|
Size: 1714
Comment:
|
Size: 1340
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 12: | Line 12: |
| [[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 30: | Line 26: |
| * [[LCGT/Meeting/Analysis090519|090519]] | * [[LCGT/Meeting/Analysis090427|2009-04-27]] |
| Line 32: | Line 28: |
| * [[LCGT/Meeting/Analysis090519|2009-05-19]] |
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