Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs - IN2P3 - Institut national de physique nucléaire et de physique des particules Accéder directement au contenu
Pré-Publication, Document De Travail Année : 2012

Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs

J. Abadie
  • Fonction : Auteur
M. Barsuglia
B. Bouhou
  • Fonction : Auteur
  • PersonId : 941023
Christelle Lesvigne-Buy
  • Fonction : Auteur
  • PersonId : 924454
E. Chassande-Mottin
Christine Michel
N. Leroy
M. Was

Résumé

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.

Dates et versions

in2p3-00679943 , version 1 (16-03-2012)

Identifiants

  • HAL Id : in2p3-00679943 , version 1
  • ARXIV : 1203.2674

Citer

J. Abadie, T. Accadia, M. Barsuglia, M. Bebronne, A. Belletoile, et al.. Sensitivity Achieved by the LIGO and Virgo Gravitational Wave Detectors during LIGO's Sixth and Virgo's Second and Third Science Runs. 2012. ⟨in2p3-00679943⟩
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