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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>>
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 * [[/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]]
  * List of minimul analysis processes
  * Procuderes for the first detection ant its confirmation
  * Software developments
  * Infrastructure for Data Analysis
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 * Data format of Pre-process data
  * For Compact Binary Coalescences
  * For Burst searches
  * For Continuous Searches
  * For Stochastic Backgrounds
 * [[/pre_processed_data|Data format of Pre-process data]]
 * [[attachment:ns_event_estimation.pdf|Estimated events for NS binary coalescence]]

== Meeting ==
 * [[LCGT/Meeting/Analysis090519|2009-05-19]]

 * [[LCGT/Meeting/Analysis090427|2009-04-27]]

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

Meeting

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