Result: How many templates for GW chirp detection? The minimal-match issue revisited
Title:
How many templates for GW chirp detection? The minimal-match issue revisited
Authors:
Source:
Classical and quantum gravity (Print). 21(21):4955-4961
Publisher Information:
Bristol: Institute of Physics, 2004.
Publication Year:
2004
Physical Description:
print, 7 ref
Original Material:
INIST-CNRS
Subject Terms:
Theoretical physics, Physique théorique, Sciences exactes et technologie, Exact sciences and technology, Physique, Physics, Generalites, General, Relativité générale et gravitation, General relativity and gravitation, Etudes expérimentales de la gravitation, Experimental studies of gravity, Détecteurs d'ondes gravitationnelles et expériences, Gravitational wave detectors and experiments, Terre, ocean, espace, Earth, ocean, space, Astronomie, Astronomy, Astronomie fondamentale et astrophysique. Instrumentation, techniques, et observations astronomiques, Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations, Instruments d'astronomie et de recherche spatiale, Astronomical and space-research instrumentation, Détecteurs de rayonnement gravitationnel; spectromètres de masse; et autres instruments et techniques, Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques, Techniques d'observation et de réduction des données. Simulation et modélisation par ordinateur, Observation and data reduction techniques. Computer modeling and simulation, Méthodes mathématiques et méthodes de simulation sur ordinateur, Mathematical procedures and computer techniques, Binaire en coalescence, Merging binary stars, Maximum vraisemblance, Maximum likelihood, Maxima verosimilitud, Onde gravitationnelle, Gravitational waves, Performance
Document Type:
Academic journal
Article
File Description:
text
Language:
English
Author Affiliations:
D.I.3E., University of Salerno, Italy
Wavesgroup, University of Sannio at Benevento, Italy
Wavesgroup, University of Sannio at Benevento, Italy
ISSN:
0264-9381
Rights:
Copyright 2005 INIST-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Notes:
Astronomy
Theoretical physics
Theoretical physics
Accession Number:
edscal.16232187
Database:
PASCAL Archive
Further Information
Refined estimates for the template density (or minimal match) yielding the best trade-off between a detector's performance (in terms of false dismissals) and computational burden are obtained in the context of the maximum likelihood of detection of gravitational wave chirps from coalescing binaries with unknown parameters, using a recently derived accurate representation of the no-signal cumulative distribution of the detection statistic.