Analysis of noise lines in the Virgo C7 data

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, Ts; Beauville, F; Bigotta, S; Birindelli, S; Bizouard, Ma; Boccara, C; Bondu, F; Bosi, L; Bradaschia, C; Braccini, S; van den Brand FJ,; Brillet, A; Brisson, V; Buskulic, D; Calloni, E; Campagna, E; Carbognani, F; Cavalier, F; Cavalieri, R; Cella, G; Cesarini, E; Chassande Mottin, E; Christensen, N; Corda, C; Corsi, A; Cottone, F; Clapson, Ac; Cleva, F; Coulon, Jp; Cuoco, E; Dari, A; Dattilo, V; Davier, M; del Prete, M; De Rosa, R; Di Fiore, L; Di Virgilio, A; Dujardin, B; Eleuteri, A; Evans, M; Ferrante, Isidoro; Fidecaro, Francesco; Fiori, I; Flaminio, R; Fournier, Jd; Frasca, S; Frasconi, F; Gammaitoni, L; Garufi, F; Genin, E; Gennai, A; Giazotto, A; Giordano, G; Giordano, L; Gouaty, R; Grosjean, D; Guidi, G; Hamdani, S; Hebri, S; Heitmann, H; Hello, P; Huet, D; Karkar, S; Kreckelbergh, S; La Penna, P; Laval, M; Leroy, N; Letendre, N; Lopez, B; Lorenzini,; Loriette, V; Losurdo, G; Mackowski, Jm; Majorana, E; Man, Cn; Mantovani, M; Marchesoni, F; Marion, F; Marque, J; Martelli, F; Masserot, A; Mazzoni, M; Milano, L; Menzinger, F; Moins, C; Moreau, J; Morgado, N; Mours, B; Nocera, F; Palomba, C; Paoletti, F; Pardi, S; Pasqualetti, A; Passaquieti, Roberto; Passuello, D; Piergiovanni, F; Pinard, L; Poggiani, Rosa; Punturo, M; Puppo, P; van der Putten, S; Qipiani, K; Rapagnani, P; Reita, V; Remillieux, A; Ricci, F; Ricciardi, I; Ruggi, P; Russo, G; Solimeno, S; Spallicci, A; Tarallo, M; Tonelli, Mauro; Toncelli, Alessandra; Tournefier, E; Travasso, F; Tremola, C; Vajente, G; Verkindt, D; Vetrano, F; Vicere, A; Vinet, Jy; Vocca, H; Yvert, M.

doi:10.1088/0264-9381/24/19/S07

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.

Titolo:	Analysis of noise lines in the Virgo C7 data
Autori interni:	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 TS Beauville F Bigotta S Birindelli S Bizouard MA Boccara C Bondu F Bosi L Bradaschia C Braccini S van den Brand FJ Brillet A Brisson V Buskulic D Calloni E Campagna E Carbognani F Cavalier F Cavalieri R Cella G Cesarini E Chassande Mottin E Christensen N Corda C Corsi A Cottone F Clapson AC Cleva F Coulon JP Cuoco E Dari A Dattilo V Davier M del Prete M De Rosa R Di Fiore L Di Virgilio A Dujardin B Eleuteri A Evans M FERRANTE, ISIDORO FIDECARO, FRANCESCO Fiori I Flaminio R Fournier JD Frasca S Frasconi F Gammaitoni L Garufi F Genin E Gennai A Giazotto A Giordano G Giordano L Gouaty R Grosjean D Guidi G Hamdani S Hebri S Heitmann H Hello P Huet D Karkar S Kreckelbergh S La Penna P Laval M Leroy N Letendre N Lopez B Lorenzini Loriette V Losurdo G Mackowski JM Majorana E Man CN Mantovani M Marchesoni F Marion F Marque J Martelli F Masserot A Mazzoni M Milano L Menzinger F Moins C Moreau J Morgado N Mours B Nocera F Palomba C Paoletti F Pardi S Pasqualetti A PASSAQUIETI, ROBERTO Passuello D Piergiovanni F Pinard L POGGIANI, ROSA Punturo M Puppo P van der Putten S Qipiani K Rapagnani P Reita V Remillieux A Ricci F Ricciardi I Ruggi P Russo G Solimeno S Spallicci A Tarallo M TONELLI, MAURO TONCELLI, ALESSANDRA Tournefier E Travasso F Tremola C Vajente G Verkindt D Vetrano F Vicere A Vinet JY Vocca H Yvert M. mostra contributor esterni nascondi contributor esterni
Anno del prodotto:	2007
Rivista:	CLASSICAL AND QUANTUM GRAVITY
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.
Handle:	http://hdl.handle.net/11568/115475
Appare nelle tipologie:	4.1 Contributo in Atti di convegno

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