论文信息 - Detector characterization in GEO 600

Detector characterization in GEO 600

The GEO 600 interferometric gravitational wave detector conducted its first science run (S1) from 23 August 2002 to 9 September 2002. The GEO 600 data acquisition system is described together with some software tools developed for doing detector characterization and data analysis. Detector characterization results are also being presented.

[1] S. Mukherjee,et al. Median-based noise floor tracker (MNFT): robust estimation of noise floor drifts in interferometric data , 2003 .

[2] M. M. Casey,et al. A report on the status of the GEO 600 gravitational wave detector , 2003 .

[3] I. Heng,et al. PQMon: a powerful veto for burst events , 2003 .

[4] H. Grote,et al. Calibration of GEO 600 for the S1 science run , 2003 .

[5] S. Mohanty,et al. Towards a data and detector characterization robot for gravitational wave detectors , 2002 .

[6] Median based line tracker (MBLT): model independent and transient preserving line removal from interferometric data , 2002 .

[7] S. Babak,et al. Data acquisition and detector characterization of GEO600 , 2002, Classical and Quantum Gravity.

[8] Soma Mukherjee,et al. Towards a data and detector characterization robot for gravitational wave detectors , 2002 .

[9] S. Babak,et al. Data acquisition and detector characterization of GEO 600 , 2001 .

[10] Bernard F. Schutz,et al. The GEO 600 gravitational wave detector , 2002 .

[11] A. Tünnermann,et al. GEO 600. Proposal for a 600 m Laser-Interferometric Gravitational Wave Antenna , 1994 .