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KAGRA collaboration meeting

Meeting schedule

Next meeting: International collaboration meeting on Nov. 6, 2012

45th(Domestic): Oct. 15, 2012(Mon) 13:00~(JST)

EVO connection [ help ]

Agenda

  1. Project Status (Kajita)　Viewgraph

  2. SEO (Kawamura) Viewgraph

  3. Status of LIGO (Rana) Viewgraph

  4. 1st Elites meeting report (Somiya) Viewgraph Timetable

  5. Subsystem Report
  6. Application for funding.
  7. Commissioning Plan
  8. others

Files

44th(Domestic): Jul. 9, 2012(Mon) 13:00~(JST)

EVO connection [ help ]

Agenda

  1. Project Status (Kajita)　Viewgraph

  2. “Commissioning Issues” (Arai) Viewgraph

  3. Research plan for Grant-in-Aid for Scientific Research (Kanda) Viewgraph

  4. Activity of SE office (Kawamura) Viewgraph

  5. Report of each subsystem (each chief)

  6. Research Collaboration with overseas project (ELiTES, Kuroda) Viewgraph

  7. Report of Workshop at Toyama University (Kawamura) Viewgraph

  8. Agenda of the forthcoming f2f meeting ViewGraph

  9. Program of PAB meeting in August (Kuroda) ViewGraph[X]

  10. Effort to get funds from JSPS ViewGraph[X]

  11. Others

Files

43th(International): May. 29, 2012(Mon) 9:00~(JST)

EVO connection [ help ]

Agenda

  1. Project Report (Kajita) ViewGraph[O]

  2. New Collaboration Members (Kuroda) ViewGraph

  3. Budget report in FY2011 (Ohashi) ViewGraph[O]

  4. SE Office report (Kawamura) ViewGraph[O]

  5. Report by Australian member (Linqing Wen) ViewGraph

  6. Report of Sub-working groups

  7. Presentation policy by CPC ViewGraph

  8. Others

Files

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

  1. Introduction of New Commers

  2. Present Status of aLIGO (K.Kawabe)viewgraph

  3. Project Report (T.Kajita) viewgraph

  4. Budget Status (M.Ohashi) viewgraph

  5. KAGRA Science Goal and Data Sharing (N.Kanda) KandaHayama

  6. Schedule and Roadmap (M.Ando) viewgraph

  7. Change of Chart (I.Nakatani) viewgraph

  8. Subgroup progress report by every chief

  9. Preparation for External Review (S. Kawamura) viewgraph

  10. Others (International Conferences in this year)

Files

Past collaboration meeting


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KAGRA/Meeting/Collaboration (last edited 2016-11-05 10:38:52 by miyoki)