Noise monitor tools and their application to Virgo data

T. Accadia*, F. Acernese, M. Agathos, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, A. Basti, Th S. Bauer, M. Bebronne, M. Bejger, M. G. Beker, M. Bitossi, M. A. Bizouard, M. Blom, F. Bondu, L. Bonelli, R. Bonnand, V. Boschi, L. BosiB. Bouhou, S. Braccini, C. Bradaschia, M. Branchesi, Gabriel Chardin T. Briant, A. Brillet, V. Brisson, T. Bulik, H. J. Bulten, D. Buskulic, C. Buy, E. Calloni, B. Canuel, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, O. Chaibi, E. Chassande-Mottin, A. Chincarini, A. Chiummo, F. Cleva, E. Coccia, P. F. Cohadon, C. N. Colacino, J. Colas, A. Colla, M. Colombini, A. Conte, J. P. Coulon, E. Cuoco, S. D'Antonio, V. Dattilo, M. Davier, R. Day, R. De Rosa, G. Debreczeni, W. Del Pozzo, L. Di Fiore, A. Di Lieto, M. Di Paolo Emilio, A. Di Virgilio, A. Dietz, M. Drago, G. Endröczi, V. Fafone, I. Ferrante, F. Fidecaro, I. Fiori, R. Flaminio, L. A. Forte, J. D. Fournier, J. Franc, S. Franco, S. Frasca, F. Frasconi, M. Galimberti, L. Gammaitoni, F. Garufi, M. E. Gáspár, G. Gemme, E. Genin, A. Gennai, A. Giazotto, R. Gouaty, M. Granata, C. Greverie, G. M. Guidi, J. F. Hayau, A. Heidmann, H. Heitmann, P. Hello, G. Hemming, P. Jaranowski, R. J.G. Jonker, M. Kasprzack, I. Kowalska, A. Królak, N. Leroy, N. Letendre, T. G.F. Li, N. Liguori, M. Lorenzini, V. Loriette, G. Losurdo, E. Majorana, I. Maksimovic, V. Malvezzi, N. Man, M. Mantovani, F. Marchesoni, F. Marion, J. Marque, F. Martelli, A. Masserot, C. Michel, L. Milano, Y. Minenkov, M. Mohan, N. Morgado, A. Morgia, S. Mosca, B. Mours, L. Naticchioni, F. Nocera, L. Palladino, C. Palomba, F. Paoletti, R. Paoletti, M. Parisi, A. Pasqualetti, R. Passaquieti, D. Passuello, G. Persichetti, F. Piergiovanni, M. Pietka, L. Pinard, R. Poggiani, M. Prato, G. A. Prodi, M. Punturo, P. Puppo, D. S. Rabeling, I. Racz, P. Rapagnani, V. Re, T. Regimbau, F. Ricci, F. Robinet, A. Rocchi, L. Rolland, R. Romano, D. Rosińska, P. Ruggi, B. Sassolas, D. Sentenac, L. Sperandio, R. Sturani, B. Swinkels, M. Tacca, L. Taffarello, A. P.M. Ter Braack, A. Toncelli, M. Tonelli, O. Torre, E. Tournefier, F. Travasso, G. Vajente, J. F.J. Van Den Brand, C. Van Den Broeck, S. Van Der Putten, M. Vasuth, M. Vavoulidis, G. Vedovato, D. Verkindt, F. Vetrano, A. Viceré, J. Y. Vinet, S. Vitale, H. Vocca, R. L. Ward, M. Was, K. Yamamoto, M. Yvert, A. Zadroźny, J. P. Zendri

*Corresponding author for this work

Research output: Contribution to journalConference articlepeer-review

Abstract (may include machine translation)

The understanding of noise in interferometric gravitational wave detectors is fundamental in terms of both enabling prompt reactions in the mitigation of noise disturbances and in the establishment of appropriate data-cleaning strategies. Monitoring tools to perform online and offline noise analysis in areas such as transient signal detection, line identification algorithms and coherence are used to characterise the Virgo detector noise. In this paper, we describe the framework into which these tools are integrated - the Noise Monitor Application Programming Interface (NMAPI) - and provide examples of its application.

Original languageEnglish
Article number012024
JournalJournal of Physics: Conference Series
Volume363
Issue number1
DOIs
StatePublished - 2012
Externally publishedYes
Event9th Edoardo Amaldi Conference on Gravitational Waves, Amaldi 9 and the 2011 Numerical Relativity - Data Analysis Meeting, NRDA 2011 - Cardiff, United Kingdom
Duration: 10 Jul 201115 Jul 2011

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