About: Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform?

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scientific article published on 01 March 1994

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована в березні 1994 (uk) article scientifique publié en 1994 (fr) im März 1994 veröffentlichter wissenschaftlicher Artikel (de) artículu científicu espublizáu en marzu de 1994 (ast) scientific article published on 01 March 1994 (en)
publication date	wds:Q74428846-6D1F201E-F6B8-43DC-814D-E21FBB060F2B
publication date	1994-03-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q74428846-3DE6FBF5-20B3-4C1B-AB8F-14EE9C6483FB
language of work or name	English
cites work	wds:Q74428846-E1D7A70D-AEF2-408B-AAB6-605BE1F874D4
cites work	Wideband laser-interferometer graviational-radiation experiment
author name string	wds:Q74428846-44CD5B46-44AE-4FE1-A865-89951F5D6141 wds:Q74428846-CAEA4A26-1642-43BC-ABDA-1B098E6EC371
author name string	Cutler C Flanagan ÉE
rdfs:label	Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (en) Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (nl)
skos:prefLabel	Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (en) Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (nl)
name	Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (en) Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (nl)
title	wds:Q74428846-F9A70ACF-08E9-44D1-90ED-932058A494A6
title	Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform? (en)
page(s)	wds:Q74428846-8C8CBCA3-F2D4-4CCC-8563-11EC784C280B
page(s)	2658-2697
instance of	wds:Q74428846-1AE6246D-3704-4305-8B27-E57506F95145
instance of	scholarly article
PubMed ID	wds:Q74428846-5C4A9B61-11AD-47C4-A2CB-2AEAC26DD183
PubMed ID	http://rdf.ncbi.nlm.nih.gov/pubchem/reference/10017261
PubMed ID	10017261
published in	wds:Q74428846-6B4CA8F4-B4A0-446E-ABDB-42EC6BAE1141
published in	Physical Review D
issue	wds:Q74428846-6AAD8192-667D-4E79-9304-99DFC121E68D
volume	wds:Q74428846-47B6E5F3-996F-4335-91A2-21C1988E1609
issue	6
volume	49
DOI	wds:Q74428846-C9A0832E-E8B3-4B5C-A241-73C25CE63DD3
DOI	http://dx.doi.org/10.1103/PHYSREVD.49.2658
DOI	10.1103/PHYSREVD.49.2658
arXiv ID	wds:Q74428846-C9EBFF20-6BB2-48AF-879D-91D920DF7E2C
arXiv ID	gr-qc/9402014
ADS bibcode	wds:Q74428846-2D6082A2-2A71-4AB2-B7B9-2325B1194D30
ADS bibcode	1994PhRvD..49.2658C
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q74428846
is cites work of	Coalescence of Black Hole-Neutron Star Binaries The Confrontation between General Relativity and Experiment Scalar-type gravitational wave emission from gravitational collapse in Brans-Dicke theory: Detectability by a laser interferometer LISA capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy Measuring gravitational waves from binary black hole coalescences. I. Signal to noise for inspiral, merger, and ringdown GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2 The Confrontation between General Relativity and Experiment. Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries Spin-induced orbital precession and its modulation of the gravitational waveforms from merging binaries GW150914: First results from the search for binary black hole coalescence with Advanced LIGO Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model Properties of the Binary Black Hole Merger GW150914 Effects of waveform model systematics on the interpretation of GW150914 Binary Black Hole Mergers in the First Advanced LIGO Observing Run The Confrontation between General Relativity and Experiment Bounding the mass of the graviton using gravitational-wave observations of inspiralling compact binaries Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries A signal transformational framework for breaking the noise floor and its applications in MRI. Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo. Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence. Physics, Astrophysics and Cosmology with Gravitational Waves. Observational Limit on Gravitational Waves from Binary Neutron Stars in the Galaxy Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA. Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3 Gravitational-Wave Data Analysis. Formalism and Sample Applications: The Gaussian Case Gravitational-Wave Tests of General Relativity with Ground-Based Detectors and Pulsar-Timing Arrays. On the Progenitor of Binary Neutron Star Merger GW170817 Search for gravitational-wave inspiral signals associated with short gamma-ray bursts during LIGO's fifth and virgo's first science run First LIGO search for gravitational wave bursts from cosmic (super)strings Hunting Gravitational Waves with Multi-Messenger Counterparts: Australia’s Role The NINJA-2 project: detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations Tanaka-Tagoshi parametrization of post-first-post-Newtonian spin-free gravitational wave chirps: Equispaced and cardinal interpolated lattices for first generation interferometric antennas Properties of the Binary Neutron Star Merger GW170817 Constraining the p -Mode– g -Mode Tidal Instability with GW170817 General relativistic magnetohydrodynamics simulations of prompt-collapse neutron star mergers: The absence of jets Measuring black-hole parameters and testing general relativity using gravitational-wave data from space-based interferometers Second-post-Newtonian generation of gravitational radiation Prospects for gravitational-wave observations of neutron-star tidal disruption in neutron-star-black-hole binaries. New approach to electromagnetic wave tails on a curved spacetime Determining the cosmic equation of state using future gravitational wave detectors Gravitational-Wave Data Analysis. Formalism and Sample Applications: The Gaussian Case Construction of a template family for the detection of gravitational waves from coalescing binaries Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA Gravitational radiation from a particle in circular orbit around a black hole. VI. Accuracy of the post-Newtonian expansion Gravitational waves from sub-lunar-mass primordial black-hole binaries: a new probe of extradimensions Matched filters for coalescing binaries detection on massively parallel computers Filtering post-Newtonian gravitational waves from coalescing binaries Observational constraints on the neutron star mass distribution Gravitational-wave asteroseismology with fundamental modes from compact binary inspirals
is cites work of	wds:Q30633708-8E63AA2F-3B91-4D6A-A0BD-76FBFE426AC7

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