Differences between revisions 232 and 233
Revision 232 as of 2014-09-12 14:37:23
Size: 25825
Comment:
Revision 233 as of 2014-09-12 14:38:07
Size: 25818
Comment:
Deletions are marked like this. Additions are marked like this.
Line 15: Line 15:
 ||General report || -Saito||
 ||Installation Scheduling || -Uchiyama||
 ||General report -Saito||
 ||Installation Scheduling -Uchiyama||

KAGRA collaboration meeting


54nd(Domestic): Oct. 15, 2014 (Wednesday) 13:00~19:00

Participants:

[Kashiwa],・・・

[SeeVogh],・・・

Agenda

General Reports (13:00~14:45)

  1. LIGO talk    -TBD (40min)
  2. Project Report -Kajita (20min)
  3. SE Office report (30min)

    General report -Saito

    Installation Scheduling -Uchiyama

  4. Safety Control -Kuroda (15min)

Coffee Break (14:45-15:00)

Renewal of Project Plan (15:00-15:50)

  1. New financial situation -Ohashi (20min)
  2. Realization of bKAGRA -TBD (30min)

Subsystem reports (15:50~19:00)

  1. Report of A Subsystem -A chief (10-30min)
  2. General report of A subsystem
  3. Topical report by young scientist A
  4. Topical report by young scientist B
  5. Report of B subsystem -B chief (10-30min)
  6. General report of B subsystem
  7. Topical report by young scientist C
  8. Topical report by young scientist D


53rd(International): Jun. 12, 2014 (Thursday) 17:00~19:00 (JST)

Participants:

[Kashiwa] Kajita, Yamamoto, Kawamura, Kuroda, Miyamaoto, Tanaka, Sakakibara, Yamanaka

[SeeVogh] Saito, Ohashi, Itoh, Hayama, Yuzurihara, Ando, Kanda, Flaminio, Ueno, Aso, Miyakawa(PolyCom)

Agenda

  1. Project report - Kajita

  2. SEO report - Saito

  3. Report of subsystem 1
  4. Report of subsystem 2
  5. Others


52th(Domestic): Apr. 16, 2014 (Wed) 13:00~(JST)

In prior to this doestic meeting, we have lectures for new members staring at 10:00 in the morning. The lecturers are Prof. Kentaro Somiya and Prof Yusuke Itoh.

  1. Gravitational-wave detector - Somiya (60 min)

  2. Gravitational-wave data analysis - Itoh (60 min)

Agenda

  1. Random thoughts about aLIGO and installation        -Kawabe (45min)

  2. Introduction of Fresh persons (10min)
  3. Project Report          -Kajita (20min)

  4. SE Office report (report of the external review)          –Ando (20min)

Coffee Break (14:35-15:00)

  1. Schedule of Installation & Commissioning          -Saito (20min)

  2. Report of each subsystem (a few topics selected by SEO)(70min)

    What can we do with iKAGRA ?, Aso Control System of Interferometer, Miyakawa, (30min)

    Specification of laser(LAS, Suzuki & Mio, 20min)

    Tunnel structure and status - Tunnel,- FCL, Uchiyama & Miyoki (20min)

  3. Status of VIS R&D          -Pena(20min)

  4. Status of Cryo-suspension          -Yamamoto(20min)

  5. Others (Safety control)          -Kuroda(10min)


51th(International): Dec. 10, 2013 (Tuesday) 9:00~11:00 (JST)

Participants:

[Kashiwa], D. Castellano, D. Chen, K. Hayama, T. Kajita, S. Kawamura, A.Khalaidovski, F. Picariello, I. Pinto, Y. Saito, K. Watanabe, K. Yamamoto

[SeeVogh], T. Akutsu, M. Ando, Y. Aso, O. Miyakawa, S. Miyoki, Y.Sakakibara, K. Somiya, H. Tagoshi, C. Tokoku, T. Uchiyama, H. Yamamoto,T. Yokozawa, H. Yuzurihara

Agenda

  1. Project report by Kajita [O]

  2. Outline of iKAGRA installation by SEO (Saito), which will include task of each SEO member.[O]

  3. Conference reports (Korea-Japan WS by Kawamura [O] and ET+ELiTES meetings by Somiya [o])

  4. Report of MIR subsystem by Kyohei Watanabe (CSIRO report)[O]

  5. Others


50th(Domestic): Oct. 9, 2013 (Wed) 13:00~(JST)

Agenda

  1. News from LIGO (Output Mode Cleaner by K. Arai)

  2. Project report (Kajita)[o]

  3. SE Office report (Saito)[o]

  4. Report of each subsystem (I)
  5. Report of each subsystem (II)
  6. Status and Schedule of Mirror (Hirose)[o]

  7. Test and Schedule of anti-vibration system (Prototype-B) utilizing TAMA facility [o]

  8. Design of Payload and Vertical anti-vibration system
  9. Current status and schedule of cryogenic payload[o]

  10. Others

Files


49th(International): June 19 (Wed) 17:00~(JST)

Participants:(Kashiwa) T.Kajita, S.Kawamura, K.Yamamoto, R.Takahashi, T.Akutsu, Y.Saito, Chen Dan, Y.Itoh, A.Khalaidovski, K.Ono, (SeeVogh) F.E.P.Arellano, K.Somiya, L.Biotti, N.Kanda, R.DeSalvo, S.Miyoki, T.H.Yoon, T.Yokozawa, T.Sekiguchi,T.Suzuki, W.Johnson,Y.Aso, K.Agatsuma,N.Kawai

Agenda

  1. Project report [O] (Kajita)

  2. SE Office report [O] (Somiya)

  3. Plan of Core-to-core program of JSPS [O] (Kawamura)

  4. Conferences and Meeting report [O] (Kuroda)

  5. Report of Subsystems (if needed)
  6. Others

Files


48th(Domestic): Apr. 17, 2013 (Mon) 13:00~(JST)

Agenda

  1. Introduction of fresh members [O](Kuroda)

  2. Project status report [O]((Kajita)

  3. Speech of new project manager and explanation of new organization and meetings (Saito)
  4. SE Office report (mainly on the new budget saving plan) & Management of JSPS core-to-core program [O] [O]((Kawamura)

  5. Installation and Commissioning [O] (Kawamura and Ohashi)

  6. Reports of sub-systems (Each Chief)
  7. Others

Files


Meeting schedule

47th(Domestic): Dec. 17, 2012(Mon) 13:00~(JST)


EVO connection [ help ]

Agenda

  1. Project status report (Kajita) Viewgraph

  2. SE Office report (Kawamura) Viewgraph

  3. Hearing report on financial plan of each subsystem (Ohashi?) Viewgraph

  4. Report of each subsystem
  5. Quartary LIGO request (Kuroda?) Viewgraph

  6. Report of 4th ET symposium (Somiya and Yamamoto)ViewgraphViewgraph

  7. 2nd KAGRA data analysis school in February 2013 (Tagoshi)Viewgraph

  8. After EVO system (Kajita and Aso ?)Viewgraph

  9. others

Files


46th(International): Nov. 6, 2012(Tue) 9:00~(JST)


EVO connection [ help ]

Agenda

  1. Project Status Report (20 minutes including discussion)Viewgraph[O]

  2. SE Office report (30 minutes including discussion)Viewgraph[O]

  3. Start of Kamioka GWPO branch (10 minutes including discussion)Viewgraph[O]

  4. International relations (15 minutes)
    • Collaboration with LSC and Virgo(Kanda and Ando)Viewgraph[O]

    • First ELiTES and Virgo meeting(Kuroda)Viewgraph[O]

  5. Application to ICRR cooperative research (5 minutes) (Kuroda)Viewgraph[O]

  6. Others


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



LCGT wiki top

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