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== Main Target == == Main Target among GW sources ==
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 [[attachment:lcgt_ana_concept_090519.pdf|2008年度 解析グループ検討案+辰巳試案]]  [[attachment:lcgt_ana_concept_090519.pdf|2008年度 解析グループ検討案+辰巳試案]]<<BR>>
 [[attachment:Analysis_20081110_kanda.pdf|2008/11/10 LCGTミーティングでの資料(神田)]]<<BR>>
 [[attachment:coordinator_ana_20090413.pdf|2009/4/13 コーディネータ会議での説明(神田)]]<<BR>>
 [[attachment:BandAndPhysics_090519.pdf|2009/5/19 会議資料:観測帯域と物理(神田)]]<<BR>>
 [[attachment:Strategiy_090519.pdf|2009/5/19 会議資料:方針提案(神田)]]<<BR>>
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 * [[/white_paper_2009|Analysis White Paper 2009]]
   Ref: [[attachment:toc.txt|Table of Contents / LSC-Virgo white paper -DRAFT]]
 * [[/white_paper_2009|Data Analysis White Paper 2009]]
   Ref: LIGO document No. T080278-00 [[attachment:toc.txt|Table of Contents / LSC-Virgo white paper -DRAFT]]

PROJECT TOP

GW Analysis

Interferometer

Vacuum & Cryostat

Laser & Optics

Seismic Isolator

Infrastructure

目的

  • 世界初の重力波信号の直接検出に最大限貢献することを目指す。
    初検出後は、重力波天文学の創生に寄与することが LCGT project の目標である。

Main Target among GW sources

  • 連星中性子合体からの重力波を年数回程度観測すること。

Conceptual design

Preliminary design

Detailed design

KAGRA/Subgroups/DAS/gw_search (last edited 2012-06-06 18:25:11 by OsamuMiyakawa)