Analysis of noise lines in the Virgo C7 data

F. Acernese, P. Amico, M. Alshourbagy, F. Antonucci, S. Aoudia, P. Astone, S. Avino, D. Babusci, G. Ballardin, F. Barone, L. Barsotti, M. Barsuglia, Th S. Bauer, F. Beauville, S. Bigotta, S. Birindelli, M. A. Bizouard, C. Boccara, F. Bondu, L. BosiC. Bradaschia, S. Braccini, F. J. Van Den Brand, A. Brillet, V. Brisson, D. Buskulic, E. Calloni, E. Campagna, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, E. Chassande-Mottin, N. Christensen, C. Corda, A. Corsi, F. Cottone, A. C. Clapson, F. Cleva, J. P. Coulon, E. Cuoco, A. Dari, V. Dattilo, M. Davier, M. Del Prete, R. De Rosa, L. Di Fiore, A. D. Virgilio, B. Dujardin, A. Eleuteri, M. Evans, 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, G. Giordano, L. Giordano, R. Gouaty, D. Grosjean, G. Guidi, S. Hamdani, S. Hebri, H. Heitmann, P. Hello, D. Huet, S. Karkar, S. Kreckelbergh, P. La Penna, M. Laval, N. Leroy, N. Letendre, B. Lopez, 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, M. Mazzoni, L. Milano, F. Menzinger, C. Moins, J. Moreau, N. Morgado, B. Mours, F. Nocera, C. Palomba, F. Paoletti, S. Pardi, A. Pasqualetti, R. Passaquieti, D. Passuello, F. Piergiovanni, L. Pinard, R. Poggiani, M. Punturo, P. Puppo, S. Van Der Putten, K. Qipiani, P. Rapagnani, V. Reita, A. Remillieux, F. Ricci, I. Ricciardi, P. Ruggi, G. Russo, S. Solimeno, A. Spallicci, M. Tarallo, M. Tonelli, A. Toncelli, E. Tournefier, F. Travasso, C. Tremola, G. Vajente, D. Verkindt, F. Vetrano, A. Viceré, J. Y. Vinet, H. Vocca, M. Yvert

Research output: Contribution to journalArticle

6 Scopus citations

Abstract

The paper presents a description of the work of detection and identification of frequency lines in the Virgo dark fringe data from run C7. A number of methods are highlighted by which noise frequency lines are detected by data analysis and measurements in the laboratory. In this paper we give a description of the list of noise line candidates provided by the pulsar search analysis, the investigation of 10 Hz (and harmonics) noise, violin modes, noise from the end station buildings' air conditioners, sidebands in calibration lines and aliasing in the 4 kHz reconstructed data.

Original languageEnglish
Article numberS07
Pages (from-to)S433-S443
JournalClassical and Quantum Gravity
Volume24
Issue number19
DOIs
StatePublished - Oct 7 2007

Fingerprint Dive into the research topics of 'Analysis of noise lines in the Virgo C7 data'. Together they form a unique fingerprint.

  • Cite this

    Acernese, F., Amico, P., Alshourbagy, M., Antonucci, F., Aoudia, S., Astone, P., Avino, S., Babusci, D., Ballardin, G., Barone, F., Barsotti, L., Barsuglia, M., Bauer, T. S., Beauville, F., Bigotta, S., Birindelli, S., Bizouard, M. A., Boccara, C., Bondu, F., ... Yvert, M. (2007). Analysis of noise lines in the Virgo C7 data. Classical and Quantum Gravity, 24(19), S433-S443. [S07]. https://doi.org/10.1088/0264-9381/24/19/S07