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| == Main Target == | == 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。<<BR>> 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。 |
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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]]<<BR>> == Preliminary design == * [[/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 == Detailed design == * [[/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]] |
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
Data Analysis White Paper 2009
Ref: LIGO document No. T080278-00 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
Detailed design