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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 Status (Kajita) ViewGraph
“Commissioning Issues” (Arai) Viewgraph
Research plan for Grant-in-Aid for Scientific Research (Kanda) Viewgraph
Activity of SE office (Kawamura) Viewgraph
- Report of each subsystem (each chief)
Research Collaboration with overseas project (ELiTES, Kuroda) Viewgraph
Report of Workshop at Toyama University (Kawamura) Viewgraph
Agenda of the forthcoming f2f meeting ViewGraph
Program of PAB meeting in August (Kuroda) ViewGraph[X]
Effort to get funds from JSPS ViewGraph[X]
- Others
Files
TUN[O] (Uchiyama)
FCL[O] (Miyoki)
VAC[O] (Saito)
CRY[X] (Suzuki[X], Yamamoto[O])
VIS[O] (Takahashi)
LAS and MIR[O] (Ueda)
- MIF[X] (Aso)
- IOO[X] (Telada)
AOS[O] (Akutsu)
AEL[O] (Miyakawa)
DGS[O] (Miyakawa)
DAS[O] (Kanda)
GIF[O] (Araya)
- DC[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