Background Noise Reduction in Gravitational Wave Detectors Through Use of an Amplitude Ratio Filter
- 1 July 2000
- journal article
- Published by Springer Nature in General Relativity and Gravitation
- Vol. 32 (7) , 1281-1300
- https://doi.org/10.1023/a:1001942721047
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Search for coincident excitation of the widely spaced resonant gravitational wave detectors EXPLORER, NAUTILUS and NIOBEAstroparticle Physics, 1999
- Status of TAMA projectClassical and Quantum Gravity, 1997
- Long term operation of a niobium resonant bar gravitational wave antennaPhysics Letters A, 1996
- The Allegro gravitational wave detector: Data acquisition and analysisPhysical Review D, 1996
- Sensitivity analysis of a resonant-mass gravitational wave antenna with a parametric transducerReview of Scientific Instruments, 1995
- Weiner filters for gravitational-wave antennas: Characteristics and applicationsIl Nuovo Cimento C, 1994
- Long-term operation of the Rome "Explorer" cryogenic gravitational wave detectorPhysical Review D, 1993
- Estimate of the background of a gravitational-wave detector due to cosmic raysIl Nuovo Cimento C, 1986
- Evidence for Discovery of Gravitational RadiationPhysical Review Letters, 1969
- Detection and Generation of Gravitational WavesPhysical Review B, 1960