Model waveform accuracy standards for gravitational wave data analysis
نویسندگان
چکیده
Lee Lindblom, Benjamin J. Owen, and Duncan A. Brown Theoretical Astrophysics 130-33, California Institute of Technology, Pasadena, California 91125, USA Institute for Gravitation and the Cosmos, and Center for Gravitational Wave Physics, Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802, USA Department of Physics, Syracuse University, Syracuse, New York 13244, USA (Received 22 September 2008; published 29 December 2008)
منابع مشابه
Sensitivity Analysis of Brown Model Waveform in Radar Altimetry
In satellite altimetry (radar altimetry), the altimeter emits a pulse, with known power, to the earth surface and receives it back continuously to determine of the sea surface height. The time series of the mean returned power is recorded individually at satellite as the so-called waveform. Analytical model for the waveform is first introduced by Brown, which consists of six parameters: signif...
متن کاملTriangulation of gravitational wave sources with a network of detectors
There is significant benefit to be gained by pursuing multi-messenger astronomy with gravitational wave and electromagnetic observations. In order to undertake electromagnetic follow-ups of gravitational wave signals, it will be necessary to accurately localize them in the sky. Since gravitational wave detectors are not inherently pointing instruments, localization will occur primarily through ...
متن کاملOn the accuracy and precision of numerical waveforms: Effect of waveform extraction methodology
We present a new set of 95 numerical relativity simulations of non-precessing binary black holes (BBHs). The simulations sample comprehensively both black-hole spins up to spin magnitude of 0.9, and cover mass ratios 1 to 3. The simulations cover on average 24 inspiral orbits, plus merger and ringdown, with low initial orbital eccentricities e < 10−4. A subset of the simulations extends the cov...
متن کاملar X iv : g r - qc / 0 51 11 46 v 1 2 7 N ov 2 00 5 Search for gravitational wave bursts in LIGO ’ s third science run B Abbott
We report on a search for gravitational wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets subsecond bursts in the frequency range 100–1100 Hz for which no waveform model is assumed, and has a sensitivity in terms of the root-sum-square (rss) strain amplitude of hrss ∼ 10 Hz. No gravitational wave signals were detected in the 8 d...
متن کاملar X iv : g r - qc / 0 51 11 46 v 1 2 7 N ov 2 00 5 Search for gravitational wave bursts in LIGO ’ s third science run
We report on a search for gravitational wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets subsecond bursts in the frequency range 100–1100 Hz for which no waveform model is assumed, and has a sensitivity in terms of the root-sum-square (rss) strain amplitude of hrss ∼ 10 Hz. No gravitational wave signals were detected in the 8 d...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008