|
Size: 1714
Comment:
|
← Revision 39 as of 2012-06-06 18:25:11 ⇥
Size: 1472
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 1: | Line 1: |
| || '''[[LCGT|PROJECT TOP]]''' ||[[LCGT/subgroup/analysis|GW Analysis]] ||[[LCGT/subgroup/ifo|Interferometer]] ||[[LCGT/subgroup/vacuum|Vacuum & Cryostat]] ||[[LCGT/subgroup/laser|Laser & Optics]] ||[[LCGT/subgroup/machanics|Seismic Isolator]] ||[[LCGT/subgroup/infra|Infrastructure]] || |
## page was renamed from LCGT/subgroup/analysis/gw_search |
| Line 12: | Line 11: |
| [[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>> |
|
| Line 19: | Line 14: |
| * [[KAGRA/Subgroups/DAS/Meeting/Analysis2010|作業中ファイル(2010)]] |
|
| Line 28: | Line 25: |
| * [[attachment:ns_event_estimation.pdf|Estimated number of events for NS binary coalescence]] | |
| Line 29: | Line 27: |
| === Meeting === * [[LCGT/Meeting/Analysis090519|090519]] |
== Meeting == === 作業班 === * [[KAGRA/Subgroups/DAS/Meeting/Analysis090519|2009-05-19]] * [[KAGRA/Subgroups/DAS/Meeting/Analysis090427|2009-04-27]] === 解析ミーティング === * [[KAGRA/Subgroups/DAS/Meeting/Analysis2010|2010]] * [[KAGRA/Subgroups/DAS/Meeting/Analysis2009|2009]] |
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
Meeting
作業班