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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[X]
New Collaboration Members (Kuroda) ViewGraph[X]
Budget report in FY2011 (Ohashi) ViewGraph[X]
SE Office report (Kawamura) ViewGraph[X]
Report by Australian member (Linqing Wen) ViewGraph[X]
- Report of Sub-working groups
Presentation policy by CPC ViewGraph[X]
- Others
Files
- TUN[X] (Uchiyama)
- FCL[X] (Miyoki)
- VAC[X] (Saito)
- CRY[X] (Suzuki[X], Yamamoto[X])
- VIS[×] (Takahashi)
- LAS and MIR[X] (Hirose/Mio)
- MIF[X] (Aso)
- IOO[X] (Telada)
- AOS[X] (Akutsu)
- AEL[X] (Miyakawa)
- DGS[X] (Miyakawa)
- DAS[X] (Kanda)
- GIF[X] (Araya)
DetChar[X] (Hayama)
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