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A first comparison between LIGO and Virgo inspiral search pipelines

F Beauville et al 2005 Class. Quantum Grav. 22 S1149-S1158   doi: 10.1088/0264-9381/22/18/S29  Help

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F Beauville1, M-A Bizouard2, L Blackburn3, L Bosi4, P Brady5, L Brocco6, D A Brown5,7, D Buskulic1, S Chatterji7, N Christensen8, A-C Clapson2, S Fairhurst5, D Grosjean1, G Guidi9, P Hello2, E Katsavounidis3, M Knight8, A Lazzarini7, F Marion1, B Mours1, F Ricci6, A Viceré9 and M Zanolin3 (The joint LIGO/Virgo working group)
1 Laboratoire d'Annecy-le-Vieux de physique des particules, Chemin de Bellevue, BP 110, 74941 Annecy-le-Vieux Cedex, France
2 Laboratoire de l'Accélérateur Linéaire (LAL), IN2P3/CNRS-Université de Paris-Sud, B.P. 34, 91898 Orsay Cedex, France
3 LIGO-Massachusetts Institute of Technology, Cambridge, MA 02139, USA
4 INFN Sezione di Perugia and/or Università di Perugia, Via A. Pascoli, I-06123, Perugia, Italy
5 University of Wisconsin—Milwaukee, Milwaukee, WI 53201, USA
6 INFN, Sezione di Roma and/or Università 'La Sapienza', P.le A. Moro 2, I-00185, Roma, Italy
7 LIGO-California Institute of Technology, Pasadena, CA 91125, USA
8 Carleton College, Northfield, MN 55057, USA
9 INFN—Sezione Firenze/Urbino Via G.Sansone 1, I-50019 Sesto Fiorentino and/or Università di Urbino, Via S.Chiara 27, I-61029, Urbino, Italy

Abstract. This paper reports on a project that is the first step the LIGO Scientific Collaboration and the Virgo Collaboration have taken to prepare for a mutual search for inspiral signals. The project involved comparing the analysis pipelines of the two collaborations on data sets prepared by both sides, containing simulated noise and injected events. The ability of the pipelines to detect the injected events was checked, and a first comparison of how the parameters of the events were recovered has been completed.

PACS numbers: 04.80.Nn, 07.05.Kf, 95.55.Ym

Print publication: Issue 18 (21 September 2005)
Received 12 April 2005, in final form 17 June 2005
Published 6 September 2005

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