Classification of glitch waveforms in gravitational wave detector characterization
نویسندگان
چکیده
منابع مشابه
A quantum-enhanced prototype gravitational-wave detector
K. GODA1, O. MIYAKAWA2, E. E. MIKHAILOV3, S. SARAF4, R. ADHIKARI2, K. MCKENZIE5, R. WARD2, S. VASS2, A. J. WEINSTEIN2 AND N. MAVALVALA1* LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA The College of William and Mary, Williamsburg, Virginia 23187, USA Rochester Instit...
متن کاملGravitational wave detector with cosmological reach
Citation Dwyer, Sheila, et al. "Gravitational wave detector with cosmological reach. Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Twenty years ago, construction...
متن کاملGravitational-wave data analysis using binary black-hole waveforms
While the inspiral and ring-down stages of the binary black-hole coalescence are well-modelled by analytical approximation methods in general relativity, the recent progress in numerical relativity has enabled us to compute accurate waveforms from the merger stage also. This has an important impact on the search for gravitational waves from binary black holes. ‘Complete’ binary black-hole wavef...
متن کاملSubtraction-noise projection in gravitational-wave detector networks
In this paper, we present a successful implementation of a subtraction-noise projection method into a simple, simulated data analysis pipeline of a gravitational-wave search. We investigate the problem to reveal a weak stochastic background signal which is covered by a strong foreground of compact-binary coalescences. The foreground, which is estimated by matched filters, has to be subtracted f...
متن کاملAngular Resolution of the LISA Gravitational Wave Detector
We calculate the angular resolution of the planned LISA detector, a space-based laser interferometer for measuring low-frequency gravitational waves from galactic and extragalactic sources. LISA is not a pointed instrument; it is an all-sky monitor with a quadrupolar beam pattern. LISA will measure simultaneously both polarization components of incoming gravitational waves, so the data will con...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of Physics: Conference Series
سال: 2010
ISSN: 1742-6596
DOI: 10.1088/1742-6596/243/1/012006