  metallicity, excitation and extinction. I find that the size is well described by the combination of two parameters: the velocity dispersion (σ) and the average surface brig... DTSTART;TZID=Asia/Shanghai:20200924T143000 DTEND;TZID=Asia/Shanghai:20200924T150000 LAST-MODIFIED:20200915T114855Z LOCATION:Zoom Meeting ID: 731 2099 7847 Passcode: astroPKU SUMMARY:Scaling Relations of HIIGs and Estimation of the Star Formation Rate in Type 1 AGNs hosts galaxies using Integral Field Spectroscopy. URL;TYPE=URI:/info/1025/7280.htm END:VEVENT BEGIN:VEVENT UID:7221@kiaa.pku.edu.cn DTSTAMP:20200824T114215Z CREATED:20200824T114215Z DESCRIPTION:2020 PKU Undergraduate Astronomy Symposium Notice No.2 The registration is now open for 2020 PKU Undergraduate Astronomy Symposium. DTSTART;TZID=Asia/Shanghai:20200925T080000 DTEND;TZID=Asia/Shanghai:20200925T180000 LAST-MODIFIED:20200824T114215Z LOCATION:Zoom ID:951 5739 6760 Password:83820367 SUMMARY:2020 PKU Undergraduate Astronomy Symposium URL;TYPE=URI:/info/1026/7221.htm END:VEVENT BEGIN:VEVENT UID:7300@kiaa.pku.edu.cn DTSTAMP:20200925T142343Z CREATED:20200925T142343Z DESCRIPTION:Abstract:Pulsating variable stars such as Cepheid and RR Lyrae are primary standard candles for the extra-galactic distance measurements. One of the most fascinating aims of contemporary variable star research is to strengthen the first-rung of the cosmic distance ladder which allows a precise measurement of the Hubble constant in the late evolutionary Universe. At present, a ~2% local measurem... DTSTART;TZID=Asia/Shanghai:20200930T100000 DTEND;TZID=Asia/Shanghai:20200930T103000 LAST-MODIFIED:20200925T142343Z LOCATION:KIAA 1st meeting room & ZOOM Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Pulsating variable stars as stellar population tracers and distance indicators URL;TYPE=URI:/info/1025/7300.htm END:VEVENT BEGIN:VEVENT UID:6715@kiaa.pku.edu.cn DTSTAMP:20191216T110430Z CREATED:20191216T110430Z DESCRIPTION:National Day Holiday DTSTART;TZID=Asia/Shanghai:20201001T000000 DTEND;TZID=Asia/Shanghai:20201008T000000 LAST-MODIFIED:20191216T110430Z LOCATION: SUMMARY:National Day Holiday URL;TYPE=URI:/info/1089/6715.htm END:VEVENT BEGIN:VEVENT UID:7291@kiaa.pku.edu.cn DTSTAMP:20200923T205037Z CREATED:20200923T205037Z DESCRIPTION:Abstract:Magnetars have magnetic field up to 10^15 G. The ultra-strong magnetic field has profound implications for the mechanical, thermal and radiative evolution of magnetars. In this talk, I will discuss the conversion of magnetic energy to radiations inside and outside magnetars. Inside the magnetar, we studied the interaction between the magnetodynamics and the mechanical responses of the ... DTSTART;TZID=Asia/Shanghai:20201015T100000 DTEND;TZID=Asia/Shanghai:20201015T103000 LAST-MODIFIED:20200923T205037Z LOCATION:KIAA first meeting room + ZOOM Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Magnetodynamics inside and outside magnetars URL;TYPE=URI:/info/1025/7291.htm END:VEVENT BEGIN:VEVENT UID:7290@kiaa.pku.edu.cn DTSTAMP:20200923T173840Z CREATED:20200923T173840Z DESCRIPTION:Abstract: The SAGE survey adopts a unique photometric system, which consists of Stromgren-Crawford (SC) intermediate-band u, self-designed v_SAGE, gri, Hα_n/Hα_w and DDO51. The system is proved to be powerful and sensitive for the study of atmospheric parameters of various types of stars. The parameters, like effective temperature, gravity, and metallicity, yielded from our SAGE system are mo... DTSTART;TZID=Asia/Shanghai:20201022T100000 DTEND;TZID=Asia/Shanghai:20201022T103000 LAST-MODIFIED:20200923T173840Z LOCATION:KIAA first meeting room & ZOOM Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:The progress of the SAGE survey URL;TYPE=URI:/info/1025/7290.htm END:VEVENT BEGIN:VEVENT UID:7330@kiaa.pku.edu.cn DTSTAMP:20201017T153454Z CREATED:20201017T153454Z DESCRIPTION:ABSTRACT:The Five-hundred-meter Aperture Spherical radio Telescope (FAST) has completed its commissioning and begun the Commensal Radio Astronomy FasT Survey (CRAFTS) in 2020. We present predictions for the number of radio-flaring ultracool dwarfs (UCDs) that are likely to be detected by CRAFTS, which will cover $\sim$23,000 deg$^2$ at its completion. Based on the observed flaring UCDs from a n... DTSTART;TZID=Asia/Shanghai:20201029T100000 DTEND;TZID=Asia/Shanghai:20201029T103000 LAST-MODIFIED:20201017T153454Z LOCATION:KIAA first meeting room + ZOOM Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:The potential of detecting radio-flaring ultracool dwarfs at L band in the FAST Drift-Scan Survey URL;TYPE=URI:/info/1025/7330.htm END:VEVENT BEGIN:VEVENT UID:7322@kiaa.pku.edu.cn DTSTAMP:20201010T170339Z CREATED:20201010T170339Z DESCRIPTION:ABSTRACT:Dark sectors consist of new light weakly coupled particles that do not interact with the known Standard Model gauge forces. Searching for dark sector particles, including dark matter itself and other associated states, is a central goal of many experimental programs around the world. The particle physics experiments at the intensity frontier try to explore them using intense particle b... DTSTART;TZID=Asia/Shanghai:20201102T120000 DTEND;TZID=Asia/Shanghai:20201102T125000 LAST-MODIFIED:20201010T170339Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:The quest of dark sectors from the Sun URL;TYPE=URI:/info/1025/7322.htm END:VEVENT BEGIN:VEVENT UID:7340@kiaa.pku.edu.cn DTSTAMP:20201023T093704Z CREATED:20201023T093704Z DESCRIPTION:The Sun is the ultimate source of space weather and the only star that can be observed at a high spatial resolution. With more than 10 advanced solar observatories on the ground and in space, solar physics is now at its golden age. I will introduce two recent advances in observational investigations of the solar atmosphere. (1) Spicules are rapidly evolving fine-scale jets of magnetized plasma ... DTSTART;TZID=Asia/Shanghai:20201105T160000 DTEND;TZID=Asia/Shanghai:20201105T170000 LAST-MODIFIED:20201023T093704Z LOCATION:KIAA Auditorium SUMMARY:Recent advances in observations of solar coronal heating and measurements of the coronal magnetic field URL;TYPE=URI:/info/1024/7340.htm END:VEVENT BEGIN:VEVENT UID:7352@kiaa.pku.edu.cn DTSTAMP:20201101T215125Z CREATED:20201101T215125Z DESCRIPTION:Abstract:Stars spend most of their lifetimes on the main sequence. Extended main-sequence turnoffs and split main sequences seen in the colour-magnitude diagrams of star clusters pose a fundamental challenge to our traditional understanding of star clusters as “single stellar populations.” These features of early-type stars with masses greater than ∼1.6 solar mass is thought to result from a... DTSTART;TZID=Asia/Shanghai:20201109T120000 DTEND;TZID=Asia/Shanghai:20201109T125000 LAST-MODIFIED:20201101T215125Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Stellar rotation: the missing piece in star clusters URL;TYPE=URI:/info/1025/7352.htm END:VEVENT BEGIN:VEVENT UID:7356@kiaa.pku.edu.cn DTSTAMP:20201106T150221Z CREATED:20201106T150221Z DESCRIPTION:The origin of cosmic rays (CRs) is a fundamental problem in astrophysics. Supernova remnants (SNRs) are regarded as the most promising source candidates for the CRs in our Galaxy. However, the recent multi-wavelength  observations reveal that SNRs cannot account for all the Galactic CRs, especially for the ultra high energy band (~ 1PeV). Due to the particle acceleration capacity, young massive... DTSTART;TZID=Asia/Shanghai:20201112T160000 DTEND;TZID=Asia/Shanghai:20201112T170000 LAST-MODIFIED:20201106T150221Z LOCATION:KIAA-Auditorium SUMMARY:Young massive clusters as sources of galactic cosmic rays URL;TYPE=URI:/info/1024/7356.htm END:VEVENT BEGIN:VEVENT UID:7341@kiaa.pku.edu.cn DTSTAMP:20201026T160000Z CREATED:20201026T160000Z DESCRIPTION:With the detection of gravitational waves emitted during black hole and neutron star mergers, LIGO has recently opened the field of gravitational wave astrophysics. In this talk I will review the astrophysical processes that may be responsible for the formation of the observed events. The event rate distribution with mass, spins, eccentricity and redshift may be used to discriminate among diff... DTSTART;TZID=Asia/Shanghai:20201119T160000 DTEND;TZID=Asia/Shanghai:20201119T170000 LAST-MODIFIED:20201026T160000Z LOCATION:KIAA Auditorium Join Zoom Meeting https://zoom.us/j/97001563773?pwd=U3dnaTdaRVYwWHVNWS9Pb1orREtpQT09 Meeting ID: 970 0156 3773 Passcode: 908473 SUMMARY:On the AGN Origin of Gravitational Wave Sources observed by LIGO/VIRGO URL;TYPE=URI:/info/1024/7341.htm END:VEVENT BEGIN:VEVENT UID:7354@kiaa.pku.edu.cn DTSTAMP:20201104T132359Z CREATED:20201104T132359Z DESCRIPTION:Abstract:Hypervelocity stars ( HVSs) are unbound stars escaping the gravitational potential of the Galaxy. HVSs can not only probe the extreme dynamics and physical processes at the Galactic center but also can be used as dynamical traces of integral properties of the Galaxy. Before Gaia data release 2 (DR2) was released, most of the confirmed HVSs were massive early-type O- and B-type stars in... DTSTART;TZID=Asia/Shanghai:20201123T120000 DTEND;TZID=Asia/Shanghai:20201123T123000 LAST-MODIFIED:20201104T132359Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Hypervelocity stars in the Galaxy URL;TYPE=URI:/info/1025/7354.htm END:VEVENT BEGIN:VEVENT UID:7361@kiaa.pku.edu.cn DTSTAMP:20201116T095056Z CREATED:20201116T095056Z DESCRIPTION: KONG DaliGaseous giant planets are a large planetary family. Formed in gas-rich protoplanetary disks, they bear lots of similarities to late-type, convective dwarf stars. However, because of their complicated molecular compositions, unique thermal conditions and fast spinning, gaseous planets have remarkably rich external and internal features, which are connected to a series of fundamental pl... DTSTART;TZID=Asia/Shanghai:20201126T160000 DTEND;TZID=Asia/Shanghai:20201126T170000 LAST-MODIFIED:20201116T095056Z LOCATION:KIAA-Auditorium SUMMARY:New Understandings of Solar System Gaseous Giant Planets in the Era of Juno and Cassini Missions URL;TYPE=URI:/info/1024/7361.htm END:VEVENT BEGIN:VEVENT UID:7360@kiaa.pku.edu.cn DTSTAMP:20201113T142013Z CREATED:20201113T142013Z DESCRIPTION:Abstract:Stacked analyses of galaxy clusters at low-to-intermediate redshift show signatures attributable to dust, but the origin of this dust is uncertain. I will first give an overview of known dust properties, then I will introduce approaches to dust evolution modeling. I applied our models to two contexts: (1) zoom-in cosmological simulations of massive galaxy clusters (10^14 to 10^15 solar... DTSTART;TZID=Asia/Shanghai:20201130T120000 DTEND;TZID=Asia/Shanghai:20201130T125000 LAST-MODIFIED:20201113T142013Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Dust Evolution in Galaxy Clusters at Low to Intermediate Redshift — With Cosmological Simulations and Analytic Methods URL;TYPE=URI:/info/1025/7360.htm END:VEVENT BEGIN:VEVENT UID:7350@kiaa.pku.edu.cn DTSTAMP:20201101T203239Z CREATED:20201101T203239Z DESCRIPTION:Abstract:The 4-meter Multi-Object Spectroscopic Telescope (4MOST) is an upcomping optical spectroscopic instrument which will survey the southern hemisphere. The instrument include both median and high resolution (R~5000 & R~20000) with a broad wavelength coverage. The first light is expected in 2022. In this talk, I will briefly introduce the current status of instrument, selected key science ... DTSTART;TZID=Asia/Shanghai:20201207T120000 DTEND;TZID=Asia/Shanghai:20201207T123000 LAST-MODIFIED:20201101T203239Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:The Upcoming 4MOST Spectroscopy Survey: Current Status, Key Sciences and Operations URL;TYPE=URI:/info/1025/7350.htm END:VEVENT BEGIN:VEVENT UID:7351@kiaa.pku.edu.cn DTSTAMP:20201101T214509Z CREATED:20201101T214509Z DESCRIPTION:Abstract:Our universe is hierarchical. In the bottom-up scenario, smaller structures form larger systems by merging. The hierarchy clustering algorithm can visualize such structures in a clear way. It organizes objects into a hierarchical tree by calculating their pairwise binding energy. This method can effectively identify structures at various levels from substructures to groups and clusters... DTSTART;TZID=Asia/Shanghai:20201214T120000 DTEND;TZID=Asia/Shanghai:20201214T125000 LAST-MODIFIED:20201101T214509Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Visualize the Hierarchical Universe URL;TYPE=URI:/info/1025/7351.htm END:VEVENT BEGIN:VEVENT UID:7390@kiaa.pku.edu.cn DTSTAMP:20201214T095923Z CREATED:20201214T095923Z DESCRIPTION:Feedback from active galactic nuclei (AGNs) at the centers of galaxies is believed to play a major role during galaxy formation and evolution of those galaxies and central black holes (BHs). However, in many popular treatments of AGN feedback model some of the most basic requirements, such as the necessity that mass and momentum be conserved have not been imposed, and the inclusion of the prese... DTSTART;TZID=Asia/Shanghai:20201217T160000 DTEND;TZID=Asia/Shanghai:20201217T170000 LAST-MODIFIED:20201214T095923Z LOCATION:（Remote Talk） PKU KIAA is inviting you to a scheduled Zoom meeting. Topic: PKU KIAA's Zoom Coloquium by Ena Choi Time: Dec 17, 2020 04:00 PM Beijing, Shanghai Join Zoom Meeting https://zoom.us/j/92584562558?pwd=VTA1NWhiSXdMNU41bHhuejhmWjlmUT09 Meeting ID: 925 8456 2558 Passcode: 141399 One tap mobile +16468769923,,92584562558#,,,,,,0#,,141399# US (New York) +16699006833,,92584562558#,,,,,,0#,,141399# US (San Jose) Dial by your location +1 646 876 9923 US (New York) +1 669 900 6833 US (San Jose) +1 253 215 8782 US (Tacoma) +1 301 715 8592 US (Washington D.C) +1 312 626 6799 US (Chicago) +1 346 248 7799 US (Houston) Meeting ID: 925 8456 2558 Passcode: 141399 Find your local number: https://zoom.us/u/acKprKScWw SUMMARY:Two phase formation of massive elliptical galaxies: the role of AGN feedback URL;TYPE=URI:/info/1024/7390.htm END:VEVENT BEGIN:VEVENT UID:7362@kiaa.pku.edu.cn DTSTAMP:20201118T172659Z CREATED:20201118T172659Z DESCRIPTION:Abstract:Exoplanets that exhibit ongoing accretion activities are excellent targets to probe the ground truth of planet formation. The accretion-induced excess emission enables a constraint on the mass accretion rate, a critical characteristic that regulates planet formation and determines the planet's ultimate mass. Based on theoretical studies, planetary accretion creates a hot shock front th... DTSTART;TZID=Asia/Shanghai:20201221T120000 DTEND;TZID=Asia/Shanghai:20201221T125000 LAST-MODIFIED:20201118T172659Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:The First Direct-Imaging Detection of an Exoplanet in Ultraviolet URL;TYPE=URI:/info/1025/7362.htm END:VEVENT BEGIN:VEVENT UID:7363@kiaa.pku.edu.cn DTSTAMP:20201118T180051Z CREATED:20201118T180051Z DESCRIPTION:Abstract:Turbulence is ubiquitous in the universe across a vast range of length scales and actively participates in diverse astrophysical processes, such as star formation, cosmic ray diffusion, dynamo amplification of cosmic magnetic fields, magnetic reconnection in high-energy astrophysical environments. Despite their scientific significance, direct measurements of turbulence in most astrophy... DTSTART;TZID=Asia/Shanghai:20201228T120000 DTEND;TZID=Asia/Shanghai:20201228T123000 LAST-MODIFIED:20201118T180051Z LOCATION:KIAA first meeting room + zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Statistical measurements of astrophysical turbulence URL;TYPE=URI:/info/1025/7363.htm END:VEVENT BEGIN:VEVENT UID:7401@kiaa.pku.edu.cn DTSTAMP:20201228T102459Z CREATED:20201228T102459Z DESCRIPTION:Imaging nearby supermassive black holes and their immediate neighborhoods provides a new astrophysical laboratory to test general relativity in a strong gravitational field regime and probe the physical processes of mass accretion and jet genesis on event horizon scales. Very Long Baseline Interferometry at millimeter wavelengths offers the highest spatial resolution achievable in astronomy. In... DTSTART;TZID=Asia/Shanghai:20201231T160000 DTEND;TZID=Asia/Shanghai:20201231T170000 LAST-MODIFIED:20201228T102459Z LOCATION:Remote Talk SUMMARY:Imaging nearby supermassive black holes and their immediate neighborhoods with millimeter-VLBI URL;TYPE=URI:/info/1024/7401.htm END:VEVENT BEGIN:VEVENT UID:7400@kiaa.pku.edu.cn DTSTAMP:20201225T085013Z CREATED:20201225T085013Z DESCRIPTION:New Year's Day Holida DTSTART;TZID=Asia/Shanghai:20210101T000000 DTEND;TZID=Asia/Shanghai:20210103T000000 LAST-MODIFIED:20201225T085013Z LOCATION: SUMMARY:New Year's Day Holiday URL;TYPE=URI:/info/1089/7400.htm END:VEVENT BEGIN:VEVENT UID:7419@kiaa.pku.edu.cn DTSTAMP:20201231T143646Z CREATED:20201231T143646Z DESCRIPTION:BHOLE Annual Meetin DTSTART;TZID=Asia/Shanghai:20210104T083000 DTEND;TZID=Asia/Shanghai:20210104T163000 LAST-MODIFIED:20201231T143646Z LOCATION:Zoom SUMMARY:BHOLE Annual Meeting URL;TYPE=URI:/info/1026/7419.htm END:VEVENT BEGIN:VEVENT UID:7394@kiaa.pku.edu.cn DTSTAMP:20201216T124243Z CREATED:20201216T124243Z DESCRIPTION:Abstract:Particle physics research can significantly deepen people's understanding about the elementary building blocks and fundamental laws of nature. The Standard Model of particle physics provides the foundation of modern high energy physics. However, the Standard Model fails miserably in several aspects. First, it has no dark matter candidate. Further, there are a few super tiny parameters,... DTSTART;TZID=Asia/Shanghai:20210104T120000 DTEND;TZID=Asia/Shanghai:20210104T125500 LAST-MODIFIED:20201216T124243Z LOCATION:zoom Meeting ID: 731 2099 7847 (Passcode: astroPKU) SUMMARY:Astrophysical Probes to New Physics Beyond the Standard Model URL;TYPE=URI:/info/1025/7394.htm END:VEVENT BEGIN:VEVENT UID:7402@kiaa.pku.edu.cn DTSTAMP:20201229T145907Z CREATED:20201229T145907Z DESCRIPTION:Faculty Intervie DTSTART;TZID=Asia/Shanghai:20210111T000000 DTEND;TZID=Asia/Shanghai:20210115T000000 LAST-MODIFIED:20201229T145907Z LOCATION: SUMMARY:Faculty Interview URL;TYPE=URI:/info/1089/7402.htm END:VEVENT BEGIN:VEVENT UID:7418@kiaa.pku.edu.cn DTSTAMP:20201231T143256Z CREATED:20201231T143256Z DESCRIPTION:Annual reports and PhD qualification exam of 202 DTSTART;TZID=Asia/Shanghai:20210118T083000 DTEND;TZID=Asia/Shanghai:20210119T173000 LAST-MODIFIED:20201231T143256Z LOCATION: SUMMARY:Annual reports and PhD qualification exam of 2020 URL;TYPE=URI:/info/1026/7418.htm END:VEVENT BEGIN:VEVENT UID:7473@kiaa.pku.edu.cn DTSTAMP:20210115T085851Z CREATED:20210115T085851Z DESCRIPTION:Postdoc final defense tal DTSTART;TZID=Asia/Shanghai:20210120T140000 DTEND;TZID=Asia/Shanghai:20210120T150000 LAST-MODIFIED:20210115T085851Z LOCATION: SUMMARY:Postdoc final defense talk URL;TYPE=URI:/info/1024/7473.htm END:VEVENT BEGIN:VEVENT UID:7403@kiaa.pku.edu.cn DTSTAMP:20201229T150113Z CREATED:20201229T150113Z DESCRIPTION:Faculty Meetin DTSTART;TZID=Asia/Shanghai:20210121T100000 DTEND;TZID=Asia/Shanghai:20210121T120000 LAST-MODIFIED:20201229T150113Z LOCATION: SUMMARY:Faculty Meeting URL;TYPE=URI:/info/1089/7403.htm END:VEVENT BEGIN:VEVENT UID:7472@kiaa.pku.edu.cn DTSTAMP:20210115T085456Z CREATED:20210115T085456Z DESCRIPTION:Abstract:Many transient phenomena are the deaths of massive short-lived stars. All else being equal, the  physical properties of the galaxies in which these events occur  should match those of the typical galaxy population weighted by  star-formation rate. Of  particular interest is metallicity, the ratio of elements heaver  than helium to that of hydrogen. In prior work I showed that while the... DTSTART;TZID=Asia/Shanghai:20210121T123000 DTEND;TZID=Asia/Shanghai:20210121T133000 LAST-MODIFIED:20210115T085456Z LOCATION: SUMMARY:Studying Transients Through the Metallicity Distributions of Their Host Galaxies URL;TYPE=URI:/info/1025/7472.htm END:VEVENT BEGIN:VEVENT UID:7031@kiaa.pku.edu.cn DTSTAMP:20200619T122219Z CREATED:20200619T122219Z DESCRIPTION:Winter Vacatio DTSTART;TZID=Asia/Shanghai:20210125T000000 DTEND;TZID=Asia/Shanghai:20210228T000000 LAST-MODIFIED:20200619T122219Z LOCATION: SUMMARY:Winter Vacation URL;TYPE=URI:/info/1089/7031.htm END:VEVENT BEGIN:VEVENT UID:7490@kiaa.pku.edu.cn DTSTAMP:20210126T155433Z CREATED:20210126T155433Z DESCRIPTION:Abstract: Astrophysical stellar objects produce various energetic transients. For example, neutron star mergers produce short-duration gamma-ray bursts, core-collapse of normal stars produce supernovae, and core-collapse of massive metal-poor stars may produce long-duration gamma-ray bursts. Their different origins make their galactic and sub-galactic environments different. Neutron star merge... DTSTART;TZID=Asia/Shanghai:20210127T100000 DTEND;TZID=Asia/Shanghai:20210127T110000 LAST-MODIFIED:20210126T155433Z LOCATION:Zoom Meeting: https://us02web.zoom.us/j/81784731046?pwd=WnM3Z0N0ckF5RjdTMmQyeGNlUGNodz09 Meeting ID: 817 8473 1046 Passcode: KIAApku SUMMARY:Stellar transients and their host galaxies URL;TYPE=URI:/info/1025/7490.htm END:VEVENT BEGIN:VEVENT UID:7491@kiaa.pku.edu.cn DTSTAMP:20210126T155707Z CREATED:20210126T155707Z DESCRIPTION:Abstract: In this talk, I will discuss the effects of magnetic and gravitomagnetic fields in some astrophysical contexts. Considering an uniform magnetic field in the Minkowski background, I will first discuss how the propagation of gravitational wave (GW) and GW bursts are affected by the magnetic field. This formulation may be extended for non-uniform magnetic fields and in curved background... DTSTART;TZID=Asia/Shanghai:20210129T133000 DTEND;TZID=Asia/Shanghai:20210129T143000 LAST-MODIFIED:20210126T155707Z LOCATION:Zoom Meeting: https://us02web.zoom.us/j/88654583207?pwd=T2Q4SjFTMGdvam40WnIyc1g1MzFtUT09 Meeting ID: 886 5458 3207 Passcode: 281949 SUMMARY:Effects of magnetic and gravitomagnetic fields in some astrophysical contexts URL;TYPE=URI:/info/1025/7491.htm END:VEVENT BEGIN:VEVENT UID:7531@kiaa.pku.edu.cn DTSTAMP:20210302T134558Z CREATED:20210302T134558Z DESCRIPTION:Abstract: Cosmological simulations predict that galaxies form in groups and filaments where the interplay between the cold gas flowing inside galaxies and outflowing winds play a key role in growth of galaxies with time. While this picture clearly emerges from simulations, observations of this baryon cycle remain scarce. In the first part of the talk I will discuss our efforts to underst... DTSTART;TZID=Asia/Shanghai:20210305T140000 DTEND;TZID=Asia/Shanghai:20210305T150000 LAST-MODIFIED:20210302T134558Z LOCATION:Zoom meeting ID: 852 9446 3987 Passcode: 195396 SUMMARY:Tracing gas flows in and around galaxies URL;TYPE=URI:/info/1025/7531.htm END:VEVENT BEGIN:VEVENT UID:7422@kiaa.pku.edu.cn DTSTAMP:20210108T162639Z CREATED:20210108T162639Z DESCRIPTION:Abstract:Herschel observations revealed omnipresent filamentary structures in Galactic star-forming clouds. Although these filaments are often identified with flowing gas that could aid the star formation, a direct implication of it might be identifying a correlation between the protostellar accretion and gas flow along the filaments. However, it is difficult to have a direct detection of ... DTSTART;TZID=Asia/Shanghai:20210308T120000 DTEND;TZID=Asia/Shanghai:20210308T125000 LAST-MODIFIED:20210108T162639Z LOCATION:Zoom ID: 833 5168 6763 , passcode: astroPKU SUMMARY:Role of filaments and outflows in star formation URL;TYPE=URI:/info/1025/7422.htm END:VEVENT BEGIN:VEVENT UID:7532@kiaa.pku.edu.cn DTSTAMP:20210305T165302Z CREATED:20210305T165302Z DESCRIPTION:AbstractThe Milky Way (MW) is a good laboratory to test galaxy formation and evolution scenarios with the advantage that the individual stars in the MW can be resolved. A number of completed or ongoing large-scale spectroscopic surveys (e.g., LAMOST, APOGEE) have propelled studies of the structure, stellar populations and the chemical and dynamic evolution of the Milky Way.  In the first part o... DTSTART;TZID=Asia/Shanghai:20210309T140000 DTEND;TZID=Asia/Shanghai:20210309T160000 LAST-MODIFIED:20210305T165302Z LOCATION:K208 SUMMARY:The chemical and dynamical evolution study of the Galactic disc based on the LAMOST spectroscopic survey data URL;TYPE=URI:/info/1025/7532.htm END:VEVENT BEGIN:VEVENT UID:7481@kiaa.pku.edu.cn DTSTAMP:20210120T165925Z CREATED:20210120T165925Z DESCRIPTION:Abstract:The molecular gas mass is the fundamental parameter to understand star formation processes in galaxies. The emission line from carbon monoxide (CO) has been used as the traditional method to measure molecular gas mass in galaxies. Recently, the modern method using the atomic carbon emission line ([CI]) has been proposed in order to estimate the molecular gas mass in high-z galaxies. In... DTSTART;TZID=Asia/Shanghai:20210315T121500 DTEND;TZID=Asia/Shanghai:20210315T124500 LAST-MODIFIED:20210120T165925Z LOCATION:Zoom ID: 833 5168 6763 , passcode: astroPKU SUMMARY:ALMA Observations of Atomic Carbon in Nearby Active Galaxies and Nobeyama 45-m Observations of Carbon Monoxide in Type 1 AGNs URL;TYPE=URI:/info/1025/7481.htm END:VEVENT BEGIN:VEVENT UID:7534@kiaa.pku.edu.cn DTSTAMP:20210308T110542Z CREATED:20210308T110542Z DESCRIPTION:Polarimetry in the X-ray band is argued to be a powerful and sometimes unique tool in diagnosing the magnetic field, geometry and emission mechanism in astrophysics. PolarLight, which is a miniature X-ray polarimeter onboard a CubeSat, is the first dedicated astronomical X-ray polarimeter since the OSO-8 experiment in 1970s. It was launched into a low-Earth orbit in October 2018 and is still wo... DTSTART;TZID=Asia/Shanghai:20210318T160000 DTEND;TZID=Asia/Shanghai:20210318T170000 LAST-MODIFIED:20210308T110542Z LOCATION:KIAA-auditorium SUMMARY:Reopening the window of astronomical X-ray polarimetry with PolarLight URL;TYPE=URI:/info/1024/7534.htm END:VEVENT BEGIN:VEVENT UID:7530@kiaa.pku.edu.cn DTSTAMP:20210225T175023Z CREATED:20210225T175023Z DESCRIPTION:Abstract:Data from the Gaia satellite are revolutionizing many fields of astronomy. I will present two discoveries about white dwarfs: one is an extreme cooling anomaly that produces a mysterious branch on the HR diagram, and the other is the existence of merger products among white dwarfs. The former poses a challenge for our understanding of white dwarf physics, and the latter has implication... DTSTART;TZID=Asia/Shanghai:20210322T120000 DTEND;TZID=Asia/Shanghai:20210322T125000 LAST-MODIFIED:20210225T175023Z LOCATION:Zoom ID: 833 5168 6763 , passcode: astroPKU SUMMARY:New populations of white dwarfs revealed by Gaia URL;TYPE=URI:/info/1025/7530.htm END:VEVENT BEGIN:VEVENT UID:7551@kiaa.pku.edu.cn DTSTAMP:20210311T091835Z CREATED:20210311T091835Z DESCRIPTION:In the standard structure formation paradigm of LambdaCDM, galaxies form at the centers of dark matter halos. Smaller galaxies and their host halos can merge with larger halos, becoming the so-called satellite galaxies and subhalos. Orbiting around the central dominant galaxy of the host halo and undergoing tidal stripping, these satellites and subhalos lose mass, which form stellar streams and... DTSTART;TZID=Asia/Shanghai:20210325T160000 DTEND;TZID=Asia/Shanghai:20210325T170000 LAST-MODIFIED:20210311T091835Z LOCATION:KIAA-auditorium SUMMARY:Studies on low-mass satellite galaxies and faint diffuse stellar halos of isolated central galaxies URL;TYPE=URI:/info/1024/7551.htm END:VEVENT BEGIN:VEVENT UID:7553@kiaa.pku.edu.cn DTSTAMP:20210315T164128Z CREATED:20210315T164128Z DESCRIPTION:abstract:Up to now LIGO-Virgo-KAGRA collaboration has detected dozens of gravitational wave events, all are mergers of binary black holes or neutron stars. Yet, the detectors are sensitive to more sources from hypothesis, thus enabling us to look for new physics. In this talk I will describe a recent work where we searched for evidence of gravitational waves from sub-solar mass compact binary c... DTSTART;TZID=Asia/Shanghai:20210330T133000 DTEND;TZID=Asia/Shanghai:20210330T143000 LAST-MODIFIED:20210315T164128Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Looking for sub-solar mass black hole merger with LIGO and Virgo URL;TYPE=URI:/info/1025/7553.htm END:VEVENT BEGIN:VEVENT UID:7535@kiaa.pku.edu.cn DTSTAMP:20210310T094858Z CREATED:20210310T094858Z DESCRIPTION:I will give a comprehensive overview of the international mega-science project SKA, it's status, progress, and the involvement and activities of the Chinese community. DTSTART;TZID=Asia/Shanghai:20210401T160000 DTEND;TZID=Asia/Shanghai:20210401T170000 LAST-MODIFIED:20210310T094858Z LOCATION:KIAA-auditorium SUMMARY:The Square Kilometer Array: Progress and the Chinese Participation URL;TYPE=URI:/info/1024/7535.htm END:VEVENT BEGIN:VEVENT UID:7585@kiaa.pku.edu.cn DTSTAMP:20210402T085438Z CREATED:20210402T085438Z DESCRIPTION:Qingming Festival Holida DTSTART;TZID=Asia/Shanghai:20210403T000000 DTEND;TZID=Asia/Shanghai:20210405T000000 LAST-MODIFIED:20210402T085438Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/7585.htm END:VEVENT BEGIN:VEVENT UID:7580@kiaa.pku.edu.cn DTSTAMP:20210329T193900Z CREATED:20210329T193900Z DESCRIPTION:abstract:Lorentz invariance is considered as one of the fundamental symmetries in the laws of physics. However, many candidates of quantum gravity suggest the breaking of Lorentz invariance at the Planck energy scale. Numerous astrophysical observations and terrestrial experiments have been used to test the possibility of Lorentz-invariance violation with no positive evidence discovered. The su... DTSTART;TZID=Asia/Shanghai:20210406T133000 DTEND;TZID=Asia/Shanghai:20210406T143000 LAST-MODIFIED:20210329T193900Z LOCATION:KIAA first meeting room + zoom SUMMARY:Signatures in pulsar and continuous gravitational wave observations due to Lorentz-invariance violation URL;TYPE=URI:/info/1025/7580.htm END:VEVENT BEGIN:VEVENT UID:7536@kiaa.pku.edu.cn DTSTAMP:20210310T100439Z CREATED:20210310T100439Z DESCRIPTION:Turbulent motions in the intracluster medium (ICM) area key piece of puzzle in the astrophysics and cosmology of galaxy clusters. A series of recent studies have demonstrated the importance of density stratification in the evolution of ICM turbulent motions. The buoyancy effect induced by ICM density stratification introduces qualitative changes to the turbulence morphology, and opens up a new ... DTSTART;TZID=Asia/Shanghai:20210408T160000 DTEND;TZID=Asia/Shanghai:20210408T170000 LAST-MODIFIED:20210310T100439Z LOCATION:KIAA-auditorium SUMMARY:The Intracluster 'Stratosphere': Dynamics and Thermodynamics URL;TYPE=URI:/info/1024/7536.htm END:VEVENT BEGIN:VEVENT UID:7571@kiaa.pku.edu.cn DTSTAMP:20210321T174332Z CREATED:20210321T174332Z DESCRIPTION:abstract:Red supergiant is a critical evolutionary phase of massive stars, with high luminosity, low effective temperature, strong mass-loss, and fabulous ending as Type IIP supernova. I will present an investigation of evolved massive stars in the Magellanic Clouds, in particular of the red supergiant stars (RSGs). Two large, clean, magnitude-limited multiwavelength source catalogs for the LMC... DTSTART;TZID=Asia/Shanghai:20210413T133000 DTEND;TZID=Asia/Shanghai:20210413T143000 LAST-MODIFIED:20210321T174332Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Red Supergiant Stars in the Magellanic Clouds URL;TYPE=URI:/info/1025/7571.htm END:VEVENT BEGIN:VEVENT UID:7537@kiaa.pku.edu.cn DTSTAMP:20210311T100000Z CREATED:20210311T100000Z DESCRIPTION:Star formation is among the most complex processes studied by astronomers to date. It is characterised by a multi-scale interplay between gravity, turbulence, magnetic field, galactic shear as well as ironising radiation. The key to understand star formation is to pin down the physical mechanics at work. I focus on the followings:-- the interaction between galactic disk and molecular cloud, thr... DTSTART;TZID=Asia/Shanghai:20210415T160000 DTEND;TZID=Asia/Shanghai:20210415T170000 LAST-MODIFIED:20210311T100000Z LOCATION:KIAA-auditorium SUMMARY:Star formation — Are complex things understandable? URL;TYPE=URI:/info/1024/7537.htm END:VEVENT BEGIN:VEVENT UID:7572@kiaa.pku.edu.cn DTSTAMP:20210321T174832Z CREATED:20210321T174832Z DESCRIPTION:abstractThe aim of this paper is to establish a complete sample of red supergiants (RSGs) in M31 and M33. The member stars of the two galaxies are selected from the near-infrared (NIR) point sources after removing the foreground dwarfs from their obvious branch in the J−H/H−K diagram with the archival photometric data taken by the UKIRT/WFCAM. This separation by NIR colors of dwarfs from gian... DTSTART;TZID=Asia/Shanghai:20210420T133000 DTEND;TZID=Asia/Shanghai:20210420T135500 LAST-MODIFIED:20210321T174832Z LOCATION:KIAA first meeting room + zoom SUMMARY:Red Supergiants in M31 and M33. I. The Complete Sample URL;TYPE=URI:/info/1025/7572.htm END:VEVENT BEGIN:VEVENT UID:7573@kiaa.pku.edu.cn DTSTAMP:20210321T175046Z CREATED:20210321T175046Z DESCRIPTION:abstract:Mass loss is an important activity for red supergiants (RSGs) and can influence their evolution and final fate. Previous estimations of mass-loss rates (MLRs) of RSGs exhibit significant dispersion due to differences in method and the incompleteness of samples. With the improved quality and depth of surveys including the UKIRT/WFCAM observations in the near-infrared, and LGGS and PS1 i... DTSTART;TZID=Asia/Shanghai:20210420T135500 DTEND;TZID=Asia/Shanghai:20210420T143000 LAST-MODIFIED:20210321T175046Z LOCATION:KIAA first meeting room + zoom SUMMARY:Mass Loss Rate of Red Supergiants in M31 and M33 URL;TYPE=URI:/info/1025/7573.htm END:VEVENT BEGIN:VEVENT UID:7538@kiaa.pku.edu.cn DTSTAMP:20210310T110955Z CREATED:20210310T110955Z DESCRIPTION:Lithium (Li) has confused scientists for decades at almost every scale of the universe. One percent of low-mass evolved stars have anomalously high Li abundances in their atmospheres, conflicting directly with the prediction of standard stellar evolution models. This finding makes the production and evolution of Li in the Universe more intriguing, not only in the sense of Big Bang nucleosynthes... DTSTART;TZID=Asia/Shanghai:20210422T160000 DTEND;TZID=Asia/Shanghai:20210422T170000 LAST-MODIFIED:20210310T110955Z LOCATION:KIAA-auditorium SUMMARY:New Insights into the Lithium-rich Low-mass Evolved Stars URL;TYPE=URI:/info/1024/7538.htm END:VEVENT BEGIN:VEVENT UID:7570@kiaa.pku.edu.cn DTSTAMP:20210318T120631Z CREATED:20210318T120631Z DESCRIPTION:Abstract:The origin of chemically peculiar stars and non-zero eccentricity in evolved close binaries have been long-standing problems in binary stellar evolution. Answers to these questions may trace back to an intense mass transfer during an AGB binary phase. In this talk, I will discuss two mass transfer modes in the AGB binaries and the transition between them. One mass transfer mode is the ... DTSTART;TZID=Asia/Shanghai:20210427T133000 DTEND;TZID=Asia/Shanghai:20210427T143000 LAST-MODIFIED:20210318T120631Z LOCATION:KIAA first meeting room + ZOOM SUMMARY:Mass transfer in AGB binaries - uncovering a new evolution channel by 3D radiation hydrodynamic simulations URL;TYPE=URI:/info/1025/7570.htm END:VEVENT BEGIN:VEVENT UID:7539@kiaa.pku.edu.cn DTSTAMP:20210310T111137Z CREATED:20210310T111137Z DESCRIPTION:Primordial black holes (PBHs) are widely considered as a hypothetical candidate of dark matter. However, the formation and astrophysical effects of PBHs still remain unclear. To gain the insights from the theoretical perspective, we recently proposed a novel mechanism of the sound speed resonance (SSR) cosmology that produces PBHs efficiently. I will briefly review the PBHs and the SSR mechanis... DTSTART;TZID=Asia/Shanghai:20210429T160000 DTEND;TZID=Asia/Shanghai:20210429T170000 LAST-MODIFIED:20210310T111137Z LOCATION:KIAA-auditorium SUMMARY:Primordial black holes and gravitational waves from the sound speed resonance cosmology URL;TYPE=URI:/info/1024/7539.htm END:VEVENT BEGIN:VEVENT UID:7033@kiaa.pku.edu.cn DTSTAMP:20200619T122536Z CREATED:20200619T122536Z DESCRIPTION:Labor Day Holida DTSTART;TZID=Asia/Shanghai:20210430T000000 DTEND;TZID=Asia/Shanghai:20210501T000000 LAST-MODIFIED:20200619T122536Z LOCATION: SUMMARY:Labor Day Holiday URL;TYPE=URI:/info/1089/7033.htm END:VEVENT BEGIN:VEVENT UID:7576@kiaa.pku.edu.cn DTSTAMP:20210323T132418Z CREATED:20210323T132418Z DESCRIPTION:Abstract:Brown dwarfs and relatively isolated young extrasolar giant planets occupy an important parameter space to understand planetary atmospheres. Recent observations of these worlds have provided unprecedented details to probe atmospheric dynamics in a new regime, raising critical questions about mechanisms generating the global circulation and its fundamental nature. Two major mechanisms h... DTSTART;TZID=Asia/Shanghai:20210504T133000 DTEND;TZID=Asia/Shanghai:20210504T143000 LAST-MODIFIED:20210323T132418Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Stormy weather on brown dwarfs and isolated young giant planets URL;TYPE=URI:/info/1025/7576.htm END:VEVENT BEGIN:VEVENT UID:7561@kiaa.pku.edu.cn DTSTAMP:20210316T094812Z CREATED:20210316T094812Z DESCRIPTION:The Zeeman effect and dust grain alignment are two major methods for probing magnetic fields (B-fields) in molecular clouds, largely motivated by the study of star formation, as the B-field may regulate gravitational contraction and channel turbulence velocity. I will review our observations of B-fields over the past decade, along with our interpretation. Galactic B-fields anchor molecular clou... DTSTART;TZID=Asia/Shanghai:20210506T160000 DTEND;TZID=Asia/Shanghai:20210506T170000 LAST-MODIFIED:20210316T094812Z LOCATION:Remote Talk https://zoom.com.cn/j/6223937478?pwd=QU9Pdm12ZHhGUHVKbFhaUWtsUDVMdz09 Meeting ID: 622 393 7478 Passcode: 2BYguM SUMMARY:Magnetic Fields in Molecular Clouds—Observation and Interpretation URL;TYPE=URI:/info/1024/7561.htm END:VEVENT BEGIN:VEVENT UID:7578@kiaa.pku.edu.cn DTSTAMP:20210325T205549Z CREATED:20210325T205549Z DESCRIPTION:abstract:This talk will try to give a timely review of dark matter physics. Dark matter is now one of the most important research areas in both astrophysics and particle physics. Yet, its non-gravitational property has not been firmly detected. This talk will start from the success of modern cosmology, showing the initial motivations of dark matter. The rest of the talk is devoted to provide a ... DTSTART;TZID=Asia/Shanghai:20210511T133000 DTEND;TZID=Asia/Shanghai:20210511T143000 LAST-MODIFIED:20210325T205549Z LOCATION:KIAA first meeting room + zoom SUMMARY:Dark Matter: from astrophysics to particle physics? URL;TYPE=URI:/info/1025/7578.htm END:VEVENT BEGIN:VEVENT UID:7562@kiaa.pku.edu.cn DTSTAMP:20210316T095845Z CREATED:20210316T095845Z DESCRIPTION:A big step forward in multi-messange astrophysics has  recently occurred by the first detection of gravitational waves, GW150914 and the first simultaneous detection of gravitational-wave and electromagnetic signals from a binaryneutron star merger GW170817. In this talk, I'll give an overview of what we learned from the multi-messanger signals of GW170817 including the neutron star equation of... DTSTART;TZID=Asia/Shanghai:20210513T160000 DTEND;TZID=Asia/Shanghai:20210513T170000 LAST-MODIFIED:20210316T095845Z LOCATION:Remote Talk Join Zoom Meeting https://zoom.com.cn/j/85869758491?pwd=MjFxVnJFOHNDS1Y4MEtyQ3ZjV0Uwdz09 Meeting ID: 858 6975 8491 Passcode: 597850 SUMMARY:Multi-messanger astrophysics of compact binary mergers URL;TYPE=URI:/info/1024/7562.htm END:VEVENT BEGIN:VEVENT UID:7577@kiaa.pku.edu.cn DTSTAMP:20210324T122359Z CREATED:20210324T122359Z DESCRIPTION:abstract:Core-collapse supernovae mark the death of massive stars. It is an important topic to understand what progenitor stars produce the supernovae of different subtypes. Answering this question is key to bridge stellar evolutionary theories and supernova explosion models. Supernova progenitors can be investigated by analysing their pre-explosion images, binary companion stars, host star clu... DTSTART;TZID=Asia/Shanghai:20210518T133000 DTEND;TZID=Asia/Shanghai:20210518T143000 LAST-MODIFIED:20210324T122359Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Understanding supernova progenitors with stellar population analysis URL;TYPE=URI:/info/1025/7577.htm END:VEVENT BEGIN:VEVENT UID:7581@kiaa.pku.edu.cn DTSTAMP:20210331T101221Z CREATED:20210331T101221Z DESCRIPTION:Turbulence is ubiquitous in the universe and plays an important role in diverse astrophysical processes, from star formation to galaxy evolution. Measuring turbulence in astrophysics, however, is not always easy. In this talk, I will discuss novel techniques my group recently developed in the analysis of turbulence in the interstellar medium (ISM) and the intracluster medium (ICM). We study the... DTSTART;TZID=Asia/Shanghai:20210520T110000 DTEND;TZID=Asia/Shanghai:20210520T120000 LAST-MODIFIED:20210331T101221Z LOCATION:Remote talk Join Zoom Meeting https://zoom.com.cn/j/89252651917?pwd=ZEVvMUZ0U1BpYks3L0grNis4TFIvZz09 Meeting ID: 892 5265 1917 Passcode: 857878 SUMMARY:Turbulence in the Universe: from the Interstellar Medium to the Intracluster Medium URL;TYPE=URI:/info/1024/7581.htm END:VEVENT BEGIN:VEVENT UID:7574@kiaa.pku.edu.cn DTSTAMP:20210322T203530Z CREATED:20210322T203530Z DESCRIPTION:abstract:As a typical disk galaxy, our Milky Way is a unique laboratory for studying the matter constitution and distribution and testing the formation and evolution scenarios of galaxies in general. Although the study of the Milky Way has a long history, many fundamental questions still remain to be answered. In the past decades, extensive large surveys have been carried out to obtain multi-di... DTSTART;TZID=Asia/Shanghai:20210525T133000 DTEND;TZID=Asia/Shanghai:20210525T143000 LAST-MODIFIED:20210322T203530Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Milky Way stellar population census with large spectroscopic surveys URL;TYPE=URI:/info/1025/7574.htm END:VEVENT BEGIN:VEVENT UID:7563@kiaa.pku.edu.cn DTSTAMP:20210316T100123Z CREATED:20210316T100123Z DESCRIPTION:Cosmic-rays (CRs) are relativistic particles that pervade galaxies and intergalactic space. They likely play a dynamically important role in a wide range of astrophysics systems by interacting with thermal gas via magnetic fields, whose consequence is known as CR feedback. The key to understanding CR feedback lies in how well the gas and CRs are coupled, which is in most cases described by a CR... DTSTART;TZID=Asia/Shanghai:20210527T160000 DTEND;TZID=Asia/Shanghai:20210527T170000 LAST-MODIFIED:20210316T100123Z LOCATION:KIAA-auditorium SUMMARY:The microphysics of cosmic-ray feedback URL;TYPE=URI:/info/1024/7563.htm END:VEVENT BEGIN:VEVENT UID:7575@kiaa.pku.edu.cn DTSTAMP:20210322T222623Z CREATED:20210322T222623Z DESCRIPTION:Abstract:The preference of supernova subtypes for specific galaxy environments (e.g., stellar age, nebular metallicity, location in the host), as well as the correlation of supernova properties with host galaxy parameters, point to the physical nature and evolutionary stage of their stellar progenitors, which are otherwise undetectable beyond the local universe. With the largest available ... DTSTART;TZID=Asia/Shanghai:20210601T133000 DTEND;TZID=Asia/Shanghai:20210601T143000 LAST-MODIFIED:20210322T222623Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Supernovae as a stellar population phenomenon - Statistical constraints on supernova progenitors from host galaxy properties URL;TYPE=URI:/info/1025/7575.htm END:VEVENT BEGIN:VEVENT UID:7533@kiaa.pku.edu.cn DTSTAMP:20210308T103921Z CREATED:20210308T103921Z DESCRIPTION:Weak gravitational lensing is one of the most powerful techniques to probe cosmology. In this talk, I will first  briefly review the current status of weak lensing surveys. Then I will present the recent cosmological parameter constraints using the Kilo-Degree Survey (KiDS). The results of different statistical quantities can find the S8 tension in comparison with the Planck CMB measurements, i... DTSTART;TZID=Asia/Shanghai:20210603T160000 DTEND;TZID=Asia/Shanghai:20210603T170000 LAST-MODIFIED:20210308T103921Z LOCATION:KIAA-auditorium SUMMARY:Weak lensing with the Kilo-Degree Survey URL;TYPE=URI:/info/1024/7533.htm END:VEVENT BEGIN:VEVENT UID:7590@kiaa.pku.edu.cn DTSTAMP:20210406T100459Z CREATED:20210406T100459Z DESCRIPTION:Tidal disruption event (TDE) occurs when a star approaches too close to a supermassive black hole (SMBH). If the circumnuclear medium is dusty, the original TDE emission (soft X-ray, UV, optical) will be reprocessed into infrared (IR) band like an echo. Therefore, the IR echoes provide us a unique opportunity to study the dust environment around SMBHs down to subparsec scale, which is otherwise... DTSTART;TZID=Asia/Shanghai:20210610T160000 DTEND;TZID=Asia/Shanghai:20210610T170000 LAST-MODIFIED:20210406T100459Z LOCATION:KIAA-auditorium SUMMARY:Infrared Echoes of Tidal Disruption Events URL;TYPE=URI:/info/1024/7590.htm END:VEVENT BEGIN:VEVENT UID:7474@kiaa.pku.edu.cn DTSTAMP:20210115T091707Z CREATED:20210115T091707Z DESCRIPTION:Dragon Boat Festival Holiday 202 DTSTART;TZID=Asia/Shanghai:20210614T000000 DTEND;TZID=Asia/Shanghai:20210614T235900 LAST-MODIFIED:20210115T091707Z LOCATION: SUMMARY:Dragon Boat Festival Holiday 2021 URL;TYPE=URI:/info/1089/7474.htm END:VEVENT BEGIN:VEVENT UID:7582@kiaa.pku.edu.cn DTSTAMP:20210331T124330Z CREATED:20210331T124330Z DESCRIPTION:Abstract:In recent years, lunar exploration programs worldwide have accumulated a large amount of remote sensing and in-situ observational data, and the latest Chinese mission has returned lunar samples to Earth. The related research continuously advances our understanding of the internal structure and evolution of the Moon. High resolution and precision gravity data from the GRAIL mission have... DTSTART;TZID=Asia/Shanghai:20210615T133000 DTEND;TZID=Asia/Shanghai:20210615T143000 LAST-MODIFIED:20210331T124330Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Lunar Crustal Structure and Thermo-Mechanical Evolution URL;TYPE=URI:/info/1025/7582.htm END:VEVENT BEGIN:VEVENT UID:7600@kiaa.pku.edu.cn DTSTAMP:20210407T090343Z CREATED:20210407T090343Z DESCRIPTION:Our universe is filled with stochastic gravitational waves (GWs) with a large range of frequencies, which may have various astrophysical/cosmological origins in the early universe. In this talk I will briefly review the properties of stochastic GWs induced by the scalar perturbation, as well as its connection to the phenomenology of primordial black holes (PBHs). Recently, NANOGrav reported the... DTSTART;TZID=Asia/Shanghai:20210617T160000 DTEND;TZID=Asia/Shanghai:20210617T170000 LAST-MODIFIED:20210407T090343Z LOCATION:KIAA-auditorium SUMMARY:Stochastic gravitational waves induced by scalar perturbation: theory and recent developments URL;TYPE=URI:/info/1024/7600.htm END:VEVENT BEGIN:VEVENT UID:7617@kiaa.pku.edu.cn DTSTAMP:20210531T122542Z CREATED:20210531T122542Z DESCRIPTION:Abstract:The microlensing mission planned on the Roman Space Telescope, scheduled to launch in the mid-2020s, is expected to revolutionize our understanding of exoplanet demographics. Owing to the pathological parameter space of binary microlensing which contains a multitude of local likelihood maximas that are narrow and deep, current analysis of such events are done on a case-by-case basis wi... DTSTART;TZID=Asia/Shanghai:20210622T133000 DTEND;TZID=Asia/Shanghai:20210622T143000 LAST-MODIFIED:20210531T122542Z LOCATION:KIAA 1st meeting room + Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Fast and automated inference of Roman binary microlensing events with neural posterior estimation URL;TYPE=URI:/info/1025/7617.htm END:VEVENT BEGIN:VEVENT UID:7604@kiaa.pku.edu.cn DTSTAMP:20210428T170151Z CREATED:20210428T170151Z DESCRIPTION:Dr.Ruobing DongPlanets form in gaseous protoplanetary disks surrounding newborn stars. As such, the most direct way to learn how they form from observations, is to observe them forming in disks. In the past, this was difficult due to a lack of observational capabilities, and planet formation was a subject of theoretical research. Now, thanks to a fleet of new instruments with unprecedented reso... DTSTART;TZID=Asia/Shanghai:20210624T160000 DTEND;TZID=Asia/Shanghai:20210624T170000 LAST-MODIFIED:20210428T170151Z LOCATION:KIAA-auditorium SUMMARY:Tracing the formation of “other worlds” in circumstellar disks around newborn stars URL;TYPE=URI:/info/1024/7604.htm END:VEVENT BEGIN:VEVENT UID:7583@kiaa.pku.edu.cn DTSTAMP:20210331T164400Z CREATED:20210331T164400Z DESCRIPTION:abstract:The cosmic web is the pattern imprinted by large-scale structure caused by gravitational collapse of the initial fluctuations of the universe, and is also intimately related to how galaxies evolve from the density field. Studies of the cosmic web have largely been limited to z<1 since it requires huge samples of spectroscopic redshifts, but over the past few years I have pioneered the ... DTSTART;TZID=Asia/Shanghai:20210629T133000 DTEND;TZID=Asia/Shanghai:20210629T143000 LAST-MODIFIED:20210331T164400Z LOCATION:Zoom ID: 885 6999 9778 , passcode: astroPKU SUMMARY:Exploring the Large-Scale Cosmic Web at Cosmic Noon (z~2) URL;TYPE=URI:/info/1025/7583.htm END:VEVENT BEGIN:VEVENT UID:7630@kiaa.pku.edu.cn DTSTAMP:20210707T090748Z CREATED:20210707T090748Z DESCRIPTION:Astronomy Summer Cam DTSTART;TZID=Asia/Shanghai:20210709T000000 DTEND;TZID=Asia/Shanghai:20210712T001211 LAST-MODIFIED:20210707T090748Z LOCATION: SUMMARY:Astronomy Summer Camp for College Students URL;TYPE=URI:/info/1089/7630.htm END:VEVENT BEGIN:VEVENT UID:7629@kiaa.pku.edu.cn DTSTAMP:20210625T100915Z CREATED:20210625T100915Z DESCRIPTION:Summer Vacatio DTSTART;TZID=Asia/Shanghai:20210719T000000 DTEND;TZID=Asia/Shanghai:20210829T000000 LAST-MODIFIED:20210625T100915Z LOCATION: SUMMARY:Summer Vacation URL;TYPE=URI:/info/1089/7629.htm END:VEVENT BEGIN:VEVENT UID:7628@kiaa.pku.edu.cn DTSTAMP:20210624T094553Z CREATED:20210624T094553Z DESCRIPTION:Gaia first discovered the snail shell structure in the Z-Vz phase space of stars in the Milky Way disk, suggesting that the disk was perturbed and dynamically young. This represents the beginning of a new promising research field, i.e., ‘Galactoseismology’, where we can study the Galactic structure formation and evolution history using the phase space signals. In this talk, I will first intro... DTSTART;TZID=Asia/Shanghai:20210722T160000 DTEND;TZID=Asia/Shanghai:20210722T170000 LAST-MODIFIED:20210624T094553Z LOCATION:KIAA-auditorium SUMMARY:Phase Space Structure in the Era of Galactoseismology URL;TYPE=URI:/info/1024/7628.htm END:VEVENT BEGIN:VEVENT UID:7772@kiaa.pku.edu.cn DTSTAMP:20210901T155355Z CREATED:20210901T155355Z DESCRIPTION:abstract:Most of the structural and evolutionary properties of galaxies rely on the numbers of stars with different masses. The initial mass function (IMF), referred to as the distribution of the initial stellar mass formed in a stellar population, plays crucial roles from the formation of stars to the evolution of galaxies. While many works found no variation of IMF in the Milky Way, studies o... DTSTART;TZID=Asia/Shanghai:20210913T133000 DTEND;TZID=Asia/Shanghai:20210913T135500 LAST-MODIFIED:20210901T155355Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472 ,Passcode: astroPKU SUMMARY:The Variation of Stellar Initial Mass Function with Age and Metallicity URL;TYPE=URI:/info/1025/7772.htm END:VEVENT BEGIN:VEVENT UID:7770@kiaa.pku.edu.cn DTSTAMP:20210830T153934Z CREATED:20210830T153934Z DESCRIPTION:In order to understand a process as complex as planet formation, the most extreme cases are often the most revealing. At the hottest extreme of planet formation are the ultra-short-period planets (USP, orbital period ~1 day, <2 R_earth) which orbit their host stars just a few stellar radii away. Our uniform analysis of USPs revealed a prevalence of Earth-like rocky composition. The high mutual ... DTSTART;TZID=Asia/Shanghai:20210916T153000 DTEND;TZID=Asia/Shanghai:20210916T163000 LAST-MODIFIED:20210830T153934Z LOCATION:Remote Talk SUMMARY:Probing Planet Formation with the Most Extreme Cases: the “ultra-short-periods”, the “super-puffs” and the “Oblique" Planets URL;TYPE=URI:/info/1024/7770.htm END:VEVENT BEGIN:VEVENT UID:7805@kiaa.pku.edu.cn DTSTAMP:20210917T161712Z CREATED:20210917T161712Z DESCRIPTION:Abstract: In the Gaia era, with the help of Large sky surveys such as current RAVE, LAMOST, APOGEE, GALAH, TESS, DESI catalog and future plans such as WEAVE, 4MOST, PFS, MSE, CSST, etc. There is no doubt that we are entering into the golden era to investigate the formation history and structure of our home galaxy in multiple stellar populations of six-phase space by chemical tagging, time taggi... DTSTART;TZID=Asia/Shanghai:20210920T133000 DTEND;TZID=Asia/Shanghai:20210920T153000 LAST-MODIFIED:20210917T161712Z LOCATION:Meeting ID: 822 8287 7472 Passcode: astroPKU SUMMARY:Mapping the Milky Way Disk Population Structures and Galactoseismology with large sky surveys (MWDPSG) URL;TYPE=URI:/info/1025/7805.htm END:VEVENT BEGIN:VEVENT UID:7475@kiaa.pku.edu.cn DTSTAMP:20210115T091936Z CREATED:20210115T091936Z DESCRIPTION:The Mid-Autumn festival holiday DTSTART;TZID=Asia/Shanghai:20210921T000000 DTEND;TZID=Asia/Shanghai:20210921T230000 LAST-MODIFIED:20210115T091936Z LOCATION: SUMMARY:The Mid-Autumn festival holiday URL;TYPE=URI:/info/1089/7475.htm END:VEVENT BEGIN:VEVENT UID:7624@kiaa.pku.edu.cn DTSTAMP:20210623T103217Z CREATED:20210623T103217Z DESCRIPTION:The Large High Altitude Air Shower Observatory (LHAASO) as the largest ground based Gamma Ray detector array is built up. The 3/4 array has been operated for months. Many VHE gamma ray sources has been observed including well known sources such as the Crab and Mkr421. With many sources found having strong emission of gamma rays in UHE(> 0.1 PeV) band, LHAASO starts the era of the UHE gamma ray ... DTSTART;TZID=Asia/Shanghai:20210923T153000 DTEND;TZID=Asia/Shanghai:20210923T163000 LAST-MODIFIED:20210623T103217Z LOCATION:KIAA-auditorium SUMMARY:LHAASO and Its First Few Discoveries —— Onset of the UHE -ray Astronomy URL;TYPE=URI:/info/1024/7624.htm END:VEVENT BEGIN:VEVENT UID:7773@kiaa.pku.edu.cn DTSTAMP:20210901T190837Z CREATED:20210901T190837Z DESCRIPTION:Abstract:Gaia survey offers a most enormous data volume and exquisite data quality compared to any ground-based projects. However, magnitude-dependent systematic effects at the 10 mmag level or higher are shown in Gaia DR2. We use the spectroscopy-based stellar color regression method with ∼0.7 million common stars between Gaia and LAMOST to acquire color corrections in G − GRP and GBP − GRP... DTSTART;TZID=Asia/Shanghai:20210927T133000 DTEND;TZID=Asia/Shanghai:20210927T142000 LAST-MODIFIED:20210901T190837Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472 ,Passcode: astroPKU SUMMARY:Analyzing Gaia photometric data: High precision photometric calibrations and binary fractions of the field GK dwarfs URL;TYPE=URI:/info/1025/7773.htm END:VEVENT BEGIN:VEVENT UID:7771@kiaa.pku.edu.cn DTSTAMP:20210830T154749Z CREATED:20210830T154749Z DESCRIPTION:The evolution of massive stellar binaries plays a key role in the formation of a range of transients: gravitational-wave sources, gamma ray bursts, some supernovae, luminous red novae, etc.  Unfortunately, a variety of key steps in the evolutionary process are poorly understood.  I will discuss some recent theoretical work on a range of processes, from common envelope physics to wind-driven mas... DTSTART;TZID=Asia/Shanghai:20210930T153000 DTEND;TZID=Asia/Shanghai:20210930T163000 LAST-MODIFIED:20210830T154749Z LOCATION:Remote Talk Zoom Link: https://zoom.us/j/86332626010?pwd=QlhhL3dSS0VDM0V4K2FlS0NudXhYUT09 Meeting ID: 863 3262 6010 Passcode: 295742 SUMMARY:Some recent results in massive binary evolution URL;TYPE=URI:/info/1024/7771.htm END:VEVENT BEGIN:VEVENT UID:7476@kiaa.pku.edu.cn DTSTAMP:20210115T092207Z CREATED:20210115T092207Z DESCRIPTION:National Days Holida DTSTART;TZID=Asia/Shanghai:20211001T002207 DTEND;TZID=Asia/Shanghai:20211007T000000 LAST-MODIFIED:20210115T092207Z LOCATION: SUMMARY:National Day Holiday URL;TYPE=URI:/info/1089/7476.htm END:VEVENT BEGIN:VEVENT UID:7834@kiaa.pku.edu.cn DTSTAMP:20211003T155503Z CREATED:20211003T155503Z DESCRIPTION:Abstract:Angular momentum is a key property regulating star formation and evolution. However, the physics driving the distribution of the stellar rotation rates of early-type main-sequence stars is as yet poorly understood. Using our catalog of over 40,000 early-type stars with homogeneous vsini parameters, we review the statistical properties of their stellar rotation rates. We discuss the imp... DTSTART;TZID=Asia/Shanghai:20211011T133000 DTEND;TZID=Asia/Shanghai:20211011T135500 LAST-MODIFIED:20211003T155503Z LOCATION:KIAA 1st meeting room + Zoom Meeting ID: 822 8287 7472 ,Passcode: astroPKU SUMMARY:Exploring the stellar rotation of early-type stars in the LAMOST Medium-Resolution Survey URL;TYPE=URI:/info/1025/7834.htm END:VEVENT BEGIN:VEVENT UID:7795@kiaa.pku.edu.cn DTSTAMP:20210917T140820Z CREATED:20210917T140820Z DESCRIPTION:Magnetic fields play an important role in the evolution of interstellar medium and star formation. As the only direct tracer of interstellar field strength, credible Zeeman measurements remain sparse due to rather limited number of spectral lines with discernible Zeeman effect, particularly for cold, molecular gas. Here we report the detection of a magnetic field of +3.8 ± 0.3 μG through the H... DTSTART;TZID=Asia/Shanghai:20211014T153000 DTEND;TZID=Asia/Shanghai:20211014T163000 LAST-MODIFIED:20210917T140820Z LOCATION:KIAA-auditorium SUMMARY:An early transition to magnetic supercriticality in star formation URL;TYPE=URI:/info/1024/7795.htm END:VEVENT BEGIN:VEVENT UID:7833@kiaa.pku.edu.cn DTSTAMP:20210930T150439Z CREATED:20210930T150439Z DESCRIPTION:Abstract:Intermediate/Extreme mass ratio inspiral (IMRI/EMRI) system provides a good tool to test the nature of gravity in strong field. We construct the self-force and use the self-force method to generate accurate waveform templates for IMRIS/EMRIs on quasi-elliptical orbits in Brans-Dicke theory. The extra monopole and dipole emissions in Brans-Dicke theory accelerate the orbital decay, so t... DTSTART;TZID=Asia/Shanghai:20211018T133000 DTEND;TZID=Asia/Shanghai:20211018T142000 LAST-MODIFIED:20210930T150439Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472, Passcode: astroPKU SUMMARY:Constraint on Brans-Dicke theory from Intermediate/Extreme Mass Ratio Inspirals with self-force method URL;TYPE=URI:/info/1025/7833.htm END:VEVENT BEGIN:VEVENT UID:7796@kiaa.pku.edu.cn DTSTAMP:20210917T142151Z CREATED:20210917T142151Z DESCRIPTION:Hypervelocity stars (HVSs) are rare objects of extreme fast velocities allowing them to escape the Milky Way galaxy.One of the most commonly proposed scenarios is that they originate near the Galactic center (GC) by dynamical interactions between (binary) stars and the central massive black hole(s) (MBH). Alternative explanations exist, for examples, they could be the tidal debris of an accrete... DTSTART;TZID=Asia/Shanghai:20211021T153000 DTEND;TZID=Asia/Shanghai:20211021T163000 LAST-MODIFIED:20210917T142151Z LOCATION:KIAA-auditorium SUMMARY:On the origins of Hypervelocity stars as revealed by large-scale Galactic surveys URL;TYPE=URI:/info/1024/7796.htm END:VEVENT BEGIN:VEVENT UID:7780@kiaa.pku.edu.cn DTSTAMP:20210910T144417Z CREATED:20210910T144417Z DESCRIPTION:bstract:Since the launch of Galaxy Zoo (GZ) in 2009, the very first project on the Zooniverse citizen science platform, the number of data driven citizen science projects boosted. In the radio astronomy regime, the most well-known project is called Radio Galaxy Zoo. Initiated by the Evolutionary Map of the Universe (EMU) project team, RGZ 1 was launched at 2015 (Banfield et al. 2015) as a pathf... DTSTART;TZID=Asia/Shanghai:20211025T133000 DTEND;TZID=Asia/Shanghai:20211025T135000 LAST-MODIFIED:20210910T144417Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472, Passcode: astroPKU SUMMARY:Radio Galaxy Zoo: a case study of how radio astronomers collaborate with the citizens URL;TYPE=URI:/info/1025/7780.htm END:VEVENT BEGIN:VEVENT UID:7797@kiaa.pku.edu.cn DTSTAMP:20210917T142617Z CREATED:20210917T142617Z DESCRIPTION:Heavy particles can be produced on shell during inflation and leave distinct signals in the correlations of density fluctuations. These signals can be searched for in the future CMB/LSS/21cm observations. In this talk I will introduce the basics of this cosmological collider program. I will then describe some recent works along this direction with fun physics and visibly large signals, includin... DTSTART;TZID=Asia/Shanghai:20211028T153000 DTEND;TZID=Asia/Shanghai:20211028T163000 LAST-MODIFIED:20210917T142617Z LOCATION:KIAA-auditorium SUMMARY:Recent progress in cosmological collider physics URL;TYPE=URI:/info/1024/7797.htm END:VEVENT BEGIN:VEVENT UID:7907@kiaa.pku.edu.cn DTSTAMP:20211027T145558Z CREATED:20211027T145558Z DESCRIPTION:Abstract: Massive O and B stars reveal the places of their birth by powerful ultraviolet (UV) radiation. The stellar UV photons illuminate and heat the surrounding gas up to thousands of Kelvin. UV photons from the massive stars ionize hydrogen atoms and lead to the formation of HII regions. The HII regions continue to grow in size, driven by the difference of the thermal pressure between the h... DTSTART;TZID=Asia/Shanghai:20211101T133000 DTEND;TZID=Asia/Shanghai:20211101T141500 LAST-MODIFIED:20211027T145558Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Gas and dust in vicinity of young massive stars URL;TYPE=URI:/info/1025/7907.htm END:VEVENT BEGIN:VEVENT UID:7798@kiaa.pku.edu.cn DTSTAMP:20210917T142754Z CREATED:20210917T142754Z DESCRIPTION:More than two decades after the first discoveries of exoplanets, the field has entered the era of finding Earth analogs as well as building samples of well-characterized exoplanets to study their formation and evolution. Precise radial velocity (RV) is taking the lead in surveying nearby bright stars for Earth analogs, while playing an important role in characterizing populations of exoplanets,... DTSTART;TZID=Asia/Shanghai:20211104T153000 DTEND;TZID=Asia/Shanghai:20211104T163000 LAST-MODIFIED:20210917T142754Z LOCATION:KIAA-auditorium SUMMARY:The Pursuit of Earth 2.0 and Other Worlds with High Precision Radial Velocities URL;TYPE=URI:/info/1024/7798.htm END:VEVENT BEGIN:VEVENT UID:7837@kiaa.pku.edu.cn DTSTAMP:20211008T142014Z CREATED:20211008T142014Z DESCRIPTION:abstract:The structure and evolution of the spiral arms of our Milky Way are basic but long-standing questions in astronomy. In particular, the lifetime of spiral arms is still a puzzle and has not been well constrained from observations. We used a large catalogue of open clusters in Gaia EDR3 to inspect these issues by analysing the distributions, kinematic properties, vertical distributions, ... DTSTART;TZID=Asia/Shanghai:20211108T133000 DTEND;TZID=Asia/Shanghai:20211108T135500 LAST-MODIFIED:20211008T142014Z LOCATION:zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:Evolution of the spiral arm structure of the Milky Way revealed by open star clusters URL;TYPE=URI:/info/1025/7837.htm END:VEVENT BEGIN:VEVENT UID:7799@kiaa.pku.edu.cn DTSTAMP:20210917T143530Z CREATED:20210917T143530Z DESCRIPTION:"The next generation of wide-area, sensitive X-ray surveys designed to map the hot and energetic Universe has arrived, thanks to eROSITA (extended ROentgen Survey with an Imaging Telescope Array), the core instrument on the Russian-German Spektrum-Roentgen-Gamma (SRG) mission. eROSITA high sensitivity, large field of view, high spatial resolution and survey efficiency is bound to revolutionise ... DTSTART;TZID=Asia/Shanghai:20211111T153000 DTEND;TZID=Asia/Shanghai:20211111T163000 LAST-MODIFIED:20210917T143530Z LOCATION:Remote Talk Join Zoom Meeting https://zoom.us/j/82813111957?pwd=Tkt3VmdtcmZPYUhWS3EzV2xKVmhJQT09 Meeting ID: 828 1311 1957 Passcode: 143360 SUMMARY:Of Bubbles, Filaments, Echoes and Eruptions: First Results from eROSITA on SRG URL;TYPE=URI:/info/1024/7799.htm END:VEVENT BEGIN:VEVENT UID:7836@kiaa.pku.edu.cn DTSTAMP:20211008T135203Z CREATED:20211008T135203Z DESCRIPTION:abstract:I will briefly introduce the main observational characteristics of radio-quiet AGN variability from UV/optical to X-ray, including single-band property and inter-band interrelationship, such as correlation and lag. These variable properties are usually understood within the X-ray reprocessing scenario, however, several challenges against this scenario have been unveiled. Instead, in a ... DTSTART;TZID=Asia/Shanghai:20211115T133003 DTEND;TZID=Asia/Shanghai:20211115T142003 LAST-MODIFIED:20211008T135203Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:Variability of radio-quiet AGNs from UV/optical to X-ray URL;TYPE=URI:/info/1025/7836.htm END:VEVENT BEGIN:VEVENT UID:7800@kiaa.pku.edu.cn DTSTAMP:20210917T145015Z CREATED:20210917T145015Z DESCRIPTION:The three-body problem is arguably the oldest open question in astrophysics and has resisted a general analytic solution for centuries. Various forms of perturbation theory provide solutions in portions of parameter space, but only where hierarchies of masses and/or separations exist. Numerical integrations show that bound, non-hierarchical triple systems of Newtonian point particles will almos... DTSTART;TZID=Asia/Shanghai:20211118T153000 DTEND;TZID=Asia/Shanghai:20211118T163000 LAST-MODIFIED:20210917T145015Z LOCATION:Zoom Link: https://zoom.us/j/86426763198?pwd=S0d1Sm5NemFzWGpwZUlHazZldFVTdz09 Meeting ID: 864 2676 3198 Passcode: 689647 SUMMARY:A New Statistical Solution to the Chaotic Three-Body Problem URL;TYPE=URI:/info/1024/7800.htm END:VEVENT BEGIN:VEVENT UID:7831@kiaa.pku.edu.cn DTSTAMP:20210927T161249Z CREATED:20210927T161249Z DESCRIPTION:Abstract:I will introduce my studies on distance measurements based on the Milky Way Imaging Scroll Painting (MWISP) survey and the Gaia DR2 catalog. Molecular clouds cause extinction augmentation along lines of sight, which can be gauged with stellar parallax and extinction. For molecular clouds at high Galactic latitudes, distance measurements are straightforward, but for those in the Galacti... DTSTART;TZID=Asia/Shanghai:20211122T133000 DTEND;TZID=Asia/Shanghai:20211122T142000 LAST-MODIFIED:20210927T161249Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:Samples and Distances of Molecular Clouds In the Milky Way URL;TYPE=URI:/info/1025/7831.htm END:VEVENT BEGIN:VEVENT UID:7801@kiaa.pku.edu.cn DTSTAMP:20210917T145347Z CREATED:20210917T145347Z DESCRIPTION:Research on understanding the formation process of planetary systems has been progressing very rapidly in recent years, but there are still many unknowns. In this talk, mainly focusing on high-resolution observations using ALMA, I would like to talk about such as the growth of dust (solid) suggested in protoplanetary disks and the ongoing observational project to probe detailed gas kinematics i... DTSTART;TZID=Asia/Shanghai:20211125T153000 DTEND;TZID=Asia/Shanghai:20211125T163000 LAST-MODIFIED:20210917T145347Z LOCATION:Join Zoom Meeting https://zoom.us/j/85454027981?pwd=VTA2UG4vcXoyWWxUWURCdkdXM2lSZz09 Meeting ID: 854 5402 7981 Passcode: 955691 SUMMARY:Detailed look at birthplaces of planets with ALMA URL;TYPE=URI:/info/1024/7801.htm END:VEVENT BEGIN:VEVENT UID:8075@kiaa.pku.edu.cn DTSTAMP:20211122T103553Z CREATED:20211122T103553Z DESCRIPTION:AbstractSince their initial discovery 20 years ago, very distant (z>2) and massive galaxies that form prodigious number of young stars – so-called dusty star-forming galaxies - represent a serious challenge for the theory of galaxy formation. On the one hand, they are difficult to detect because they reside in dense regions of the distant Universe and contain dusty particles which absorb most ... DTSTART;TZID=Asia/Shanghai:20211129T133000 DTEND;TZID=Asia/Shanghai:20211129T141500 LAST-MODIFIED:20211122T103553Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:Dusty giants with ALMA: Cosmic evolution of dust-to-stellar mass ratio in very distant galaxies URL;TYPE=URI:/info/1025/8075.htm END:VEVENT BEGIN:VEVENT UID:8072@kiaa.pku.edu.cn DTSTAMP:20211122T102358Z CREATED:20211122T102358Z DESCRIPTION:Connections between the circumgalactic medium (CGM) gas accretion and the galaxy central star formation has long been inspected. In a series of two papers, we put this interlink between the CGM and star formation into a framework on a larger scale (several hundreds of kpcs), i.e., the merging environment of neighbouring galaxies. Such an environment, to a certain degree, maps out various paths ... DTSTART;TZID=Asia/Shanghai:20211202T153000 DTEND;TZID=Asia/Shanghai:20211202T163000 LAST-MODIFIED:20211122T102358Z LOCATION:KIAA-auditorium SUMMARY:The entangled fate between galaxies, their ambient gas and larger-scale environments URL;TYPE=URI:/info/1024/8072.htm END:VEVENT BEGIN:VEVENT UID:7835@kiaa.pku.edu.cn DTSTAMP:20211005T141333Z CREATED:20211005T141333Z DESCRIPTION:abstract:The growing history of the Milky Way has been tightly imprinted into the elemental abundances of the interstellar medium, especially for the isotopes of Carbon, Nitrogen, and Oxygen, due to their different origins of parental stars. The ratios of these CNO isotopes have been well known as their systematic gradients from the inner Galaxy to the outer disk, which, in turn, set constraint... DTSTART;TZID=Asia/Shanghai:20211206T133000 DTEND;TZID=Asia/Shanghai:20211206T135500 LAST-MODIFIED:20211005T141333Z LOCATION:zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:The CNO isotope ratio gradients of the Milky Way: new results from the Galactic outer disk URL;TYPE=URI:/info/1025/7835.htm END:VEVENT BEGIN:VEVENT UID:7802@kiaa.pku.edu.cn DTSTAMP:20210917T145700Z CREATED:20210917T145700Z DESCRIPTION:About 5000 exoplanets have been confirmed, and the number is still increasing rapidly. Discovering planets itself is insufficient, however, unless we also know which of them are potentially habitable: Do any of these planets have conditions that would support life? What factors favor the building and maintenance of a temperate environment for life? In this talk, I will present how to define hab... DTSTART;TZID=Asia/Shanghai:20211209T153000 DTEND;TZID=Asia/Shanghai:20211209T163000 LAST-MODIFIED:20210917T145700Z LOCATION:KIAA-auditorium SUMMARY:Habitable Zone: Definitions, Estimations, and Recent Advances URL;TYPE=URI:/info/1024/7802.htm END:VEVENT BEGIN:VEVENT UID:7910@kiaa.pku.edu.cn DTSTAMP:20211027T153610Z CREATED:20211027T153610Z DESCRIPTION:Abstract:Polarization observations are a current trend of the Atacama Large Millimeter/submillimeter Array (ALMA), which trace magnetic fields or other phenomena around protostars. My previous ALMA observations suggested that magnetic fields with a strength of ~2 mG could result in an infall motion at ~30% of the free fall velocity in the envelope of the Class I protostellar system TMC-1A. To v... DTSTART;TZID=Asia/Shanghai:20211213T133000 DTEND;TZID=Asia/Shanghai: LAST-MODIFIED:20211027T153610Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Polarization and Kinematics observations toward the Class I protostar TMC-1A URL;TYPE=URI:/info/1025/7910.htm END:VEVENT BEGIN:VEVENT UID:8140@kiaa.pku.edu.cn DTSTAMP:20211201T102540Z CREATED:20211201T102540Z DESCRIPTION:The successful achievement of near-IR interferometry by European Southern Observatory marks the beginning of the era of high-resolution astronomy in the optical/near-IR. This talk will introduce how to perform high-precision measurement of black hole masses, cosmological distances, the history of the expanding universe, and nano-Hz gravitational waves from supermassive binary black holes in the... DTSTART;TZID=Asia/Shanghai:20211216T153000 DTEND;TZID=Asia/Shanghai:20211216T163000 LAST-MODIFIED:20211201T102540Z LOCATION:KIAA-auditorium SUMMARY:Study of Supermassive Black Holes in the Era of Interferometry URL;TYPE=URI:/info/1024/8140.htm END:VEVENT BEGIN:VEVENT UID:7838@kiaa.pku.edu.cn DTSTAMP:20211008T160057Z CREATED:20211008T160057Z DESCRIPTION:Abstract:This talk primarily focus on introducing the kinematically misaligned galaxies in MaNGA survey, including (1) gas-star misalignments; (2) galaxies with two counter-rotating stellar disks; (3) galaxies with two misaligned gas disks. Through studying the properties of these three types of galaxies, we discuss their formation scenarios and the influence of external processes on the evolut... DTSTART;TZID=Asia/Shanghai:20211220T133000 DTEND;TZID=Asia/Shanghai:20211220T142000 LAST-MODIFIED:20211008T160057Z LOCATION:zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU SUMMARY:Kinematic misaligned galaxies in MaNGA URL;TYPE=URI:/info/1025/7838.htm END:VEVENT BEGIN:VEVENT UID:8076@kiaa.pku.edu.cn DTSTAMP:20211122T152500Z CREATED:20211122T152500Z DESCRIPTION:abstract:Distance is a fundamental parameter in astronomical observations. How to accurately measure distances to objects has always been an important issue. Interstellar extinction, the absorption and scattering of starlight, affects the accuracy of distance measurements based on stellar physics. Therefore, an extinction correction is often required before distance measurements.  For supernova... DTSTART;TZID=Asia/Shanghai:20211227T133000 DTEND;TZID=Asia/Shanghai:20211227T142000 LAST-MODIFIED:20211122T152500Z LOCATION:KIAA 1st meeting room + zoom 822 8287 7472 SUMMARY:Distances to the Supernova Remnants and the molecular clouds URL;TYPE=URI:/info/1025/8076.htm END:VEVENT BEGIN:VEVENT UID:8143@kiaa.pku.edu.cn DTSTAMP:20211210T145050Z CREATED:20211210T145050Z DESCRIPTION:Winter Vacatio DTSTART;TZID=Asia/Shanghai:20220107T000000 DTEND;TZID=Asia/Shanghai:20220220T000000 LAST-MODIFIED:20211210T145050Z LOCATION: SUMMARY:Winter Vacation URL;TYPE=URI:/info/1089/8143.htm END:VEVENT BEGIN:VEVENT UID:8220@kiaa.pku.edu.cn DTSTAMP:20220223T141952Z CREATED:20220223T141952Z DESCRIPTION:Abstract: Understanding the nature and properties of the sources of the reionization requires quantifying the escape fraction (f_esc) of the Lyman Continuum photons from the galaxies. The most straightforward method to measure f_esc is to detect LyC photons from galaxies directly. In recent years, several works have detected LyC sources from the nearby universe to redshift ∼4. However, the suc... DTSTART;TZID=Asia/Shanghai:20220228T133000 DTEND;TZID=Asia/Shanghai:20220228T140000 LAST-MODIFIED:20220223T141952Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Detection of Lyman Continuum from z>3 galaxies in the Hubble Deep UV Legacy Survey URL;TYPE=URI:/info/1025/8220.htm END:VEVENT BEGIN:VEVENT UID:8130@kiaa.pku.edu.cn DTSTAMP:20211126T134802Z CREATED:20211126T134802Z DESCRIPTION:Hot accretion flow is widely believed to be essential for our understanding of low-luminosity AGNs (LLAGNs) and black hole X-ray binaries (BHBs) in their hard (and quiescent) state. In this talk, I will first review the current status of accretion theory. The progresses viewed from fundamental physics perspective are angular momentum transport, turbulent heating mechanism, and outflow/wind; fro... DTSTART;TZID=Asia/Shanghai:20220303T153000 DTEND;TZID=Asia/Shanghai:20220303T163000 LAST-MODIFIED:20211126T134802Z LOCATION:Zoom Link: https://zoom.us/j/89093214828?pwd=TmxISnBxeG8xV2lEMTVUY1RMbVJCdz09 Meeting ID: 890 9321 4828 Passcode: 033141 SUMMARY:Hot accretion flow: progress and application URL;TYPE=URI:/info/1024/8130.htm END:VEVENT BEGIN:VEVENT UID:8221@kiaa.pku.edu.cn DTSTAMP:20220303T094317Z CREATED:20220303T094317Z DESCRIPTION:Abstract: We examine whether stellar flyby simulations can initiate FU Orionis outbursts using 3d hydrodynamics simulations coupled to live Monte Carlo radiative transfer. We find that a flyby where the secondary penetrates the circumprimary disc triggers a 1–2 year rise in the mass accretion rate to 10^−4 M_sun/yr that remains high (&10^−5 M_sun/yr) for more than a hundred years, similar to... DTSTART;TZID=Asia/Shanghai:20220307T133000 DTEND;TZID=Asia/Shanghai:20220307T140000 LAST-MODIFIED:20220303T094317Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:On the rise times in FU Orionis events URL;TYPE=URI:/info/1025/8221.htm END:VEVENT BEGIN:VEVENT UID:8201@kiaa.pku.edu.cn DTSTAMP:20220215T140626Z CREATED:20220215T140626Z DESCRIPTION:Supernovae ultimately deposit ~10% of their total energy in a population of relativistic cosmic rays that subsequently interact with the interstellar medium (ISM) via magnetic forces. Because these particles lose energy to radiation only slowly compared to the ~90% of the supernova energy that is deposited in the ISM as heat, they are a potentially important feedback mechanism in galaxies despi... DTSTART;TZID=Asia/Shanghai:20220310T153000 DTEND;TZID=Asia/Shanghai:20220310T163000 LAST-MODIFIED:20220215T140626Z LOCATION:https://zoom.us/j/82497007833?pwd=Z3dOYjEwU1NvaUY2QVZhR042UnVYUT09 Meeting ID: 824 9700 7833 Passcode: 060437 SUMMARY:Cosmic rays in star-forming galaxies: transport, feedback, and non-thermal messengers URL;TYPE=URI:/info/1024/8201.htm END:VEVENT BEGIN:VEVENT UID:8230@kiaa.pku.edu.cn DTSTAMP:20220309T093758Z CREATED:20220309T093758Z DESCRIPTION:Abstract: The proposed TianQin mission is a space-borne gravitational wave observatory, which is planned to harvest gravitational wave science in the milli-Hertz range. In this talk, I'll give a brief overview of the scientific prospect of the TianQin observatory, specifically on the astronomical implication of TianQin DTSTART;TZID=Asia/Shanghai:20220314T133000 DTEND;TZID=Asia/Shanghai:20220314T142000 LAST-MODIFIED:20220309T093758Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Gravitational Universe with the TianQin observatory URL;TYPE=URI:/info/1025/8230.htm END:VEVENT BEGIN:VEVENT UID:8202@kiaa.pku.edu.cn DTSTAMP:20220215T141222Z CREATED:20220215T141222Z DESCRIPTION:We still do not understand how planets form, or why extra-solar planetary systems are so different from our own solar system. Recent observations of protoplanetary discs have revealed rings and gaps, spirals and asymmetries. These features have been interpreted as signatures of newborn protoplanets, but the exact origin is unknown, and remained until recently poorly constrained by direct observ... DTSTART;TZID=Asia/Shanghai:20220317T153000 DTEND;TZID=Asia/Shanghai:20220317T163000 LAST-MODIFIED:20220215T141222Z LOCATION:https://zoom.us/j/84029625902?pwd=MTlya0hiVVhqdkVFamRiVVFkUDIydz09 Meeting ID: 840 2962 5902 Passcode: 148845 SUMMARY:Observing Planet Formation URL;TYPE=URI:/info/1024/8202.htm END:VEVENT BEGIN:VEVENT UID:8223@kiaa.pku.edu.cn DTSTAMP:20220303T165148Z CREATED:20220303T165148Z DESCRIPTION:ABSTRACT: Astronomical instrumentation has greatly advanced over the last 40 years: for example with digital detectors, space telescopes and +8m class ground-based telescopes. However, the signal-based detection paradigm (for example from Petrosian or Kron in the 1970s, mostly used as implemented in SExtractor from the mid-1990s) is still the dominant method of low-level data analysis: detecti... DTSTART;TZID=Asia/Shanghai:20220321T133000 DTEND;TZID=Asia/Shanghai:20220321T140000 LAST-MODIFIED:20220303T165148Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 Passcode: astroPKU Link: https://us02web.zoom.us/j/82282877472pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Non-parametric detection and segmentation in astronomical imaging URL;TYPE=URI:/info/1025/8223.htm END:VEVENT BEGIN:VEVENT UID:8203@kiaa.pku.edu.cn DTSTAMP:20220215T141518Z CREATED:20220215T141518Z DESCRIPTION:Gravitational-wave detections have opened up a new window to the universe. We have detected signals from many compact-binary events, including the famous binary neutron star event GW170817, the first joint detection with electromagnetic and gravitational waves. GW170817 has revolutionized our understanding of neutron star physics and the origin of heavy elements. However, due to limitations fro... DTSTART;TZID=Asia/Shanghai:20220324T153000 DTEND;TZID=Asia/Shanghai:20220324T163000 LAST-MODIFIED:20220215T141518Z LOCATION:KIAA-auditorium SUMMARY:kHz Gravitational Wave Detector URL;TYPE=URI:/info/1024/8203.htm END:VEVENT BEGIN:VEVENT UID:8240@kiaa.pku.edu.cn DTSTAMP:20220325T135817Z CREATED:20220325T135817Z DESCRIPTION:Abstract: Since the systematic discovery of filamentary structures in molecular clouds by the Herschel observations, more and more attention has been paid to filaments. Molecular clouds usually exhibit filamentary structures, within which a significant fraction of gravitationally bound dense cores and protostars are embedded. We wonder if all of the molecular clouds are filamentary. If not, wha... DTSTART;TZID=Asia/Shanghai:20220328T133000 DTEND;TZID=Asia/Shanghai:20220328T140000 LAST-MODIFIED:20220325T135817Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:MWSIP Survey: A large sample of molecular clouds classified as filaments and nonfilaments URL;TYPE=URI:/info/1025/8240.htm END:VEVENT BEGIN:VEVENT UID:8170@kiaa.pku.edu.cn DTSTAMP:20211227T111721Z CREATED:20211227T111721Z DESCRIPTION:We experience a golden era in testing and exploring relativistic gravity. Whether it is results from gravitational wave detectors, satellite or lab experiments, radio astronomy plays an important complementary role. Here one can mention the cosmic microwave background, black hole imaging and, obviously, binary pulsars. This talk will provide an overview how these methods relate to each other, a... DTSTART;TZID=Asia/Shanghai:20220331T153000 DTEND;TZID=Asia/Shanghai:20220331T163000 LAST-MODIFIED:20211227T111721Z LOCATION:Join Zoom Meeting https://zoom.us/j/83775634656?pwd=YlI0UlR6Nlc4WHZOMGpLYTR3VjVZUT09 Meeting ID: 837 7563 4656 Passcode: 473114 SUMMARY:Probing relativistic gravity with radio astronomy URL;TYPE=URI:/info/1024/8170.htm END:VEVENT BEGIN:VEVENT UID:8228@kiaa.pku.edu.cn DTSTAMP:20220307T113809Z CREATED:20220307T113809Z DESCRIPTION:2022 Qingming Festival Holida DTSTART;TZID=Asia/Shanghai:20220403T000000 DTEND;TZID=Asia/Shanghai:20220405T000000 LAST-MODIFIED:20220307T113809Z LOCATION: SUMMARY:2022 Qingming Festival Holiday URL;TYPE=URI:/info/1089/8228.htm END:VEVENT BEGIN:VEVENT UID:8233@kiaa.pku.edu.cn DTSTAMP:20220310T145022Z CREATED:20220310T145022Z DESCRIPTION:Abstract:The properties of protostellar (Class 0/I) disks play an important role in planet formation by setting the environment for dust grain growth and the initial conditions for subsequent protoplanetary (Class II) disk evolution. However, obtaining these properties, especially the disk mass, has been challenging because translating observations of dust thermal emission to disk mass are subj... DTSTART;TZID=Asia/Shanghai:20220404T133000 DTEND;TZID=Asia/Shanghai:20220404T142000 LAST-MODIFIED:20220310T145022Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Protostellar disks might be way more massive than we thought: Insights through a synergy between theory and observation URL;TYPE=URI:/info/1025/8233.htm END:VEVENT BEGIN:VEVENT UID:8204@kiaa.pku.edu.cn DTSTAMP:20220215T141752Z CREATED:20220215T141752Z DESCRIPTION:太赫兹，一般定义为0.1THz~10THz的频率区间，对应的波长范围是3毫米至30微米，涵盖部分毫米波段、亚毫米波段和大部分远红外波段。太赫兹天文观测在恒星及其行星系统的形成与演化和早期宇宙演化等前沿领域研究中，具有不可替代的作用。超导探测器则在太赫兹谱段天体物理与宇宙学观测研究中发挥越来越重要的作用，推动了太赫兹天文学的快速发展。本报告将主要介绍当前国际主流的太赫兹高灵敏度超导探测技术发展现状和天文应用，并... DTSTART;TZID=Asia/Shanghai:20220407T153000 DTEND;TZID=Asia/Shanghai:20220407T163000 LAST-MODIFIED:20220215T141752Z LOCATION:Join Zoom Meeting https://zoom.us/j/89492776551?pwd=WlhyVU0yWkNGVk1wRWtkbzFiNFVaQT09 Meeting ID: 894 9277 6551 Passcode: 890761 SUMMARY:Superconducting detectors for terahertz astronomical applications. URL;TYPE=URI:/info/1024/8204.htm END:VEVENT BEGIN:VEVENT UID:8224@kiaa.pku.edu.cn DTSTAMP:20220303T171009Z CREATED:20220303T171009Z DESCRIPTION:ABSTRACT: I will report on a spectroscopic program to search for dual quasars using Subaru Hyper Suprime-Cam (HSC) images of SDSS quasars, which represent an important stage during galaxy mergers. Using the full sample of six spectroscopically confirmed dual quasars, we find that the black holes in these systems have black hole masses similar to single SDSS quasars as well as their bolometric ... DTSTART;TZID=Asia/Shanghai:20220411T133000 DTEND;TZID=Asia/Shanghai:20220411T140000 LAST-MODIFIED:20220303T171009Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 Passcode: astroPKU Link: https://us02web.zoom.us/j/82282877472pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:An insight of SMBH-host galaxy coevolution through dual quasar systems URL;TYPE=URI:/info/1025/8224.htm END:VEVENT BEGIN:VEVENT UID:8251@kiaa.pku.edu.cn DTSTAMP:20220331T141501Z CREATED:20220331T141501Z DESCRIPTION:Abstract: Ultralight bosons can potentially accumulate around these supermassive black holes and form a gravitational atom-like bound state. A new way to look for the gravitational atom made of axion is through birefringence effect from the axion-photon coupling.The presence of coherently oscillating axion leads to a frequency independent oscillation to the electric vector position angle (EVPA)... DTSTART;TZID=Asia/Shanghai:20220411T150000 DTEND;TZID=Asia/Shanghai:20220411T160000 LAST-MODIFIED:20220331T141501Z LOCATION:KIAA first meeting room; Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Probing axion using Event Horizon Telescope polarimetric measurement URL;TYPE=URI:/info/1025/8251.htm END:VEVENT BEGIN:VEVENT UID:8163@kiaa.pku.edu.cn DTSTAMP:20211227T105717Z CREATED:20211227T105717Z DESCRIPTION:Planetary nebulae (PNe) are descendants of the low- to intermediate-mass stars (1-8 solar masses), which account for the absolute majority (>90%) of the stellar populations in the universe. As the only interstellar media that exist in both galaxy disk and halo, PNe are widespread emission-line objects. They are one of the few classes of celestial objects that are active in almost every part of ... DTSTART;TZID=Asia/Shanghai:20220414T153000 DTEND;TZID=Asia/Shanghai:20220414T163000 LAST-MODIFIED:20211227T105717Z LOCATION:Join Zoom Meeting https://zoom.us/j/82361636041?pwd=dktUZmpYekh1QWgzTTFqcUxjRXdxdz09 Meeting ID: 823 6163 6041 Passcode: 998118 SUMMARY:Chemical and Morphological Studies of Planetary Nebulae as Probes of Stellar and Galaxy Evolution URL;TYPE=URI:/info/1024/8163.htm END:VEVENT BEGIN:VEVENT UID:8231@kiaa.pku.edu.cn DTSTAMP:20220310T144121Z CREATED:20220310T144121Z DESCRIPTION:Abstract:The astrophysical sites which dominate the production of r-process elements have been a matter of contention for decades. The event GW170817/AT2017gfo, with the confirmed observation of the neutron-capture element strontium, originally raised hopes that neutron star mergers (NSM) could be a leading contributor to the production of heavy elements. However, galactic chemical evolution (G... DTSTART;TZID=Asia/Shanghai:20220418T133000 DTEND;TZID=Asia/Shanghai:20220418T142000 LAST-MODIFIED:20220310T144121Z LOCATION:Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:The Galactic Chemical Evolution of Heavy Elements URL;TYPE=URI:/info/1025/8231.htm END:VEVENT BEGIN:VEVENT UID:8253@kiaa.pku.edu.cn DTSTAMP:20220413T141730Z CREATED:20220413T141730Z DESCRIPTION:On Earth’s surface, there are only a handful of high-quality astronomical sites that meet the requirements for very large next-generation facilities. In the context of scientific opportunities in time-domain astronomy, a good site on the Tibetan Plateau will bridge the longitudinal gap between the known best sites1,2 (all in the Western Hemisphere). The Tibetan Plateau is the highest plateau o... DTSTART;TZID=Asia/Shanghai:20220421T153000 DTEND;TZID=Asia/Shanghai:20220421T163000 LAST-MODIFIED:20220413T141730Z LOCATION:KIAA-auditorium SUMMARY:Reaching the deep universe from Lenghu on the Tibetan plateau -current status and future perspective URL;TYPE=URI:/info/1024/8253.htm END:VEVENT BEGIN:VEVENT UID:8232@kiaa.pku.edu.cn DTSTAMP:20220310T144626Z CREATED:20220310T144626Z DESCRIPTION:Abstract: Most astrophysical objects are moving due to an interaction with their environment or due to the motion of their host system. Gravitational wave sources are no exception. In contrast, most gravitational wave sources are likely moving with velocities of 100s to 1000s km/s since they usually form in the densest regions of galaxies. We show that when considering a complete description of... DTSTART;TZID=Asia/Shanghai:20220425T133000 DTEND;TZID=Asia/Shanghai:20220425T142000 LAST-MODIFIED:20220310T144626Z LOCATION:KIAA first meeting room; Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Detecting a constant center-of-mass velocity for gravitational wave sources URL;TYPE=URI:/info/1025/8232.htm END:VEVENT BEGIN:VEVENT UID:8252@kiaa.pku.edu.cn DTSTAMP:20220408T090422Z CREATED:20220408T090422Z DESCRIPTION:Red supergiants (RSGs) are massive Population I stars, the major progenitor of supernovae. With strong stellar wind, RSGs are an important source of interstellar dust, in particularly for the high redshift galaxies in the early universe when low-mass stars have not evolved to the asymptotic giant branch phase. However, the estimation of contribution of RSGs to interstellar dust suffers large un... DTSTART;TZID=Asia/Shanghai:20220428T153000 DTEND;TZID=Asia/Shanghai:20220428T163000 LAST-MODIFIED:20220408T090422Z LOCATION:Join Zoom Meeting https://zoom.us/j/82046267592?pwd=WXo3Q1ZmL0ZQK1F0clFZTllqRnR3Zz09 Meeting ID: 820 4626 7592 Passcode: 342641 SUMMARY:The most complete sample of red supergiants in 14 galaxies of the Local Group URL;TYPE=URI:/info/1024/8252.htm END:VEVENT BEGIN:VEVENT UID:8182@kiaa.pku.edu.cn DTSTAMP:20211228T094649Z CREATED:20211228T094649Z DESCRIPTION:Labor Day Holida DTSTART;TZID=Asia/Shanghai:20220501T000000 DTEND;TZID=Asia/Shanghai:20220506T000000 LAST-MODIFIED:20211228T094649Z LOCATION: SUMMARY:Labor Day Holiday URL;TYPE=URI:/info/1089/8182.htm END:VEVENT BEGIN:VEVENT UID:8225@kiaa.pku.edu.cn DTSTAMP:20220303T171247Z CREATED:20220303T171247Z DESCRIPTION:ABSTRACT:I present X-ray properties of mid-IR selected Active Galactic Nuclei (AGN) at z < 4 in the 140 deg^2 field observed by SRG/eROSITA using the PV phase program (eFEDS). By cross-matching the WISE 22 µm (W4)-detected sample and the eFEDS X-ray point-source catalog (Salvato et al. 2022), 693 galaxies were selected. We then compiled a multi-wavelength dataset extending from X-ray to far-IR... DTSTART;TZID=Asia/Shanghai:20220509T133000 DTEND;TZID=Asia/Shanghai:20220509T140000 LAST-MODIFIED:20220303T171247Z LOCATION:Full online, Zoom Meeting ID: 822 8287 7472, Passcode: astroPKU, Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:X-ray properties of WISE selected AGN viewed with eROSITA URL;TYPE=URI:/info/1025/8225.htm END:VEVENT BEGIN:VEVENT UID:8205@kiaa.pku.edu.cn DTSTAMP:20220215T142747Z CREATED:20220215T142747Z DESCRIPTION:Galaxies are complex systems including stars, gas, dark matter, and et cetra. The stellar content is best viewed using optical photometry and spectroscopy, while the neutral gas is best traced by the HI 21cm line in the radio band. I will first summarize our previous results on stellar population distribution within galaxies (mostly in 1D radial profiles) made using optical surveys such as Pan-... DTSTART;TZID=Asia/Shanghai:20220512T153000 DTEND;TZID=Asia/Shanghai:20220512T163000 LAST-MODIFIED:20220215T142747Z LOCATION:https://zoom.us/j/81238353860?pwd=cEpHWjNpdlBmYjdVa0J1NzVlaUYydz09 Meeting ID: 812 3835 3860 Passcode: 413300 SUMMARY:Nearby galaxies: a view from optical to radio URL;TYPE=URI:/info/1024/8205.htm END:VEVENT BEGIN:VEVENT UID:8311@kiaa.pku.edu.cn DTSTAMP:20220512T214507Z CREATED:20220512T214507Z DESCRIPTION:Abstract: In the past decade, ALMA observations have revealed that a large fraction of protoplanetary disks contains rings in the dust continuum and gas molecular line emission. Dust trapping induced by gap-opening planets is a popular explanation for these rings. However, it is unclear whether pressure bumps can survive for evolutionary time scales. In addition, the formation of planets is ine... DTSTART;TZID=Asia/Shanghai:20220516T133000 DTEND;TZID=Asia/Shanghai:20220516T143000 LAST-MODIFIED:20220512T214507Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU, Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Chickens or Eggs? Rings in Protoplanetary Disks URL;TYPE=URI:/info/1025/8311.htm END:VEVENT BEGIN:VEVENT UID:8206@kiaa.pku.edu.cn DTSTAMP:20220215T143006Z CREATED:20220215T143006Z DESCRIPTION:The multi-messenger observations of binary merger events have provided us unprecedented opportunities to study the state of matter under extreme conditions, such as those inside neutron stars. For instance, depending on the total mass of the merging binary, the post-merger remnant could undergo collapse to black hole at different timescales, producing very different gravitational wave and elect... DTSTART;TZID=Asia/Shanghai:20220519T153000 DTEND;TZID=Asia/Shanghai:20220519T163000 LAST-MODIFIED:20220215T143006Z LOCATION:https://zoom.us/j/87865454404?pwd=d8eG-_Y6oZwlOb9bqbLS7s-Vg2fGUH.1 Meeting ID: 878 6545 4404 Passcode: 921641 SUMMARY:Post-merger evolution of binary quark stars URL;TYPE=URI:/info/1024/8206.htm END:VEVENT BEGIN:VEVENT UID:8312@kiaa.pku.edu.cn DTSTAMP:20220512T215934Z CREATED:20220512T215934Z DESCRIPTION:Abstract: I will report some recent work in stellar and planetary sciences. They are stellar convection dynamo, a tidal dynamo in close binaries, Ohmic dissipation for tidal evolution, radius anomaly of hot Jupiters, and wave transmission in the stellar or planetary interior DTSTART;TZID=Asia/Shanghai:20220523T133000 DTEND;TZID=Asia/Shanghai:20220523T141500 LAST-MODIFIED:20220512T215934Z LOCATION:Zoom information: Meeting ID: 822 8287 7472 , Passcode: astroPKU, Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Some recent work in stellar and planetary sciences URL;TYPE=URI:/info/1025/8312.htm END:VEVENT BEGIN:VEVENT UID:8226@kiaa.pku.edu.cn DTSTAMP:20220303T171415Z CREATED:20220303T171415Z DESCRIPTION:ABSTRACT: This presentation shows ALMA 100 GHz continuum observations at 0.05" (4 pc) resolution of the kiloparsec-scale jet seen in the nearby Seyfert galaxy NGC 1068. ALMA detected parsec-scale blobs at the head of the jet. According to the radio flux (0.8mJy), the spectral index (0.5), and the size (12 pc), a strongly amplified magnetic-field (B~230 G) is confirmed, which indicates that the ... DTSTART;TZID=Asia/Shanghai:20220530T133000 DTEND;TZID=Asia/Shanghai:20220530T140000 LAST-MODIFIED:20220303T171415Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:ALMA detection of parsec-scale blobs at the head of kiloparsec-scale jet in the nearby Seyfert galaxy NGC 1068 URL;TYPE=URI:/info/1025/8226.htm END:VEVENT BEGIN:VEVENT UID:8229@kiaa.pku.edu.cn DTSTAMP:20220307T114019Z CREATED:20220307T114019Z DESCRIPTION:2022 Dragon Boat Festival Holida DTSTART;TZID=Asia/Shanghai:20220603T000000 DTEND;TZID=Asia/Shanghai:20220605T000000 LAST-MODIFIED:20220307T114019Z LOCATION: SUMMARY:2022 Dragon Boat Festival Holiday URL;TYPE=URI:/info/1089/8229.htm END:VEVENT BEGIN:VEVENT UID:8235@kiaa.pku.edu.cn DTSTAMP:20220313T104118Z CREATED:20220313T104118Z DESCRIPTION:Abstract: Long gamma-ray bursts (LGRBs) are associated with the death of massive stars, they therefore should be a powerful tool for tracing the cosmic star formation rate (SFR) in principle. However, numerous studies indicate that the LGRB rate does not purely trace the SFR, remaining an open question in this field. Actually, the intrinsic formation rate and luminosity function of LGRBs cannot... DTSTART;TZID=Asia/Shanghai:20220606T133000 DTEND;TZID=Asia/Shanghai:20220606T142000 LAST-MODIFIED:20220313T104118Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:The evolution of the formation rate and luminosity function of long gamma-ray bursts URL;TYPE=URI:/info/1025/8235.htm END:VEVENT BEGIN:VEVENT UID:8210@kiaa.pku.edu.cn DTSTAMP:20220221T090705Z CREATED:20220221T090705Z DESCRIPTION:Since the formal commencement of the Five-hundred-meter Aperture Spherical radio Telescope, more than 120 peer-reviewed papers have been published, including at least 1 cover article on SCPMA, 1 on Science, 2 on Nature Astronomy, and 5 on Nature (including the one published online this morning).Although never have doubted FAST's eventual historical impact, I am stunned and overwhelmed by its in... DTSTART;TZID=Asia/Shanghai:20220609T153000 DTEND;TZID=Asia/Shanghai:20220609T163000 LAST-MODIFIED:20220221T090705Z LOCATION:Join Zoom Meeting https://zoom.us/j/85297708549?pwd=elFXUEdFNFBXKzZtbGVQNzIrb0ZYdz09 Meeting ID: 852 9770 8549 Passcode: 289896 SUMMARY:Probe the Universe: Faraday Style URL;TYPE=URI:/info/1024/8210.htm END:VEVENT BEGIN:VEVENT UID:8310@kiaa.pku.edu.cn DTSTAMP:20220512T161404Z CREATED:20220512T161404Z DESCRIPTION:Abstract：In this work, we consider the burst signal of the dark photon, the hypothetical vector boson of the U_B or U_B-L gauge group, generated by a compact binary star system. The absence of the signal in the laser interferometer puts bounds on the coupling constant ϵ to the ordinary matter. It turns out that if the dark photon is massless, ϵ^2 is at the order of 10^-37–10^-33 at most; in... DTSTART;TZID=Asia/Shanghai:20220613T133000 DTEND;TZID=Asia/Shanghai:20220613T143000 LAST-MODIFIED:20220512T161404Z LOCATION:Online Zoom meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Dark photon bursts from compact binary systems and constraints URL;TYPE=URI:/info/1025/8310.htm END:VEVENT BEGIN:VEVENT UID:8330@kiaa.pku.edu.cn DTSTAMP:20220616T192008Z CREATED:20220616T192008Z DESCRIPTION:Abstract: Understanding how super-massive black holes (SMBHs) form and grow in the early universe has become a major challenge since the discovery of luminous quasars only 700 million years after the Big Bang. Simulations indicate an evolutionary sequence of dust-reddened quasars emerging from heavily dust-obscured starbursts that then transition to unobscured luminous quasars by expelling gas ... DTSTART;TZID=Asia/Shanghai:20220620T133000 DTEND;TZID=Asia/Shanghai:20220620T140000 LAST-MODIFIED:20220616T192008Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:A dusty, compact object bridging galaxies and quasars at cosmic dawn URL;TYPE=URI:/info/1025/8330.htm END:VEVENT BEGIN:VEVENT UID:8183@kiaa.pku.edu.cn DTSTAMP:20211228T094841Z CREATED:20211228T094841Z DESCRIPTION:Summer Vacatio DTSTART;TZID=Asia/Shanghai:20220711T000000 DTEND;TZID=Asia/Shanghai:20220828T000000 LAST-MODIFIED:20211228T094841Z LOCATION: SUMMARY:Summer Vacation URL;TYPE=URI:/info/1089/8183.htm END:VEVENT BEGIN:VEVENT UID:8374@kiaa.pku.edu.cn DTSTAMP:20220708T144200Z CREATED:20220708T144200Z DESCRIPTION:9:15am:  WelcomeGaia DR3---------------9:30am:  Fu Yuming, Extragalactic sources in Gaia DR39:45am:  Zhang Shuo, Stellar parameters in Gaia DR310:00am:  Zhou Xingyu, Star formation in Gaia DR310:15-10:45am:  Coffee/tea breakPlanet Formation--------------10:45am:  Aoyama Yuhiko,  Modeling of observable signatures of forming giant planets 11:00am: Yang Haifeng, Probing Magnetic Fields in Protopla... DTSTART;TZID=Asia/Shanghai:20220714T091500 DTEND;TZID=Asia/Shanghai:20220714T170000 LAST-MODIFIED:20220708T144200Z LOCATION:KIAA Auditorium SUMMARY:Summer Science Day URL;TYPE=URI:/info/1089/8374.htm END:VEVENT BEGIN:VEVENT UID:8550@kiaa.pku.edu.cn DTSTAMP:20220902T103708Z CREATED:20220902T103708Z DESCRIPTION:ABSTRACTLinearly polarized emission from dust grains and molecular spectroscopy is an effective probe of the magnetic field topology in the interstellar medium and molecular clouds. The longstanding Davis-Chandrasekhar-Fermi (DCF) method and the recently developed Histogram of Relative Orientations (HRO) analysis and the polarization-intensity gradient (KTH) method are widely used to assess the... DTSTART;TZID=Asia/Shanghai:20220906T133000 DTEND;TZID=Asia/Shanghai:20220906T140000 LAST-MODIFIED:20220902T103708Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Magnetic field properties in molecular clouds and star formation: analysis methods and interpretation URL;TYPE=URI:/info/1025/8550.htm END:VEVENT BEGIN:VEVENT UID:8533@kiaa.pku.edu.cn DTSTAMP:20220825T131052Z CREATED:20220825T131052Z DESCRIPTION:Based on the MWISP survey, we study high-z CO emission toward the tangent points, in which the distances of the molecular clouds (MCs) are well determined. In the region of l = 12°--26° and |b| < 5°, a total of 321 MCs with |z|>110 pc are identified, of which nearly 30 extreme high-z MCs (EHMCs at |z|> 260 pc) are concentrated in a very narrow region of R_GC = 2.6--3.1 kpc. The EHMC concentrati... DTSTART;TZID=Asia/Shanghai:20220908T153000 DTEND;TZID=Asia/Shanghai:20220908T163000 LAST-MODIFIED:20220825T131052Z LOCATION:Zoom Link: https://zoom.us/j/85367481924?pwd=OTZLRG5YeVRMUUlqWGdlWU1SVkJwZz09 Meeting ID: 853 6748 1924 Passcode: 804585 SUMMARY:The Galactic Nuclear Wind and the CO Disk URL;TYPE=URI:/info/1024/8533.htm END:VEVENT BEGIN:VEVENT UID:8570@kiaa.pku.edu.cn DTSTAMP:20220912T091640Z CREATED:20220912T091640Z DESCRIPTION:Abstract:PSR B1821-24A is located in the dense globular cluster M28 and is known to exhibit complex timing behavior. The nature leading to the complex timing behavior become an interesting question. We present 33 years of timing observations of this pulsar and investigate various effects that could be responsible for the observed spin behavior. We analyzed the noise properties, and modeled the ... DTSTART;TZID=Asia/Shanghai:20220913T133000 DTEND;TZID=Asia/Shanghai:20220913T142000 LAST-MODIFIED:20220912T091640Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Thirty-three years of timing PSR B1821-24A with the Lovell Telescope and LEAP URL;TYPE=URI:/info/1025/8570.htm END:VEVENT BEGIN:VEVENT UID:8534@kiaa.pku.edu.cn DTSTAMP:20220825T160857Z CREATED:20220825T160857Z DESCRIPTION:a. The multiwavelength observations and theoretical modelings of magnetars are presented. Magnetars may be young neutron stars having strong magnetic field. They are different from normal pulsars mainly because their magnetic field may be twisted. A twisted magnetic field will explain the outburst, timing and radio polarization of magnetars. Possible presence of multipole field may also explain... DTSTART;TZID=Asia/Shanghai:20220915T153000 DTEND;TZID=Asia/Shanghai:20220915T163000 LAST-MODIFIED:20220825T160857Z LOCATION:https://zoom.us/j/87479260027?pwd=SGNEeThERHBJZ3R5WEJRN3d3U20xdz09 Meeting ID: 874 7926 0027 Passcode: 954780 SUMMARY:Magnetospheric physics of magnetars URL;TYPE=URI:/info/1024/8534.htm END:VEVENT BEGIN:VEVENT UID:8577@kiaa.pku.edu.cn DTSTAMP:20220915T152437Z CREATED:20220915T152437Z DESCRIPTION:Abstract:About one hundred gravitational wave (GW) events have been detected by LIGO/Virgo, most of which (>90%) are from binary black-holes (BBH). Thus, we have opportunities to testing general relativity (GR) in the strong gravity regime. Generally, in GW data analyses, we do not consider effects of charge since it is often thought to be negligible for an astrophysical BH. However, according ... DTSTART;TZID=Asia/Shanghai:20220920T133000 DTEND;TZID=Asia/Shanghai:20220920T142000 LAST-MODIFIED:20220915T152437Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU, Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Constraining BH charge with GW data of LIGO/Virgo URL;TYPE=URI:/info/1025/8577.htm END:VEVENT BEGIN:VEVENT UID:8536@kiaa.pku.edu.cn DTSTAMP:20220830T091119Z CREATED:20220830T091119Z DESCRIPTION:Computational simulations are essential tools in astrophysics today and many codes are publicly available. Athena++ is a magnetohydrodynamics simulation code we develop in international collaboration led by Institute for Advanced Study / Princeton University. This code supports adaptive mesh refinement and various physical processes for astrophysical applications, and adopts new concepts to imp... DTSTART;TZID=Asia/Shanghai:20220922T153000 DTEND;TZID=Asia/Shanghai:20220922T163000 LAST-MODIFIED:20220830T091119Z LOCATION:Join Zoom Meeting https://zoom.us/j/87979065838?pwd=a1BoaUdYVVpyM29wbUdBcUR5NjBnQT09 Meeting ID: 879 7906 5838 Passcode: 415671 SUMMARY:The Athena++ Adaptive Mesh Refinement Framework: Code Design and Applications URL;TYPE=URI:/info/1024/8536.htm END:VEVENT BEGIN:VEVENT UID:8581@kiaa.pku.edu.cn DTSTAMP:20220919T155119Z CREATED:20220919T155119Z DESCRIPTION:Abstract:Recent improvements in observational instruments and techniques enable us to observe the forming planets directly. Particularly, the detection of hydrogen lines is expected to be a clue to understanding the gas accretion process onto the protoplanets. The hydrogen line excess due to gas accretion is well known and has been studied in the context of accreting protostars. As the simples... DTSTART;TZID=Asia/Shanghai:20220927T133000 DTEND;TZID=Asia/Shanghai:20220927T142000 LAST-MODIFIED:20220919T155119Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Hydrogen line emission from accreting planets; Difference from accreting protostars URL;TYPE=URI:/info/1025/8581.htm END:VEVENT BEGIN:VEVENT UID:8535@kiaa.pku.edu.cn DTSTAMP:20220830T090842Z CREATED:20220830T090842Z DESCRIPTION:I will introduce  our recent work on excitation and radiation model of atomic hydrogen in ionized gas, as well on-going  radio recombination line (RRL) observations with FAST.  The key result is that most RRLs are weak maser instead of thermal emission.  We also discuss the systematic bias of using line (RRL) to continuum ratio (free-free) to obtain electron density of ionized gas under LTE ass... DTSTART;TZID=Asia/Shanghai:20220929T153000 DTEND;TZID=Asia/Shanghai:20220929T163000 LAST-MODIFIED:20220830T090842Z LOCATION:Join Zoom Meeting https://zoom.us/j/83102096662?pwd=SStwUlU5NHFKSHF6L0t0allwa1Bldz09 Meeting ID: 831 0209 6662 Passcode: 368889 SUMMARY:Radio recombination lines: Theory and observations 射电复合线：理论与观测 URL;TYPE=URI:/info/1024/8535.htm END:VEVENT BEGIN:VEVENT UID:8573@kiaa.pku.edu.cn DTSTAMP:20220914T133726Z CREATED:20220914T133726Z DESCRIPTION:National Day Holiday DTSTART;TZID=Asia/Shanghai:20221001T000026 DTEND;TZID=Asia/Shanghai:20221003T000026 LAST-MODIFIED:20220914T133726Z LOCATION: SUMMARY:National Day Holidays URL;TYPE=URI:/info/1089/8573.htm END:VEVENT BEGIN:VEVENT UID:8613@kiaa.pku.edu.cn DTSTAMP:20221007T094425Z CREATED:20221007T094425Z DESCRIPTION:Abstract: The feedback of massive stars and clusters, such as radiation, wind, and supernovae, accounts for most of the energy budget in galaxies. However, our understanding of massive stars and cluster formation, especially the early evolutionary stages is still poor. The early evolutionary phases are crucial for understanding the initial conditions of massive star and cluster formation. Massi... DTSTART;TZID=Asia/Shanghai:20221011T133000 DTEND;TZID=Asia/Shanghai:20221011T143000 LAST-MODIFIED:20221007T094425Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Shining in the Darkness (在黑暗中闪闪发光) — The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES) URL;TYPE=URI:/info/1025/8613.htm END:VEVENT BEGIN:VEVENT UID:8594@kiaa.pku.edu.cn DTSTAMP:20220928T102553Z CREATED:20220928T102553Z DESCRIPTION:As the importance of gravitational wave (GW) astrophysics increases rapidly, astronomers interested in GWs who are not experts in this field sometimes need to get a quick idea of what GW sources can be detected by certain detectors, and the accuracy of the measured parameters. The GW-Toolbox is a set of easy-to-use, flexible tools to simulate observations of the GW universe with different detec... DTSTART;TZID=Asia/Shanghai:20221013T153000 DTEND;TZID=Asia/Shanghai:20221013T163000 LAST-MODIFIED:20220928T102553Z LOCATION:Join Zoom Meeting https://zoom.us/j/87037404550?pwd=UUtwQjQwTXNpaS9ObVJEQ3dJc2Yxdz09 Meeting ID: 870 3740 4550 Passcode: 299788 SUMMARY:Gravitational wave Universe toolbox 引力波宇宙工具箱 URL;TYPE=URI:/info/1024/8594.htm END:VEVENT BEGIN:VEVENT UID:8590@kiaa.pku.edu.cn DTSTAMP:20220920T173216Z CREATED:20220920T173216Z DESCRIPTION:Abstract: This talk explores whether gravitational waves (GWs) from neutron star (NS) mountains can be detected with current 2nd-generation and future 3rd-generation GW detectors. In particular, we focus on a scenario where transient mountains are formed immediately after a glitch. In a glitch, the NS's spin frequency abruptly increases and then often exponentially relaxes back to, but never qu... DTSTART;TZID=Asia/Shanghai:20221018T133000 DTEND;TZID=Asia/Shanghai:20221018T142000 LAST-MODIFIED:20220920T173216Z LOCATION:KIAA first meeting room, with also online zoom session Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Transient gravitational waves from pulsar post-glitch recoveries URL;TYPE=URI:/info/1025/8590.htm END:VEVENT BEGIN:VEVENT UID:8595@kiaa.pku.edu.cn DTSTAMP:20220928T103609Z CREATED:20220928T103609Z DESCRIPTION:As fuel of star formation, the cold gas plays an important role in the evolution of galaxies. In this talk, I will briefly introduce our recent work on estimating the amount of cold gas in star-forming and quenched galaxies, as well as how it regulates the star formation processes. We took advantange of the completed ALFALFA survey and stacked the atomic neutral hydrogen (HI) spectra to obtain ... DTSTART;TZID=Asia/Shanghai:20221020T153000 DTEND;TZID=Asia/Shanghai:20221020T163000 LAST-MODIFIED:20220928T103609Z LOCATION:Join Zoom Meeting https://zoom.us/j/84352288927?pwd=U2N6MHZGcTZUWDhUcmIxS1pWMk9Hdz09 Meeting ID: 843 5228 8927 Passcode: 004061 SUMMARY:The Role of Cold Gas in the Star formation and Quenching of Central Galaxies URL;TYPE=URI:/info/1024/8595.htm END:VEVENT BEGIN:VEVENT UID:8623@kiaa.pku.edu.cn DTSTAMP:20221024T145120Z CREATED:20221024T145120Z DESCRIPTION:GO Program超大质量黑洞和活动星系核观测前景综述A Summary on the Category of "Supermassive Black Holes and AGN" in the Cycle 1 GO Program of JWSTThe James Webb Space Telescope (JWST) has already started its science operations in the summer of 2022. The Cycle 1 General Observers (GO) program provides the opportunity for studies of supermassive black holes (SMBH) and AGN at high redshift (z$\gtrsim... DTSTART;TZID=Asia/Shanghai:20221025T093020 DTEND;TZID=Asia/Shanghai:20221025T110020 LAST-MODIFIED:20221024T145120Z LOCATION:KIAA 1st Meeting Room https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】GO Program超大质量黑洞和活动星系核观测前景综述 URL;TYPE=URI:/info/1259/8623.htm END:VEVENT BEGIN:VEVENT UID:8593@kiaa.pku.edu.cn DTSTAMP:20220923T152438Z CREATED:20220923T152438Z DESCRIPTION:Abstract:Strong magnetic fields could exist in the inner region of the explosive astrophysical site, such as MHD-Jet SNe. The phase space of the electrons is quantized inside the magnetic field so that the weak interaction rates deviate from the field-free case. This talk focuses on the (anti)neutrinos absorption process. This process is essential since it determines the opacity of the neutrin... DTSTART;TZID=Asia/Shanghai:20221025T133000 DTEND;TZID=Asia/Shanghai:20221025T140000 LAST-MODIFIED:20220923T152438Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Strong magnetic field impact on the neutrino process inside SNe explosion URL;TYPE=URI:/info/1025/8593.htm END:VEVENT BEGIN:VEVENT UID:8537@kiaa.pku.edu.cn DTSTAMP:20220830T091349Z CREATED:20220830T091349Z DESCRIPTION:Electron capture supernovae (ECSNe) are considered the main source of low-velocity neutron stars, which in turn are important for the formation of double neutron star systems. I will review recent work  suggesting that a large fraction of ECSNe may produce thermonuclear explosions instead of neutron stars. I will then discuss how a subset of core-collapse supernovae with subsonic ejecta may ser... DTSTART;TZID=Asia/Shanghai:20221027T153000 DTEND;TZID=Asia/Shanghai:20221027T163000 LAST-MODIFIED:20220830T091349Z LOCATION:Join Zoom Meeting https://zoom.us/j/89101255446?pwd=UTl1c2hOVnJYcnJnek1WZUozUjJmZz09 Meeting ID: 891 0125 5446 Passcode: 709491 SUMMARY:Are Electron capture supernovae the primary source of low-velocity neutron stars? URL;TYPE=URI:/info/1024/8537.htm END:VEVENT BEGIN:VEVENT UID:8621@kiaa.pku.edu.cn DTSTAMP:20221024T152804Z CREATED:20221024T152804Z DESCRIPTION:Schedule:9:30-9:40Welcome speechProf. Xian ChenChair: Zhenwei Lyu9:40-10:00Pulsar Timing Arrays and Massive Black HolesSiyuan Chen10:00-10:20Gravitational Waves from Pulsar Timing IrregularitiesGarvin Yim10:20-10:40Multi-messenger Detectability of Binary Neutron Star MergerHaoxiang Lin10:40-10:50Coffee breakChair: Dicong Liang10:50-11:10Heavy Elements from Neutron Star MergersYudong Luo11:10-11... DTSTART;TZID=Asia/Shanghai:20221029T093004 DTEND;TZID=Asia/Shanghai:20221029T153004 LAST-MODIFIED:20221024T152804Z LOCATION:First Meeting Room (1st floor) at KIAA SUMMARY:The Postdoc Workshop on Gravitational Waves at KIAA - Fall 2022 URL;TYPE=URI:/info/1026/8621.htm END:VEVENT BEGIN:VEVENT UID:8642@kiaa.pku.edu.cn DTSTAMP:20221027T144007Z CREATED:20221027T144007Z DESCRIPTION:莱曼连续谱星系的搜寻及其性质的研究The searching of Lyman continuum galaxies and their propertiesLyman continnum (LyC) photons (rest-frame λ<912 angstrom ), which are produced by OB stars in star-forming galaxies or active super-massive black holes (AGNs), can ionize the neutral hydrogen gas. The ionizing radiation which escapes into the IGM contributes either to the reionization at z>6 or to k... DTSTART;TZID=Asia/Shanghai:20221101T093000 DTEND;TZID=Asia/Shanghai:20221101T110000 LAST-MODIFIED:20221027T144007Z LOCATION:KIAA 1st Meeting Room https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】莱曼连续谱星系的搜寻及其性质的研究 URL;TYPE=URI:/info/1259/8642.htm END:VEVENT BEGIN:VEVENT UID:8622@kiaa.pku.edu.cn DTSTAMP:20221025T165915Z CREATED:20221025T165915Z DESCRIPTION:Abstract: We use Gaia DR3 data to study the Collinder 132–Gulliver 21 region via the machine-learning algorithm STARGO and find eight subgroups of stars (ASCC 32, Collinder 132 gp 1–6, Gulliver 21) located in close proximity. Three comoving populations were identified among these eight subgroups: (i) a coeval 25 Myr old moving group (Collinder 132), (ii) an intermediate-age (50–100 Myr) grou... DTSTART;TZID=Asia/Shanghai:20221101T133000 DTEND;TZID=Asia/Shanghai:20221101T141500 LAST-MODIFIED:20221025T165915Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Dynamical Origin for the Collinder 132–Gulliver 21 Stream: A Mixture of Three Comoving Populations with an Age Difference of 250Myr URL;TYPE=URI:/info/1025/8622.htm END:VEVENT BEGIN:VEVENT UID:8596@kiaa.pku.edu.cn DTSTAMP:20220928T110905Z CREATED:20220928T110905Z DESCRIPTION:Understanding the evolution of structure formation in the young Universe remains one of the outstanding challenges for modern astronomy. By observing the Universe at longer FIR-to-cm wavelengths we can obtain a unique perspective on the growth of massive galaxies at high-redshift. Powerful radio galaxies have long been known to act as the sign posts for over-dense regions when the Universe was ... DTSTART;TZID=Asia/Shanghai:20221103T153000 DTEND;TZID=Asia/Shanghai:20221103T163000 LAST-MODIFIED:20220928T110905Z LOCATION:Join Zoom Meeting https://zoom.us/j/83754398263?pwd=bjJFYjhLd3hZeWtFYzVjdW5jamx1UT09 Meeting ID: 837 5439 8263 Passcode: 692403 SUMMARY:The Radio Galaxy Environment Reference Survey URL;TYPE=URI:/info/1024/8596.htm END:VEVENT BEGIN:VEVENT UID:8650@kiaa.pku.edu.cn DTSTAMP:20221106T110914Z CREATED:20221106T110914Z DESCRIPTION:用JWST积分视场光谱仪研究深场Researching Deep Fields with JWST Integral Field SpectroscopyWith the instruments of extraordinary capabilities, the James Webb Space Telescope(JWST) will expand the boundary of near-IR and mid-IR astronomy. JWST is equipped with the Integral Field Spectroscopy (IFS), which has the ability to obtain resolved spectrum of high quality and has never been used on previo... DTSTART;TZID=Asia/Shanghai:20221108T093000 DTEND;TZID=Asia/Shanghai:20221108T110000 LAST-MODIFIED:20221106T110914Z LOCATION:KIAA 1st Meeting Room https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】用JWST积分视场光谱仪研究深场 URL;TYPE=URI:/info/1259/8650.htm END:VEVENT BEGIN:VEVENT UID:8630@kiaa.pku.edu.cn DTSTAMP:20221103T164109Z CREATED:20221103T164109Z DESCRIPTION:Abstract:Recent gravitational wave observations allow us to probe gravity in the strong and dynamical field regime. In this work, we focus on testing Einstein-dilation Gauss-Bonnet gravity which is motivated by string theory. In particular, we use two new neutron star black hole binaries (GW200105 and GW200115). Adopting the leading post-Newtonian correction and carrying out a Bayesian Markov-c... DTSTART;TZID=Asia/Shanghai:20221108T133000 DTEND;TZID=Asia/Shanghai:20221108T142000 LAST-MODIFIED:20221103T164109Z LOCATION:KIAA first meeting room, with also online zoom session Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Constraints on Einstein-dilation-Gauss-Bonnet gravity from black hole-neutron star gravitational wave events URL;TYPE=URI:/info/1025/8630.htm END:VEVENT BEGIN:VEVENT UID:8538@kiaa.pku.edu.cn DTSTAMP:20220830T091543Z CREATED:20220830T091543Z DESCRIPTION:Meteorites display an isotopic composition dichotomy between non-carbonaceous (NC) and carbonaceous (CC) groups, indicating that planetesimal formation in the solar protoplanetary disk occurred in two distinct reservoirs. A new model will be introduced to explain this dichotomy from the circumstance that the arrival of the outer CC dust particles in the inner disk is delayed for several million... DTSTART;TZID=Asia/Shanghai:20221110T153000 DTEND;TZID=Asia/Shanghai:20221110T163000 LAST-MODIFIED:20220830T091543Z LOCATION:Join Zoom Meeting https://zoom.us/j/86453322468?pwd=NVVHV0ZWMkNJWExvOWw5TE5qWFd1dz09 Meeting ID: 864 5332 2468 Passcode: 258990 SUMMARY:Setting the stage for the Solar System formation URL;TYPE=URI:/info/1024/8538.htm END:VEVENT BEGIN:VEVENT UID:8651@kiaa.pku.edu.cn DTSTAMP:20221111T133351Z CREATED:20221111T133351Z DESCRIPTION:AbstractUnderstanding the physics of the interstellar medium is critical for understanding star formation, its feedback, and AGN feedback. Line ratio diagnostics diagrams, such as BPT diagrams, have been extensively used to study the ISM. However, their limitations hide inaccuracies of photoionization models, leading to a number of discrepant results in the literature on metallicity, abundance... DTSTART;TZID=Asia/Shanghai:20221114T133000 DTEND;TZID=Asia/Shanghai:20221114T143000 LAST-MODIFIED:20221111T133351Z LOCATION:Hybrid mode (in person & zoom) Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Towards Precision Astrophysics for Warm Ionized Gas通向热电离气体的精确天体物理学 URL;TYPE=URI:/info/1025/8651.htm END:VEVENT BEGIN:VEVENT UID:8624@kiaa.pku.edu.cn DTSTAMP:20221111T133105Z CREATED:20221111T133105Z DESCRIPTION:SDSS-MaNGA:利用IFU统计数据研究附近星系恒星形成以及恒星动力学结构)SDSS-MaNGA: statistical IFU data for revealing SF and stellar kinematics in neaby galaxiesAs one of the most well-known sky surveies in the world, SDSS have been continuously observing the skies for roughly 20yr from 1998. The Mapping Nearby Galaxies at APO(MaNGA) survey is one of the three main surveies during the fourth phase o... DTSTART;TZID=Asia/Shanghai:20221115T093000 DTEND;TZID=Asia/Shanghai:20221115T110000 LAST-MODIFIED:20221111T133105Z LOCATION:KIAA 1st Meeting Room https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】SDSS-MaNGA:利用IFU统计数据研究附近星系恒星形成以及恒星动力学结构 URL;TYPE=URI:/info/1259/8624.htm END:VEVENT BEGIN:VEVENT UID:8611@kiaa.pku.edu.cn DTSTAMP:20221004T164410Z CREATED:20221004T164410Z DESCRIPTION:AbstractMass accretion is a fundamental process for the growth of supermassive black holes and activating the central engine. However, detailed accretion properties have not been observationally identified at the central ~10 parsec of active galaxies due to its compactness. Here we for the first time ever report the direct detection of parsec-scale (i.e., 0.01% scale of the host galaxy) dense ... DTSTART;TZID=Asia/Shanghai:20221115T133000 DTEND;TZID=Asia/Shanghai:20221115T140000 LAST-MODIFIED:20221004T164410Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Resolving supermassive black hole feeding and feedback: multiphase flows down to sub-parsec URL;TYPE=URI:/info/1025/8611.htm END:VEVENT BEGIN:VEVENT UID:8641@kiaa.pku.edu.cn DTSTAMP:20221104T142258Z CREATED:20221104T142258Z DESCRIPTION:Self-consistent radiation transfer and hydrodynamics is a very important but still under-explored field in computational astrophysics. In this talk, I will discuss some of the basic concepts of radiation hydrodynamics and equation of state (EoS). I will also present a novel 2D code, Guangqi, that can solve radiation hydrodynamics with a realistic EoS self-consistently. The code is thoroughly te... DTSTART;TZID=Asia/Shanghai:20221117T153000 DTEND;TZID=Asia/Shanghai:20221117T163000 LAST-MODIFIED:20221104T142258Z LOCATION:Zoom Link: https://zoom.us/j/83104709301?pwd=NW1QTlhCZmJJbXBXaXVWdE9pUkgzQT09 Meeting ID: 831 0470 9301 Passcode: 652434 SUMMARY:Radiation hydrodynamics and its prospects in planet formation and stellar evolution URL;TYPE=URI:/info/1024/8641.htm END:VEVENT BEGIN:VEVENT UID:8660@kiaa.pku.edu.cn DTSTAMP:20221117T103609Z CREATED:20221117T103609Z DESCRIPTION:产生星系样本来对星系巡天进行预研究Generate galaxy populations to forecast galaxy surveysModeling galaxy formation and evolution presents one of the greatest challenges in modern astrophysics due to its multiscale and multiphysics character. In past decades, tremendous progress has been made toward deep insights into these complex processes, with the help of large amounts of observational data ... DTSTART;TZID=Asia/Shanghai:20221122T093000 DTEND;TZID=Asia/Shanghai:20221122T110000 LAST-MODIFIED:20221117T103609Z LOCATION:KIAA 1st Meeting Room https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】产生星系样本来对星系巡天进行预研究 URL;TYPE=URI:/info/1259/8660.htm END:VEVENT BEGIN:VEVENT UID:8661@kiaa.pku.edu.cn DTSTAMP:20221118T164841Z CREATED:20221118T164841Z DESCRIPTION:Abstract: AliCPT-1 is the first Chinese CMB experiment aiming for high precision measurement of Cosmic Microwave Background B-mode polarization. The telescope, currently under deployment in Tibet, will observe in two frequency bands centered at 90 and 150 GHz. Currently the telescope is under construction and will start observation in 2023. In this talk, I will present the design and progress o... DTSTART;TZID=Asia/Shanghai:20221122T133000 DTEND;TZID=Asia/Shanghai:20221122T143000 LAST-MODIFIED:20221118T164841Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:AliCPT1: Design and Progress and kinetic inductance detectors 阿里原初引力波探测项目和动态电感探测器 URL;TYPE=URI:/info/1025/8661.htm END:VEVENT BEGIN:VEVENT UID:8542@kiaa.pku.edu.cn DTSTAMP:20220830T092900Z CREATED:20220830T092900Z DESCRIPTION:Planets form in protoplanetary disks surrounding newborn stars. As such, the most direct way to learn how they form from observations, is to observe them forming in disks. Thanks to a fleet of new instruments with unprecedented resolving power that have come online in the past decade, we have started to unveil features in imaging observations of protoplanetary disks, such as gaps and spiral arm... DTSTART;TZID=Asia/Shanghai:20221124T153000 DTEND;TZID=Asia/Shanghai:20221124T163000 LAST-MODIFIED:20220830T092900Z LOCATION:https://zoom.us/j/86079618428?pwd=Y2lMK3Ztd3RhcE9nN1Z4cGdYMmpHZz09 Meeting ID: 860 7961 8428 Passcode: 051366 SUMMARY:Deciphering planet formation signals in protoplanetary disks URL;TYPE=URI:/info/1024/8542.htm END:VEVENT BEGIN:VEVENT UID:8670@kiaa.pku.edu.cn DTSTAMP:20221127T132920Z CREATED:20221127T132920Z DESCRIPTION:关于暗能量光谱巡天项目的概述：从巡天到科学Overview of the Dark Energy Spectroscopic instrument (DESI): From survey to scienceAiming to explore the nature of dark energy, the Dark Energy Spectroscopic Instrument (DESI) is conducting a five-year massive survey to map the large structure of universe over one third of the sky and 11 billion years, with a powerful 5000-fiber multi-object optical sp... DTSTART;TZID=Asia/Shanghai:20221129T093000 DTEND;TZID=Asia/Shanghai:20221129T110000 LAST-MODIFIED:20221127T132920Z LOCATION:online only https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】关于暗能量光谱巡天项目的概述：从巡天到科学 URL;TYPE=URI:/info/1259/8670.htm END:VEVENT BEGIN:VEVENT UID:8610@kiaa.pku.edu.cn DTSTAMP:20221004T161059Z CREATED:20221004T161059Z DESCRIPTION:Abstract:After five years of operation, the GRAVITY instrument has enabled a major step forward in infrared interferometry by its high spatial resolution and sensitivity. This talk will provide an overview of GRAVITY's technology and observation capabilities. I will highlight some revolutionary science results of the Galactic Center, exoplanet, and active galactic nuclei (AGNs). A particular fo... DTSTART;TZID=Asia/Shanghai:20221129T133000 DTEND;TZID=Asia/Shanghai:20221129T140000 LAST-MODIFIED:20221004T161059Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Near-infrared Interferometry Science with VLTI/GRAVITY URL;TYPE=URI:/info/1025/8610.htm END:VEVENT BEGIN:VEVENT UID:8541@kiaa.pku.edu.cn DTSTAMP:20220830T092250Z CREATED:20220830T092250Z DESCRIPTION:Pulsars and Fast Radio Bursts (FRB) are some of the most energetic and "fast" objects in radio astronomy. They are both possibly from "neutron stars". In this talk, I will introduce some of my group and collaborators' pulsars and FRB research using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). I will talk about the discovery and timing of new pulsars, testing theories of gra... DTSTART;TZID=Asia/Shanghai:20221201T153000 DTEND;TZID=Asia/Shanghai:20221201T163000 LAST-MODIFIED:20220830T092250Z LOCATION:Join Zoom Meeting https://zoom.us/j/88922686623?pwd=VEs2amdHbnFFQjUyWWROZXF1bFFjUT09 Meeting ID: 889 2268 6623 Passcode: 823104 SUMMARY:Pulsar and Fast Radio Burst study using FAST 基于FAST的一些脉冲星和快速射电暴研究 URL;TYPE=URI:/info/1024/8541.htm END:VEVENT BEGIN:VEVENT UID:8690@kiaa.pku.edu.cn DTSTAMP:20221205T095955Z CREATED:20221205T095955Z DESCRIPTION:模拟中的暗物质晕对星系性质的影响Dark matter halo-galaxy connection in simulationsIn the current concordance  CDM paradigm, galaxies form and evolve in dark matter haloes, so the halo-galaxy connection is crucial for understanding the underlying physical processes and constraining cosmological models. However, due to the dissipationless nature of dark matter, it is extremely hard to directly ... DTSTART;TZID=Asia/Shanghai:20221206T093000 DTEND;TZID=Asia/Shanghai:20221206T110000 LAST-MODIFIED:20221205T095955Z LOCATION:online only https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】模拟中的暗物质晕对星系性质的影响 URL;TYPE=URI:/info/1259/8690.htm END:VEVENT BEGIN:VEVENT UID:8680@kiaa.pku.edu.cn DTSTAMP:20221201T174659Z CREATED:20221201T174659Z DESCRIPTION:Abstract:We propose a scenario where superheavy dark matter (DM) can be produced via symmetry restoration first-order phase transition during inflation triggered by the evolution of the inflaton field. The phase transition happens in a spectator sector coupled to the inflaton field. During the phase transition, the spectator field tunnels from a symmetry-broken vacuum to a symmetry-restored vac... DTSTART;TZID=Asia/Shanghai:20221206T133000 DTEND;TZID=Asia/Shanghai:20221206T142000 LAST-MODIFIED:20221201T174659Z LOCATION:Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Superheavy Dark Matter Production from Symmetry Restoration First-Order Phase Transition During Inflation URL;TYPE=URI:/info/1025/8680.htm END:VEVENT BEGIN:VEVENT UID:8540@kiaa.pku.edu.cn DTSTAMP:20220830T092037Z CREATED:20220830T092037Z DESCRIPTION:Cosmic reionization marks the latest phase transition of the IGM in the early Universe. High-redshift (redshift around 6 or higher) quasars and galaxies are powerful tools to probe this epoch. I will review how the absorption spectra of quasars and the statistical properties of galaxies (particularly Lyman-alpha emitting galaxies) are used to estimate the IGM state during the reionization epoch... DTSTART;TZID=Asia/Shanghai:20221208T153000 DTEND;TZID=Asia/Shanghai:20221208T163000 LAST-MODIFIED:20220830T092037Z LOCATION:Join Zoom Meeting https://zoom.us/j/84019952918?pwd=V09zK2YyL1VWMzZLTmkrQ1NZanNEQT09 Meeting ID: 840 1995 2918 Passcode: 733052 SUMMARY:Probing cosmic reionization using high-redshift quasars and galaxies 利用高红移星系和类星体探测宇宙再电离 URL;TYPE=URI:/info/1024/8540.htm END:VEVENT BEGIN:VEVENT UID:8700@kiaa.pku.edu.cn DTSTAMP:20221209T112217Z CREATED:20221209T112217Z DESCRIPTION:Abstract:Compact objects (white dwarfs, neutron stars, or black holes) are stellar 'fossils' bearing critical information about the Galactic stellar evolutionary history. In binary systems, hidden compact objects can be revealed by monitoring the 'wobbling' effect of the visible companion star. We utilise efficient wide-field spectroscopic surveys like LAMOST (a.k.a. the GuoShouJing telescope) ... DTSTART;TZID=Asia/Shanghai:20221213T133000 DTEND;TZID=Asia/Shanghai:20221213T141000 LAST-MODIFIED:20221209T112217Z LOCATION:Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Hidden compact objects revealed by wide-field optical surveys URL;TYPE=URI:/info/1025/8700.htm END:VEVENT BEGIN:VEVENT UID:8543@kiaa.pku.edu.cn DTSTAMP:20220830T093144Z CREATED:20220830T093144Z DESCRIPTION:Galaxies are living in complex cosmic ecosystem which is composed of dark matter and baryonic matter. The baryon cycle through hot gaseous halo, circumgalactic medium and inter-stellar medium is important for galaxy formation and evolution while the detail of the cycle is not very clear. In this talk, I will present our empirical model to constrain the baryon cycle process in galaxy formation a... DTSTART;TZID=Asia/Shanghai:20221215T153000 DTEND;TZID=Asia/Shanghai:20221215T163000 LAST-MODIFIED:20220830T093144Z LOCATION:Join Zoom Meeting https://zoom.us/j/84140171908?pwd=ZnJQZXY1QnZmaXA5anNYMXRxOVEzUT09 Meeting ID: 841 4017 1908 Passcode: 478479 SUMMARY:Baryon Cycle in Galaxy Formation 星系形成中的重子循环 URL;TYPE=URI:/info/1024/8543.htm END:VEVENT BEGIN:VEVENT UID:8703@kiaa.pku.edu.cn DTSTAMP:20221215T170638Z CREATED:20221215T170638Z DESCRIPTION:Abstract:We propose a physical process to use a Schwarzschild black hole as a rechargeable battery and nuclear reactor. As a rechargeable battery, it can at most transform 25% of input mass into available electric energy in a controllable and slow way. We study its internal resistance, efficiency of discharging, maximum output power, cycle life and totally available energy. As a nuclear reactor... DTSTART;TZID=Asia/Shanghai:20221220T133000 DTEND;TZID=Asia/Shanghai:20221220T142000 LAST-MODIFIED:20221215T170638Z LOCATION:Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Using black holes as rechargable batteries and nuclear reactors URL;TYPE=URI:/info/1025/8703.htm END:VEVENT BEGIN:VEVENT UID:8544@kiaa.pku.edu.cn DTSTAMP:20220830T093314Z CREATED:20220830T093314Z DESCRIPTION:Up to today, more than 5000 exoplanets have been detected and confirmed. Among them, about 60 are habitable Earth-like planets. It is expected that the ongoing and future space-borne planet survey missions including TESS, PLATO will detect thousands of small to medium-sized planets via the transit technique, including over a hundred habitable terrestrial rocky planets. To conduct a detailed atm... DTSTART;TZID=Asia/Shanghai:20221222T153000 DTEND;TZID=Asia/Shanghai:20221222T163000 LAST-MODIFIED:20220830T093314Z LOCATION:https://zoom.us/j/86726957916?pwd=S3lCc3BGaWRDRlVKc2JsRlppM2pXdz09 Meeting ID: 867 2695 7916 Passcode: 314131 SUMMARY:From exoplanet atmospheres to extraterrestrial life URL;TYPE=URI:/info/1024/8544.htm END:VEVENT BEGIN:VEVENT UID:8705@kiaa.pku.edu.cn DTSTAMP:20221223T234257Z CREATED:20221223T234257Z DESCRIPTION:HSC-SSP：高分辨率深场巡天HSC-SSP: A deep, high-resolution surveyThe Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered, multiband (grizy plus 4 narrow-band filters) imaging survey using the Hyper Suprime-Cam (HSC) on the 8.2m Subaru Telescope. The wide layer covers 1,400 degrees squared around the equator and reaches a depth of 26 mag in r-band, and the deep and ultradeep... DTSTART;TZID=Asia/Shanghai:20221227T093000 DTEND;TZID=Asia/Shanghai:20221227T110000 LAST-MODIFIED:20221223T234257Z LOCATION:online only https://meeting.tencent.com/dm/SQEllZOIDE7s 腾讯会议：940-6639-5711 SUMMARY:【CSST Discussion】HSC-SSP：高分辨率深场巡天 URL;TYPE=URI:/info/1259/8705.htm END:VEVENT BEGIN:VEVENT UID:8640@kiaa.pku.edu.cn DTSTAMP:20221104T104043Z CREATED:20221104T104043Z DESCRIPTION:Abstract:The molecular gas in the host galaxies of the quasars at high redshift reveals key aspects in the formation and evolution of the SMBHs and their hosts at the early evolutionary stage. The CO spectral energy distributions (SLEDs) serve as powerful diagnostics of the physical conditions as well as heating mechanisms of the molecular gas, e.g., the photo-dissociation regions (PDRs),... DTSTART;TZID=Asia/Shanghai:20221227T133000 DTEND;TZID=Asia/Shanghai:20221227T143000 LAST-MODIFIED:20221104T104043Z LOCATION:Online Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Probing the molecular gas excitations in two quasar host galaxies at z~6 URL;TYPE=URI:/info/1025/8640.htm END:VEVENT BEGIN:VEVENT UID:8574@kiaa.pku.edu.cn DTSTAMP:20220914T133943Z CREATED:20220914T133943Z DESCRIPTION:Winter Holiday DTSTART;TZID=Asia/Shanghai:20230102T000043 DTEND;TZID=Asia/Shanghai:20230219T000043 LAST-MODIFIED:20220914T133943Z LOCATION: SUMMARY:Winter Holidays URL;TYPE=URI:/info/1089/8574.htm END:VEVENT BEGIN:VEVENT UID:8720@kiaa.pku.edu.cn DTSTAMP:20230217T101107Z CREATED:20230217T101107Z DESCRIPTION:Abstract: The origin of cosmic rays and neutrinos with ultra-high energy ( > 10^18eV) remains mysterious for more than half a century after the first observation. Radio detection of air showers induced by them is considered the technique for next-generation experiments with its low cost and unprecedented sensitivity. More and more experiments (GRAND, BEACON, TRINITY) attempt to detect upward-go... DTSTART;TZID=Asia/Shanghai:20230221T133000 DTEND;TZID=Asia/Shanghai:20230221T141500 LAST-MODIFIED:20230217T101107Z LOCATION:Hybird Meeting: KIAA, First Meeting Room Zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:New mechanism and simulation tools in radio detection of air showers induced by UHE cosmic rays and neutrinos URL;TYPE=URI:/info/1025/8720.htm END:VEVENT BEGIN:VEVENT UID:8723@kiaa.pku.edu.cn DTSTAMP:20230219T131009Z CREATED:20230219T131009Z DESCRIPTION:Abstract: Cosmic reionization corresponds to the milestone of the Universe where theintergalactic medium transitions from primarily neutral, dark, and cold into mainly ionized, moreluminous, and warmer. During this transition, the intergalactic medium is violently heated andripples from the additional injected energy can be seen millions of years after this milestone.However, estimates of the... DTSTART;TZID=Asia/Shanghai:20230223T120000 DTEND;TZID=Asia/Shanghai:20230223T130000 LAST-MODIFIED:20230219T131009Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Nailing down the evolution of the IGM in the post-reionization era through high-resolution Simulations URL;TYPE=URI:/info/1025/8723.htm END:VEVENT BEGIN:VEVENT UID:8722@kiaa.pku.edu.cn DTSTAMP:20230219T130154Z CREATED:20230219T130154Z DESCRIPTION:Abstract: Star formation history (SFH) is important in a galaxy’s formation and evolution. It affects the shape, mass, metallicity, color, and many other properties of a galaxy. And it also encodes the physics which drives the galaxy evolution. Retrieving the SFH of galaxies is always a critical issue in the research of galaxy formation. This is a tough task due to the complexities and uncert... DTSTART;TZID=Asia/Shanghai:20230223T120000 DTEND;TZID=Asia/Shanghai:20230223T130000 LAST-MODIFIED:20230219T130154Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Reproduce the star formation history of galaxies from simulations URL;TYPE=URI:/info/1025/8722.htm END:VEVENT BEGIN:VEVENT UID:8721@kiaa.pku.edu.cn DTSTAMP:20230219T124406Z CREATED:20230219T124406Z DESCRIPTION:Abstract: Rapid advances in deep learning have brought not only myriad powerful neural networks, but also breakthroughs that benefit established scientific research. In particular, automatic differentiation (AD) tools and computational accelerators like GPUs have facilitated forward modeling of the Universe with differentiable simulations. Current differentiable cosmological simulations are li... DTSTART;TZID=Asia/Shanghai:20230223T120000 DTEND;TZID=Asia/Shanghai:20230223T122000 LAST-MODIFIED:20230219T124406Z LOCATION:KIAA 1st meeting room + zoom Meeting ID: 822 8287 7472 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/82282877472?pwd=VXFOYmtaRUhZMVplYWp1OFQ4OGsvQT09 SUMMARY:Differentiable Cosmological Simulation with Adjoint Method URL;TYPE=URI:/info/1025/8721.htm END:VEVENT BEGIN:VEVENT UID:8724@kiaa.pku.edu.cn DTSTAMP:20230219T230430Z CREATED:20230219T230430Z DESCRIPTION:The stellar IMF is one of the most important astrophysical distribution and plays vital role in galactic astronomy. Both constant and variable IMFs across different environments have been claimed despite a large number of theoretical and observational efforts. However, the measurement of the IMF in Galactic stellar populations has been limited by the relatively small number of photometrically o... DTSTART;TZID=Asia/Shanghai:20230223T153000 DTEND;TZID=Asia/Shanghai:20230223T163000 LAST-MODIFIED:20230219T230430Z LOCATION:KIAA-Auditorium SUMMARY:The variation of the stellar initial mass function (IMF) with metallicity and time 恒星初始质量函数（IMF）随金属丰度和时间变化 URL;TYPE=URI:/info/1024/8724.htm END:VEVENT BEGIN:VEVENT UID:8770@kiaa.pku.edu.cn DTSTAMP:20230224T234257Z CREATED:20230224T234257Z DESCRIPTION:星系模拟中的气体 Gas in simulations The gas in the Universe is in multi-phase. Some gas dissipates its internal energy through various cooling processes and eventually forms stars, while some is hotter than 10^7 K and remain in the surrounding of galaxies. Gas not only interacts with itself, but also with gravity, radiation, stars, AGN, and magnetic field. To deal with the gas component in sim... DTSTART;TZID=Asia/Shanghai:20230228T093000 DTEND;TZID=Asia/Shanghai:20230228T110000 LAST-MODIFIED:20230224T234257Z LOCATION:KIAA 1st meeting room https://meeting.tencent.com/dm/owyFu6OS3Rd7 腾讯会议：401-8779-0146 SUMMARY:【CSST Discussion】星系模拟中的气体 URL;TYPE=URI:/info/1259/8770.htm END:VEVENT BEGIN:VEVENT UID:8761@kiaa.pku.edu.cn DTSTAMP:20230227T095241Z CREATED:20230227T095241Z DESCRIPTION:Abstract:The speaker leads a line survey of TianMa 65 m radio teleacope (TMRT) aimimg to provide an unprecedently sensitive (mK) spectral template covering 1--50 GHz, in preparation for the forthcoming era of low-frequency radio interferometers (e.g., ALMA band 1, SKA). More than one thousand line features were detected from the already accomplished Ka/Q-band (26-50 GHz) pioneer surveys towards... DTSTART;TZID=Asia/Shanghai:20230228T133030 DTEND;TZID=Asia/Shanghai:20230228T140500 LAST-MODIFIED:20230227T095241Z LOCATION:Online Meeting: Zoom Meeting ID: 878 6573 2980 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 SUMMARY:Spectral Line Survey of TMRT in searching for COMs and RRLs URL;TYPE=URI:/info/1025/8761.htm END:VEVENT BEGIN:VEVENT UID:8725@kiaa.pku.edu.cn DTSTAMP:20230220T113835Z CREATED:20230220T113835Z DESCRIPTION:Discovery of pulsars is one of main goals for large radio telescopes. The Five-hundred-meter Aperture Spherical radio Tetelscope (FAST) has the largest collecting area for radio waves, with an aperture of 300~m in diameter. Mounted with the 19-beam L-band receiver with a system temperature of about 20 K, it is the most sensitive radio telescope. The Galactic Plane Pulsar Snapshot (GPPS) surve... DTSTART;TZID=Asia/Shanghai:20230302T153000 DTEND;TZID=Asia/Shanghai:20230302T163000 LAST-MODIFIED:20230220T113835Z LOCATION:KIAA-Auditorium SUMMARY:New results from the FAST Galactic Plane Pulsar Snapshot survey URL;TYPE=URI:/info/1024/8725.htm END:VEVENT BEGIN:VEVENT UID:8810@kiaa.pku.edu.cn DTSTAMP:20230306T104742Z CREATED:20230306T104742Z DESCRIPTION:GAMA巡天概述Overview of GAMA surveyThe Galaxy And Mass Assembly Survey (GAMA) began in 2008 with the goal of building upon the legacy of the original 2dFGRS and SDSS surveys to produce a highly complete redshift survey with maximal multiwavelength data (xray-to-radio via eROSITA, GALEX, VST, VISTA, WISE, Herschel, SKAP, and MWA). GAMA covers five fields with highly complete spectroscopic cove... DTSTART;TZID=Asia/Shanghai:20230307T093000 DTEND;TZID=Asia/Shanghai:20230307T110000 LAST-MODIFIED:20230306T104742Z LOCATION:KIAA 1st meeting room https://meeting.tencent.com/dm/owyFu6OS3Rd7 腾讯会议：401-8779-0146 SUMMARY:【CSST Discussion】GAMA巡天概述 URL;TYPE=URI:/info/1259/8810.htm END:VEVENT BEGIN:VEVENT UID:8760@kiaa.pku.edu.cn DTSTAMP:20230226T130952Z CREATED:20230226T130952Z DESCRIPTION:Abstract: The bimodal distribution of galaxies on the M_*-SFR plane implies a rapid transition from the state of star-forming to quiescence, which process is usually referred to as galaxy quenching. Previous studies have established that galaxy quenching is regulated by both internal and external processes. The internal quenching process is also known as mass quenching since it is primarily dep... DTSTART;TZID=Asia/Shanghai:20230307T133000 DTEND;TZID=Asia/Shanghai:20230307T143000 LAST-MODIFIED:20230226T130952Z LOCATION:hybrid (KIAA 1st meeting room + zoom), https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 Meeting ID: 878 6573 2980 Passcode: astroPKU SUMMARY:Central Galaxy Quenching and its relation to Large-scale Environment & Halo Formation Time URL;TYPE=URI:/info/1025/8760.htm END:VEVENT BEGIN:VEVENT UID:8726@kiaa.pku.edu.cn DTSTAMP:20230220T114015Z CREATED:20230220T114015Z DESCRIPTION:The cosmic acceleration, first probed by observations of SNIa in 1998, is one of the most significant discoveries in modern sciences. In the past 25 years, extensive studies have been performed to unveil the physical origin of this surprising phenomenon, including studies on dark energy and modified gravity. In this talk, I will report the latest progress in this field, and focus on cosmological implications of large galaxy surveys including eBOSS, DESI and PFS. DTSTART;TZID=Asia/Shanghai:20230309T153000 DTEND;TZID=Asia/Shanghai:20230309T163000 LAST-MODIFIED:20230220T114015Z LOCATION:KIAA-Auditorium SUMMARY:Understanding the cosmic acceleration with massive galaxy surveys 依托大规模星系巡天的宇宙加速膨胀机制研究 URL;TYPE=URI:/info/1024/8726.htm END:VEVENT BEGIN:VEVENT UID:8830@kiaa.pku.edu.cn DTSTAMP:20230312T105150Z CREATED:20230312T105150Z DESCRIPTION:数值模拟中黑洞的形成与演化Black hole formation and evolution in numerical simulationsObservations suggest that there is a supermassive black hole (SMBH) at the center of each galaxy. On the theoretical part, SMBHs are also required to explain the low efficiency of converting baryons into stars for massive galaxies. However, the formation and growth of SMBHs is still unresolved, especially for ... DTSTART;TZID=Asia/Shanghai:20230314T093000 DTEND;TZID=Asia/Shanghai:20230314T110000 LAST-MODIFIED:20230312T105150Z LOCATION:KIAA 1st meeting room https://meeting.tencent.com/dm/owyFu6OS3Rd7 腾讯会议：401-8779-0146 SUMMARY:【CSST Discussion】数值模拟中黑洞的形成与演化 URL;TYPE=URI:/info/1259/8830.htm END:VEVENT BEGIN:VEVENT UID:8821@kiaa.pku.edu.cn DTSTAMP:20230309T070000Z CREATED:20230309T070000Z DESCRIPTION:Abstract: Dark matter (DM) occupies the majority of matter content in the universe and is probably cold (CDM). However, modifications to the standard CDM model may be required by the small-scale observations, and DM may be self-interacting (SIDM), warm (WDM) or fuzzy (FDM). Here we show that the diffractive lensing of gravitational waves (GWs) from binary black hole mergers by small halos (∼ 1... DTSTART;TZID=Asia/Shanghai:20230314T133000 DTEND;TZID=Asia/Shanghai:20230314T143000 LAST-MODIFIED:20230309T070000Z LOCATION:hybrid (KIAA 1st meeting room + zoom), https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 Meeting ID: 878 6573 2980 Passcode: astroPKU SUMMARY:Probing the Nature of Dark Matter via Gravitational Waves Lensed by Small Dark Matter Halos URL;TYPE=URI:/info/1025/8821.htm END:VEVENT BEGIN:VEVENT UID:8727@kiaa.pku.edu.cn DTSTAMP:20230220T114219Z CREATED:20230220T114219Z DESCRIPTION:Measuring the mass and distance of a gravitational wave (GW) source is a fundamental problem in GW astronomy. The issue is becoming even more pressing since LIGO and Virgo have detected massive black holes that in the past were thought to be rare, if not entirely impossible. The waveform templates used in the detection are developed under the assumption that the sources are residing in a vacuum... DTSTART;TZID=Asia/Shanghai:20230316T153000 DTEND;TZID=Asia/Shanghai:20230316T163000 LAST-MODIFIED:20230220T114219Z LOCATION:KIAA-Auditorium SUMMARY:Impact of astrophysical environments on gravitational-wave detection and interpretation URL;TYPE=URI:/info/1024/8727.htm END:VEVENT BEGIN:VEVENT UID:8780@kiaa.pku.edu.cn DTSTAMP:20230228T134309Z CREATED:20230228T134309Z DESCRIPTION:Abstract:Understanding the thermal structure of protoplanetary disks (PPDs) is crucial for elucidating the formation of rocky planets and how the water abundance of planets is determined. We present 2D global radiative magnetohydrodynamic (MHD) simulations of the inner region of PPDs which take into account all three non-ideal MHD effects, irradiation, and Joule heating due to the global magne... DTSTART;TZID=Asia/Shanghai:20230321T133000 DTEND;TZID=Asia/Shanghai:20230321T143000 LAST-MODIFIED:20230228T134309Z LOCATION:KIAA 1st meeting room Zoom: Meeting ID: 878 6573 2980 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 SUMMARY:Radiative Nonideal MHD Simulations of the Inner Protoplanetary Disks URL;TYPE=URI:/info/1025/8780.htm END:VEVENT BEGIN:VEVENT UID:8841@kiaa.pku.edu.cn DTSTAMP:20230314T165813Z CREATED:20230314T165813Z DESCRIPTION:Postdoc Science Da DTSTART;TZID=Asia/Shanghai:20230322T090000 DTEND;TZID=Asia/Shanghai:20230322T180000 LAST-MODIFIED:20230314T165813Z LOCATION: SUMMARY:Postdoc Science Day URL;TYPE=URI:/info/1089/8841.htm END:VEVENT BEGIN:VEVENT UID:8728@kiaa.pku.edu.cn DTSTAMP:20230220T120048Z CREATED:20230220T120048Z DESCRIPTION:Relativistic jets are launched in the vicinity of the central black holes and emit powerful radiation across the electromagnetic spectrum. According to our current understanding, relativistic jets are launched by directly tapping the rotational energy of spinning black holes via the so-called Blandford-Znajek process. In addition to the spin of the black hole, numerical simulations showed the a... DTSTART;TZID=Asia/Shanghai:20230323T153000 DTEND;TZID=Asia/Shanghai:20230323T163000 LAST-MODIFIED:20230220T120048Z LOCATION:KIAA-Auditorium SUMMARY:Relativistic Jet Simulations and Modeling on Horizon Scale URL;TYPE=URI:/info/1024/8728.htm END:VEVENT BEGIN:VEVENT UID:8861@kiaa.pku.edu.cn DTSTAMP:20230327T103107Z CREATED:20230327T103107Z DESCRIPTION:几个SKAP巡天的概述：以HI为主Overview of Several SKAP Surveys: Focus on HIStudies of the atomic interstellar medium (ISM), using the 21 cm line of atomic hydrogen (HI), is crucial to understand many astronomical questions, such as the formation and evolution of galaxies. And Square Kilometre Array (SKA) gives us a unique combination of high sensitivity, high angular resolution and wide field o... DTSTART;TZID=Asia/Shanghai:20230328T093000 DTEND;TZID=Asia/Shanghai:20230328T110000 LAST-MODIFIED:20230327T103107Z LOCATION:KIAA 1st meeting room https://meeting.tencent.com/dm/owyFu6OS3Rd7 腾讯会议：401-8779-0146 SUMMARY:【CSST Discussion】几个SKAP巡天的概述：以HI为主 URL;TYPE=URI:/info/1259/8861.htm END:VEVENT BEGIN:VEVENT UID:8736@kiaa.pku.edu.cn DTSTAMP:20230220T160718Z CREATED:20230220T160718Z DESCRIPTION:Abstract: In this talk, I will overview my recent works on up-down quark matter and the associated new possible types of compact stars, such as up-down quark stars and the inverted hybrid stars that we termed ``cross stars” (CrSs). CrSs consist of a hadronic matter core and a quark matter crust, with an inverted structure compared to conventional hybrid stars. This distinct stellar structure n... DTSTART;TZID=Asia/Shanghai:20230328T133000 DTEND;TZID=Asia/Shanghai:20230328T143000 LAST-MODIFIED:20230220T160718Z LOCATION:KIAA 1st meeting room Zoom: Meeting ID: 878 6573 2980 , Passcode: astroPKU , Link: https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 SUMMARY:up-down quark stars and inverted hybrid stars URL;TYPE=URI:/info/1025/8736.htm END:VEVENT BEGIN:VEVENT UID:8737@kiaa.pku.edu.cn DTSTAMP:20230220T161012Z CREATED:20230220T161012Z DESCRIPTION:Gravitational wave astronomy is revolutionizing our understanding of the Universe. Since the historic discovery of GW150914 in 2015, ground-based interferometers have discovered over 90 compact binary coalescence events. These events, lasting from fractions of seconds to minutes, include stellar-mass binary black holes, binary neutron stars and neutron star-black hole binaries. Meanwhile, pulsa... DTSTART;TZID=Asia/Shanghai:20230330T150000 DTEND;TZID=Asia/Shanghai:20230330T160000 LAST-MODIFIED:20230220T161012Z LOCATION:KIAA-Auditorium SUMMARY:Gravitational wave astronomy: some investigations on binary neutron stars and supermassive binary black holes URL;TYPE=URI:/info/1024/8737.htm END:VEVENT BEGIN:VEVENT UID:8738@kiaa.pku.edu.cn DTSTAMP:20230220T161332Z CREATED:20230220T161332Z DESCRIPTION:Pulsars are fascinating stellar objects. Their nature being a celestial clock make them extremely sensitive probes to tiny perturbations in spacetime. In this talk, I will introduce two applications of pulsar to probe our theory of gravity under extreme physical conditions: Detecting low-frequency gravitational waves with a pulsar timing array (PTA), and measuring the properties of the supermas... DTSTART;TZID=Asia/Shanghai:20230330T160000 DTEND;TZID=Asia/Shanghai:20230330T170000 LAST-MODIFIED:20230220T161332Z LOCATION:KIAA-Auditorium SUMMARY:Experimenting with gravity under extreme physical conditions with pulsars URL;TYPE=URI:/info/1024/8738.htm END:VEVENT BEGIN:VEVENT UID:8881@kiaa.pku.edu.cn DTSTAMP:20230403T125857Z CREATED:20230403T125857Z DESCRIPTION:数值模拟中活动星系核的反馈作用AGN feedback in simulationsThe existence of SMBHs barbered at galaxy centers and the correlations between their masses and host galaxy properties across cosmic evolution has been challenging our outstanding of the formation and evolution of galaxies. It is widely believed that the feedback from SMBH activities (or feedback from active galactic nuclei, AGN) plays a ... DTSTART;TZID=Asia/Shanghai:20230404T093000 DTEND;TZID=Asia/Shanghai:20230404T110000 LAST-MODIFIED:20230403T125857Z LOCATION:KIAA 1st meeting room https://meeting.tencent.com/dm/owyFu6OS3Rd7 腾讯会议：401-8779-0146 SUMMARY:【CSST Discussion】AGN feedback in simulations (数值模拟中活动星系核的反馈作用) URL;TYPE=URI:/info/1259/8881.htm END:VEVENT BEGIN:VEVENT UID:8870@kiaa.pku.edu.cn DTSTAMP:20230330T101330Z CREATED:20230330T101330Z DESCRIPTION:Abstract: Recently, several major international pulsar timing array collaborations, including NANOGrav, PPTA, EPTA, and IPTA, have detected a common-spectrum process resembling a gravitational wave background in their latest data, indicating that pulsar timing arrays may soon detect gravitational waves in the nanohertz band. We will report some new developments in probing novel physics through ... DTSTART;TZID=Asia/Shanghai:20230404T133000 DTEND;TZID=Asia/Shanghai:20230404T143000 LAST-MODIFIED:20230330T101330Z LOCATION:hybrid (KIAA 1st meeting room + zoom), Meeting ID: 878 6573 2980, Passcode: astroPKU, Link: https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 SUMMARY:Probing novel physics through pulsar timing arrays URL;TYPE=URI:/info/1025/8870.htm END:VEVENT BEGIN:VEVENT UID:8863@kiaa.pku.edu.cn DTSTAMP:20230329T092043Z CREATED:20230329T092043Z DESCRIPTION:Qingming Festival Holida DTSTART;TZID=Asia/Shanghai:20230405T000000 DTEND;TZID=Asia/Shanghai:20230405T000000 LAST-MODIFIED:20230329T092043Z LOCATION: SUMMARY:Qingming Festival Holiday URL;TYPE=URI:/info/1089/8863.htm END:VEVENT BEGIN:VEVENT UID:8851@kiaa.pku.edu.cn DTSTAMP:20230320T100346Z CREATED:20230320T100346Z DESCRIPTION:In addition to the high-energy frontier, there exists a frontier that is characterized by ultra-light and ultra-weak phenomena. Detection of ultralight wave-like dark matter is an important aspect in addition to gravitational wave detection. When particle mass is extremely light, its de Broglie wavelength reaches the galactic scale. This makes detection possible through gravitational wave detec... DTSTART;TZID=Asia/Shanghai:20230406T153000 DTEND;TZID=Asia/Shanghai:20230406T163000 LAST-MODIFIED:20230320T100346Z LOCATION:KIAA-Auditorium SUMMARY:Search for ultra-light dark matter and gravitational waves using astronomical observations URL;TYPE=URI:/info/1024/8851.htm END:VEVENT BEGIN:VEVENT UID:8852@kiaa.pku.edu.cn DTSTAMP:20230320T135638Z CREATED:20230320T135638Z DESCRIPTION:The first detection of another planet around a Sun-like star marked the beginning of a new era in which our understanding of how planets typically form and the uniqueness of our Solar System were radically upended. We now know that planet formation is incredibly resilient, and produces a diverse myriad of planets around a wide range of stellar types. These remarkable findings tell us that the S... DTSTART;TZID=Asia/Shanghai:20230407T153000 DTEND;TZID=Asia/Shanghai:20230407T163000 LAST-MODIFIED:20230320T135638Z LOCATION:KIAA-Auditorium SUMMARY:Solving the Mystery of Small Exoplanets through Holistic Characterization URL;TYPE=URI:/info/1024/8852.htm END:VEVENT BEGIN:VEVENT UID:8862@kiaa.pku.edu.cn DTSTAMP:20230328T132701Z CREATED:20230328T132701Z DESCRIPTION:When the orbital pericenter of a star is equal to or smaller than the tidal radius of a black hole, the star will be tidally disrupted, triggering the so-called tidal disruption events (TDEs). The TDEs can generate electromagnetic radiation from radio to gamma ray bands. My talk focus on the optical and radio emission. The observationally inferred location of optical emission is 1014-16cm from ... DTSTART;TZID=Asia/Shanghai:20230411T160000 DTEND;TZID=Asia/Shanghai:20230411T170000 LAST-MODIFIED:20230328T132701Z LOCATION:KIAA-Auditorium SUMMARY:The optical/UV and radio emission of tidal disruption events URL;TYPE=URI:/info/1024/8862.htm END:VEVENT BEGIN:VEVENT UID:8739@kiaa.pku.edu.cn DTSTAMP:20230220T161816Z CREATED:20230220T161816Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230413T153000 DTEND;TZID=Asia/Shanghai:20230413T163000 LAST-MODIFIED:20230220T161816Z LOCATION:Remote Talk SUMMARY:TBD URL;TYPE=URI:/info/1024/8739.htm END:VEVENT BEGIN:VEVENT UID:8790@kiaa.pku.edu.cn DTSTAMP:20230228T141636Z CREATED:20230228T141636Z DESCRIPTION:TB DTSTART;TZID=Asia/Shanghai:20230418T133000 DTEND;TZID=Asia/Shanghai:20230418T143000 LAST-MODIFIED:20230228T141636Z LOCATION:zoom SUMMARY:TBD URL;TYPE=URI:/info/1025/8790.htm END:VEVENT BEGIN:VEVENT UID:8800@kiaa.pku.edu.cn DTSTAMP:20230302T110410Z CREATED:20230302T110410Z DESCRIPTION:TB DTSTART;TZID=Asia/Shanghai:20230418T133000 DTEND;TZID=Asia/Shanghai:20230418T143000 LAST-MODIFIED:20230302T110410Z LOCATION:zoom SUMMARY:TBD URL;TYPE=URI:/info/1025/8800.htm END:VEVENT BEGIN:VEVENT UID:8880@kiaa.pku.edu.cn DTSTAMP:20230331T133013Z CREATED:20230331T133013Z DESCRIPTION:The circumgalactic medium (CGM) plays a critical role in galaxy formation and evolution by mediating inflows and outflows. Recent years have seen significant progress in observations and understanding of the multiphase nature of the CGM. This talk will specifically focus on two phases: the hot phase with temperatures of log T >~ 6 and the photoionized cool phase at log T ~ 4, which have the mos... DTSTART;TZID=Asia/Shanghai:20230419T133000 DTEND;TZID=Asia/Shanghai:20230419T143000 LAST-MODIFIED:20230331T133013Z LOCATION:hybrid (KIAA 1st meeting room + zoom), Meeting ID: 878 6573 2980, Passcode: astroPKU, Link: https://us02web.zoom.us/j/87865732980?pwd=VmNqQkxXM21WVzBibnA1TmNxa0Radz09 SUMMARY:The Multiphase Circumgalactic Medium URL;TYPE=URI:/info/1025/8880.htm END:VEVENT BEGIN:VEVENT UID:8740@kiaa.pku.edu.cn DTSTAMP:20230220T163653Z CREATED:20230220T163653Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230427T153000 DTEND;TZID=Asia/Shanghai:20230427T163000 LAST-MODIFIED:20230220T163653Z LOCATION:Remote Talk SUMMARY:TBD URL;TYPE=URI:/info/1024/8740.htm END:VEVENT BEGIN:VEVENT UID:8730@kiaa.pku.edu.cn DTSTAMP:20230220T155201Z CREATED:20230220T155201Z DESCRIPTION:Labor Day Holida DTSTART;TZID=Asia/Shanghai:20230501T000000 DTEND;TZID=Asia/Shanghai:20230505T000000 LAST-MODIFIED:20230220T155201Z LOCATION: SUMMARY:Labor Day Holiday URL;TYPE=URI:/info/1089/8730.htm END:VEVENT BEGIN:VEVENT UID:8741@kiaa.pku.edu.cn DTSTAMP:20230222T141118Z CREATED:20230222T141118Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230511T153000 DTEND;TZID=Asia/Shanghai:20230511T163000 LAST-MODIFIED:20230222T141118Z LOCATION:KIAA-Auditorium SUMMARY:TBD URL;TYPE=URI:/info/1024/8741.htm END:VEVENT BEGIN:VEVENT UID:8742@kiaa.pku.edu.cn DTSTAMP:20230222T142911Z CREATED:20230222T142911Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230518T153000 DTEND;TZID=Asia/Shanghai:20230518T163000 LAST-MODIFIED:20230222T142911Z LOCATION:KIAA-Auditorium SUMMARY:TBD URL;TYPE=URI:/info/1024/8742.htm END:VEVENT BEGIN:VEVENT UID:8743@kiaa.pku.edu.cn DTSTAMP:20230222T143106Z CREATED:20230222T143106Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230525T153000 DTEND;TZID=Asia/Shanghai:20230525T163000 LAST-MODIFIED:20230222T143106Z LOCATION:KIAA-Auditorium SUMMARY:TBD URL;TYPE=URI:/info/1024/8743.htm END:VEVENT BEGIN:VEVENT UID:8831@kiaa.pku.edu.cn DTSTAMP:20230313T114006Z CREATED:20230313T114006Z DESCRIPTION:TB DTSTART;TZID=Asia/Shanghai:20230530T133000 DTEND;TZID=Asia/Shanghai:20230530T143000 LAST-MODIFIED:20230313T114006Z LOCATION:zoom SUMMARY:TBD URL;TYPE=URI:/info/1025/8831.htm END:VEVENT BEGIN:VEVENT UID:8744@kiaa.pku.edu.cn DTSTAMP:20230222T143302Z CREATED:20230222T143302Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230601T153000 DTEND;TZID=Asia/Shanghai:20230601T163000 LAST-MODIFIED:20230222T143302Z LOCATION:Remote Talk SUMMARY:TBD URL;TYPE=URI:/info/1024/8744.htm END:VEVENT BEGIN:VEVENT UID:8745@kiaa.pku.edu.cn DTSTAMP:20230222T143922Z CREATED:20230222T143922Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230608T153000 DTEND;TZID=Asia/Shanghai:20230608T163000 LAST-MODIFIED:20230222T143922Z LOCATION:Remote Talk SUMMARY:TBD URL;TYPE=URI:/info/1024/8745.htm END:VEVENT BEGIN:VEVENT UID:8746@kiaa.pku.edu.cn DTSTAMP:20230222T151740Z CREATED:20230222T151740Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230615T153000 DTEND;TZID=Asia/Shanghai:20230615T163000 LAST-MODIFIED:20230222T151740Z LOCATION:KIAA-Auditorium SUMMARY:TBD URL;TYPE=URI:/info/1024/8746.htm END:VEVENT BEGIN:VEVENT UID:8832@kiaa.pku.edu.cn DTSTAMP:20230313T115944Z CREATED:20230313T115944Z DESCRIPTION:TB DTSTART;TZID=Asia/Shanghai:20230620T133000 DTEND;TZID=Asia/Shanghai:20230620T143000 LAST-MODIFIED:20230313T115944Z LOCATION:hybrid SUMMARY:TBD URL;TYPE=URI:/info/1025/8832.htm END:VEVENT BEGIN:VEVENT UID:8747@kiaa.pku.edu.cn DTSTAMP:20230222T152130Z CREATED:20230222T152130Z DESCRIPTION:TBD DTSTART;TZID=Asia/Shanghai:20230622T153000 DTEND;TZID=Asia/Shanghai:20230622T163000 LAST-MODIFIED:20230222T152130Z LOCATION:Remote Talk SUMMARY:TBD URL;TYPE=URI:/info/1024/8747.htm END:VEVENT BEGIN:VEVENT UID:8731@kiaa.pku.edu.cn DTSTAMP:20230220T155530Z CREATED:20230220T155530Z DESCRIPTION:Summer Holida DTSTART;TZID=Asia/Shanghai:20230710T000000 DTEND;TZID=Asia/Shanghai:20230829T000000 LAST-MODIFIED:20230220T155530Z LOCATION: SUMMARY:Summer Holiday URL;TYPE=URI:/info/1089/8731.htm END:VEVENT BEGIN:VEVENT UID:8732@kiaa.pku.edu.cn DTSTAMP:20230220T155808Z CREATED:20230220T155808Z DESCRIPTION:Mid-Autumn Festival Holida DTSTART;TZID=Asia/Shanghai:20230929T000000 DTEND;TZID=Asia/Shanghai:20230929T000000 LAST-MODIFIED:20230220T155808Z LOCATION: SUMMARY:Mid-Autumn Festival Holiday URL;TYPE=URI:/info/1089/8732.htm END:VEVENT BEGIN:VEVENT UID:8733@kiaa.pku.edu.cn DTSTAMP:20230220T155946Z CREATED:20230220T155946Z DESCRIPTION:National Day Holida DTSTART;TZID=Asia/Shanghai:20231001T000000 DTEND;TZID=Asia/Shanghai:20231006T000000 LAST-MODIFIED:20230220T155946Z LOCATION: SUMMARY:National Day Holiday URL;TYPE=URI:/info/1089/8733.htm END:VEVENT BEGIN:VEVENT UID:8734@kiaa.pku.edu.cn DTSTAMP:20230220T160049Z CREATED:20230220T160049Z DESCRIPTION:Winter Holida DTSTART;TZID=Asia/Shanghai:20240115T000000 DTEND;TZID=Asia/Shanghai:20240215T000000 LAST-MODIFIED:20230220T160049Z LOCATION: SUMMARY:Winter Holiday URL;TYPE=URI:/info/1089/8734.htm END:VEVENT END:VCALENDAR