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 * [[LCGT/subgroup/analysis/Meeting/Analysis2010|作業中ファイル(2010)]]
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 * Estimated events for NS binary coalescence  * [[attachment:ns_event_estimation.pdf|Estimated number of events for NS binary coalescence]]
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 * [[LCGT/Meeting/Analysis090519|2009-05-19]] === 作業班 ===
 * [[LCGT/subgroup/analysis/Meeting/Analysis090519|2009-05-19]]
 * [[LCGT/subgroup/analysis/Meeting/Analysis090427|2009-04-27]]
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 * [[LCGT/Meeting/Analysis090427|2009-04-27]] === 解析ミーティング ===
 * [[LCGT/subgroup/analysis/Meeting/Analysis2010|2010]]
 * [[LCGT/subgroup/analysis/Meeting/Analysis2009|2009]]

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

作業班

解析ミーティング

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