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Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs
Abadie J., Accadia T., Barsuglia M., Bebronne M., Belletoile A. et al
http://hal.in2p3.fr/in2p3-00679943
Physique/Relativité Générale et Cosmologie Quantique
Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs
J. Abadie, T. Accadia1, M. Barsuglia2, M. Bebronne1, A. Belletoile1, B. Bouhou2, D. Buskulic1, C. Buy2, E. Chassande-Mottin2, A. Dietz1, M. Granata2, R. Gouaty1, N. Letendre1, F. Marion1, A. Masserot1, B. Mours1, L. Rolland1, E. Tournefier1, D. Verkindt1, M. Yvert1, R. Bonnand3, R. Flaminio3, J. Franc3, M. Galimberti3, C. Michel3, N. Morgado3, L. Pinard3, B. Sassolas3, M.-A. Bizouard4, V. Brisson4, F. Cavalier4, M. Davier4, P. Hello4, N. Leroy4, F. Robinet4, M. Vavoulidis4, R.L. Ward2, M. Was4
1 :  LAPP - Laboratoire d'Annecy le Vieux de Physique des Particules
http://wwwlapp.in2p3.fr/
CNRS : UMR5814 – IN2P3 – Université de Savoie
9 Chemin de Bellevue - BP 110 - 74941 Annecy-le-Vieux CEDEX - France
France
2 :  APC - UMR 7164 - AstroParticule et Cosmologie
http://www.apc.univ-paris7.fr/
CNRS : UMR7164 – IN2P3 – Observatoire de Paris – Université Paris VII - Paris Diderot – CEA : DSM/IRFU
APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13
France
3 :  LMA - Laboratoire des matériaux avancés
CNRS : USR3264 – IN2P3 – Université Claude Bernard - Lyon I (UCBL)
Bâtiment 213 VIRGO 22 7 avenue Pierre de Coubertin 69622 VILLEURBANNE CEDEX
France
4 :  LAL - Laboratoire de l'Accélérateur Linéaire
http://www.lal.in2p3.fr/
CNRS : UMR8607 – IN2P3 – Université Paris XI - Paris Sud
Centre Scientifique d'Orsay B.P. 34 91898 ORSAY Cedex
France
APC - Cosmologie et Gravitation
APC - ADAMIS
We summarize the sensitivity achieved by the LIGO and Virgo gravitational wave detectors for low-mass compact binary coalescence (CBC) searches during LIGO's sixth science run and Virgo's second and third science runs. We present strain noise power spectral densities (PSDs) which are representative of the typical performance achieved by the detectors in these science runs. The data presented here and in the accompanying web-accessible data files are intended to be released to the public as a summary of detector performance for low-mass CBC searches during S6 and VSR2-3.
LIGO
VIRGO

Pré-publications
2012

See paper for full list of authors - Associated data products are publicly accessible here https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=63432

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1203.2674