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---- == 44th(Domestic): Jul. 9, 2012(Mon) 13:00~(JST) == ---- [[LCGT/Meeting/weekly/20120416/EVO|EVO connection]] [ [[LCGT/Meeting/EVOen|help]] ] Agenda 1. Project Report (Kajita) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1074|ViewGraph[O]]] 1. New Collaboration Members (Kuroda) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=|ViewGraph]] 1. Budget report in FY2011 (Ohashi) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1071|ViewGraph[O]]] 1. SE Office report (Kawamura) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1066|ViewGraph[O]]] 1. Report by Australian member (Linqing Wen) [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1079|ViewGraph]] 1. Report of Sub-working groups 1. Presentation policy by CPC [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=|ViewGraph]] 1. Others Files . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1069|TUN[O]]] (Uchiyama) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1049|VAC[O]]] (Saito) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=|CRY[O]]] ([[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1065|Suzuki[O]]], [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1072|Yamamoto[O]]]) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1068|VIS[O]]] (Takahashi) . LAS and [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1078|MIR[O]] ] (Hirose/Mio) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=1075|MIF[O]]] (Aso) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=|IOO[X]]] (Telada) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1077|AOS[O]]] (Akutsu) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=1064|DGS[O]]] (Miyakawa) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1047|DAS[O]]] (Kanda) . [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=1076|DetChar[O]]] (Hayama) Talk by Dr.Linqing Wen. . Title: The scientific benefit of a larger GW detector network . Speaker: Linqing Wen (on behalf of the ACIGA collaboration) . Abstract: We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of tens of detections a year. A larger GW network is forming with the KAGRA detector in Japan partially funded and LIGO-India on the near horizon. In this talk, I will show that the GW detector network is approaching the desirable capacity that allows prompt and yet precise follow-up observations of gravitational wave events by conventional electromagnetic telescopes. I will then argue for a larger network that includes AIGO - a GW detector at the southern hemisphere. At the end of my presentation, I'll address briefly the status and future plan for AIGO. |
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. [[LCGT/Meeting/weekly/2011|Meetings in FY2011]] . [[LCGT/Meeting/weekly/2010|Meetings in FY2010]] |
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. [[LCGT/Meeting/weekly/2010|Meetings in FY2010]] . [[LCGT/Meeting/weekly/|Meetings in FY2011]] |
KAGRA collaboration meeting
Meeting schedule
Next meeting: International collaboration meeting on Nov. 6, 2012
44th(Domestic): Jul. 9, 2012(Mon) 13:00~(JST)
EVO connection [ help ]
Agenda
Project Report (Kajita) ViewGraph[O]
New Collaboration Members (Kuroda) ViewGraph
Budget report in FY2011 (Ohashi) ViewGraph[O]
SE Office report (Kawamura) ViewGraph[O]
Report by Australian member (Linqing Wen) ViewGraph
- Report of Sub-working groups
Presentation policy by CPC ViewGraph
- Others
Files
TUN[O] (Uchiyama)
VAC[O] (Saito)
CRY[O] (Suzuki[O], Yamamoto[O])
VIS[O] (Takahashi)
LAS and MIR[O ] (Hirose/Mio)
MIF[O] (Aso)
IOO[X] (Telada)
AOS[O] (Akutsu)
DGS[O] (Miyakawa)
DAS[O] (Kanda)
DetChar[O] (Hayama)
Talk by Dr.Linqing Wen.
- Title: The scientific benefit of a larger GW detector network
- Speaker: Linqing Wen (on behalf of the ACIGA collaboration)
- Abstract: We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of tens of detections a year. A larger GW network is forming with the KAGRA detector in Japan partially funded and LIGO-India on the near horizon. In this talk, I will show that the GW detector network is approaching the desirable capacity that allows prompt and yet precise follow-up observations of gravitational wave events by conventional electromagnetic telescopes. I will then argue for a larger network that includes AIGO - a GW detector at the southern hemisphere. At the end of my presentation, I'll address briefly the status and future plan for AIGO.
43th(International): May. 29, 2012(Mon) 9:00~(JST)
EVO connection [ help ]
Agenda
Project Report (Kajita) ViewGraph[O]
New Collaboration Members (Kuroda) ViewGraph
Budget report in FY2011 (Ohashi) ViewGraph[O]
SE Office report (Kawamura) ViewGraph[O]
Report by Australian member (Linqing Wen) ViewGraph
- Report of Sub-working groups
Presentation policy by CPC ViewGraph
- Others
Files
TUN[O] (Uchiyama)
VAC[O] (Saito)
CRY[O] (Suzuki[O], Yamamoto[O])
VIS[O] (Takahashi)
LAS and MIR[O ] (Hirose/Mio)
MIF[O] (Aso)
IOO[X] (Telada)
AOS[O] (Akutsu)
DGS[O] (Miyakawa)
DAS[O] (Kanda)
DetChar[O] (Hayama)
Talk by Dr.Linqing Wen.
- Title: The scientific benefit of a larger GW detector network
- Speaker: Linqing Wen (on behalf of the ACIGA collaboration)
- Abstract: We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of tens of detections a year. A larger GW network is forming with the KAGRA detector in Japan partially funded and LIGO-India on the near horizon. In this talk, I will show that the GW detector network is approaching the desirable capacity that allows prompt and yet precise follow-up observations of gravitational wave events by conventional electromagnetic telescopes. I will then argue for a larger network that includes AIGO - a GW detector at the southern hemisphere. At the end of my presentation, I'll address briefly the status and future plan for AIGO.
42th(Domestic): Apr. 16, 2012(Mon) 13:00~(JST)
EVO connection [ help ]
Agenda
- Introduction of New Commers
Present Status of aLIGO (K.Kawabe)viewgraph
Project Report (T.Kajita) viewgraph
Budget Status (M.Ohashi) viewgraph
Schedule and Roadmap (M.Ando) viewgraph
Change of Chart (I.Nakatani) viewgraph
- Subgroup progress report by every chief
Preparation for External Review (S. Kawamura) viewgraph
- Others (International Conferences in this year)
Files
DAS[O] (Kanda)
TUN[O] (Uchiyama)
VAC[O] (Saito)
LAS and MIR[O] (Hirose/Mio)
VIS[O] (Takahashi)
CRY[O] (Suzuki)
IOO (Telada)
MIF[O] (Aso)
AOS[O] (Akutsu)
DGS[O] (Miyakawa)
DetChar[O] (Hayama)
Past collaboration meeting