Automatic Alignment for the first science run of the Virgo interferometer

F. Acernese,M. Alshourbagy,F. Antonucci,S. Aoudia,K.G. Arun,P. Astone,G. Ballardin,F. Barone,M. Barsuglia,Th.S. Bauer,S. Bigotta,S. Birindelli,M.A. Bizouard,C. Boccara,F. Bondu,L. Bonelli,L. Bosi,S. Braccini,C. Bradaschia,A. Brillet,V. Brisson,H.J. Bulten, D. Buskulic,G. Cagnoli,E. Calloni,E. Campagna,B. Canuel,F. Carbognani,L. Carbone,F. Cavalier,R. Cavalieri,G. Cella,E. Cesarini,E. Chassande-Mottin,S. Chatterji,F. Cleva,E. Coccia,J. Colas,M. Colombini,C. Corda,A. Corsi,J.-P. Coulon,E. Cuoco,S. D’Antonio,A. Dari,V. Dattilo, M. Davier,R. De Rosa, M. Del Prete,L. Di Fiore,A. Di Lieto,M. Di Paolo Emilio,A. Di Virgilio,V. Fafone,I. Ferrante, F. Fidecaro,I. Fiori,R. Flaminio,J.-D. Fournier,S. Frasca,F. Frasconi,L. Gammaitoni,F. Garufi,E. Genin,A. Gennai,A. Giazotto,M. Granata,V. Granata,C. Greverie,G. Guidi,H. Heitmann,P. Hello, S. Hild,D. Huet,P. La Penna,M. Laval,N. Leroy,N. Letendre,M. Lorenzini,V. Loriette,G. Losurdo,J.-M. Mackowski,E. Majorana,C.N. Man,M. Mantovani, F. Marchesoni,F. Marion,J. Marque,F. Martelli,A. Masserot,F. Menzinger, C. Michel,L. Milano,Y. Minenkov,M. Mohan,J. Moreau,N. Morgado,S. Mosca, B. Mours,I. Neri,F. Nocera,G. Pagliaroli,C. Palomba,F. Paoletti,S. Pardi,A. Pasqualetti,R. Passaquieti,D. Passuello,G. Persichetti,F. Piergiovanni,L. Pinard,R. Poggiani,M. Punturo,P. Puppo,O. Rabaste,P. Rapagnani,T. Regimbau,F. Ricci,A. Rocchi,L. Rolland,R. Romano,P. Ruggi,B. Sassolas,D. Sentenac,B.L. Swinkels,R. Terenzi,A. Toncelli,M. Tonelli,E. Tournefier,F. Travasso,J. Trummer,G. Vajente, J.F.J. van den Brand,S. van der Putten,D. Verkindt,F. Vetrano,A. Viceré,J.-Y. Vinet,H. Vocca,M. Was,M. Yvert

Astroparticle Physics（2010）

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摘要

During the past few years a network of large-scale laser interferometers, including the Virgo detector, has been developed with the aim of detecting gravitational waves. To properly operate the detectors, the longitudinal and angular positions of the suspended detector test masses, the interferometer mirrors, must be kept within a small range from the operating point.

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关键词

Gravitational wave detectors,Interferometry,Control systems,Angular

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