Result: Making h(t) for LIGO
Title:
Making h(t) for LIGO
Source:
Proceedings of the 8th gravitational wave data analysis workshop, Milwaukee, WI, USA, 17-20 December 2003Classical and quantum gravity (Print). 21(20):S1723-S1735
Publisher Information:
Bristol: Institute of Physics, 2004.
Publication Year:
2004
Physical Description:
print, 10 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, Analyse des séries temporelles, variabilité temporelle, Time series analysis, time variability, Détecteur onde gravitationnelle, Gravitational wave detectors, Méthode domaine temps, Time domain method, Método dominio tiempo
Document Type:
Conference
Conference Paper
File Description:
text
Language:
English
Author Affiliations:
Center for Gravitation and Cosmology, Department of Physics, University of Wisconsin-Milwaukee, PO Box 413, WI 53201, United States
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) und Universität Hannover, Aussenstelle Hannover, Callinstr. 38, 30167 Hannover, Germany
LIGO Hanford Observatory, PO Box 159, Richland, WA 99352, United States
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) und Universität Hannover, Aussenstelle Hannover, Callinstr. 38, 30167 Hannover, Germany
LIGO Hanford Observatory, PO Box 159, Richland, WA 99352, United States
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.16210580
Database:
PASCAL Archive
Further Information
The conversion of the read-out from the anti-symmetric port of the LIGO interferometers into gravitational strain has thus far been performed in the frequency domain. Here we describe a conversion in the time domain which is based on the method developed by GEO. We illustrate the method using the Hanford 4 km interferometer during the second LIGO science run (S2).