Operational status of TAMA300 with the seismic attenuation system (SAS)
Authors:
- R TakahashiRTR Takahashi
- K AraiKAK Arai
- D TatsumiDTD Tatsumi
- M FukushimaMFM Fukushima
- T YamazakiTYT Yamazaki
- M-K FujimotoMFM-K Fujimoto
- K AgatsumaKAK Agatsuma
- Y AraseYAY Arase
- N NakagawaNNN Nakagawa
- A TakamoriATA Takamori
- K TsubonoKTK Tsubono
- R DeSalvoRDR DeSalvo
- 15 May 2008
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 25 (11)
Abstract
No abstract availableThis publication has 20 references indexed in Scilit:
- Results of the search for inspiraling compact star binaries from TAMA300’s observation in 2000–2004Physical Review D, 2006
- The status of LCGTClassical and Quantum Gravity, 2006
- The status of VIRGOClassical and Quantum Gravity, 2006
- Status of the LIGO detectorsClassical and Quantum Gravity, 2006
- Status of the GEO600 detectorClassical and Quantum Gravity, 2006
- Current status of the TAMA300 gravitational-wave detectorClassical and Quantum Gravity, 2005
- Status of TAMA300Classical and Quantum Gravity, 2004
- Vacuum-compatible vibration isolation stack for an interferometric gravitational wave detector TAMA300Review of Scientific Instruments, 2002
- Anatomy of the TAMA SAS seismic attenuation systemClassical and Quantum Gravity, 2002
- Improvement of the vibration isolation system for TAMA300Classical and Quantum Gravity, 2002