Abstract
Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is backscattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with a large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer.
Original language | English |
---|---|
Article number | 194011 |
Journal | Classical and Quantum Gravity |
Volume | 27 |
Issue number | 19 |
DOIs | |
State | Published - Oct 7 2010 |
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Noise from scattered light in Virgo's second science run data. / Accadia, T.; Acernese, F.; Antonucci, F.; Astone, P.; Ballardin, G.; Barone, F.; Barsuglia, M.; Bauer, Th S.; Beker, M. G.; Belletoile, A.; Birindelli, S.; Bitossi, M.; Bizouard, M. A.; Blom, M.; Bondu, F.; Bonelli, L.; Bonnand, R.; Boschi, V.; Bosi, L.; Bouhou, B.; Braccini, S.; Bradaschia, C.; Brillet, A.; Brisson, V.; Budzyński, R.; Bulik, T.; Bulten, H. J.; Buskulic, D.; Buy, C.; Cagnoli, G.; Calloni, E.; Campagna, E.; Canuel, B.; Carbognani, F.; Cavalier, F.; Cavalieri, R.; Cella, G.; Cesarini, E.; Mottin, E. Chassande; Chincarini, A.; Cleva, F.; Coccia, E.; Colacino, C. N.; Colas, J.; Colla, A.; Colombini, M.; Corsi, A.; Coulon, J. P.; Cuoco, E.; D'Antonio, S.; Dattilo, V.; Davier, M.; Day, R.; De Rosa, R.; Debreczeni, G.; Del Prete, M.; Di Fiore, L.; Di Lieto, A.; Di Paolo Emilio, M.; Di Virgilio, A.; Dietz, A.; Drago, M.; Fafone, V.; Ferrante, I.; Fidecaro, F.; Fiori, I.; Flaminio, R.; Fournier, J. D.; Franc, J.; Frasca, S.; Frasconi, F.; Freise, A.; Galimberti, M.; Gammaitoni, L.; Garufi, F.; Gáspár, M. E.; Gemme, G.; Genin, E.; Gennai, A.; Giazotto, A.; Gouaty, R.; Granata, M.; Greverie, C.; Guidi, G. M.; Hayau, J. F.; Heitmann, H.; Hello, P.; Hild, S.; Huet, D.; Jaranowski, P.; Kowalska, I.; Królak, A.; Leroy, N.; Letendre, N.; Li, T. G.F.; Lorenzini, M.; Loriette, V.; Losurdo, G.; Majorana, E.; Maksimovic, I.; Man, N.; Mantovani, M.; Marchesoni, F.; Marion, F.; Marque, J.; Martelli, F.; Masserot, A.; Michel, C.; Milano, L.; Minenkov, Y.; Mohan, M.; Morgado, N.; Morgia, A.; Mosca, S.; Moscatelli, V.; Mours, B.; Neri, I.; Nocera, F.; Pagliaroli, G.; Palladino, L.; Palomba, C.; Paoletti, F.; Pardi, S.; Parisi, M.; Pasqualetti, A.; Passaquieti, R.; Passuello, D.; Persichetti, G.; Pichot, M.; Piergiovanni, F.; Pietka, M.; Pinard, L.; Poggiani, R.; Prato, M.; Prodi, G. A.; Punturo, M.; Puppo, P.; Rabeling, D. S.; Rácz, I.; Rapagnani, P.; Re, V.; Regimbau, T.; Ricci, F.; Robinet, F.; Rocchi, A.; Rolland, L.; Romano, R.; Rosińska, D.; Ruggi, P.; Sassolas, B.; Sentenac, D.; Sperandio, L.; Sturani, R.; Swinkels, B. L.; Toncelli, A.; Tonelli, M.; Torre, O.; Tournefier, E.; Travasso, F.; Vajente, G.; Van Den Brand, J. F.J.; Van Der Putten, S.; Vasuth, M.; Vavoulidis, M.; Vedovato, G.; Verkindt, D.; Vetrano, F.; Viceré, A.; Vinet, J. Y.; Vocca, H.; Was, M.; Yvert, M.
In: Classical and Quantum Gravity, Vol. 27, No. 19, 194011, 07.10.2010.Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - Noise from scattered light in Virgo's second science run data
AU - Accadia, T.
AU - Acernese, F.
AU - Antonucci, F.
AU - Astone, P.
AU - Ballardin, G.
AU - Barone, F.
AU - Barsuglia, M.
AU - Bauer, Th S.
AU - Beker, M. G.
AU - Belletoile, A.
AU - Birindelli, S.
AU - Bitossi, M.
AU - Bizouard, M. A.
AU - Blom, M.
AU - Bondu, F.
AU - Bonelli, L.
AU - Bonnand, R.
AU - Boschi, V.
AU - Bosi, L.
AU - Bouhou, B.
AU - Braccini, S.
AU - Bradaschia, C.
AU - Brillet, A.
AU - Brisson, V.
AU - Budzyński, R.
AU - Bulik, T.
AU - Bulten, H. J.
AU - Buskulic, D.
AU - Buy, C.
AU - Cagnoli, G.
AU - Calloni, E.
AU - Campagna, E.
AU - Canuel, B.
AU - Carbognani, F.
AU - Cavalier, F.
AU - Cavalieri, R.
AU - Cella, G.
AU - Cesarini, E.
AU - Mottin, E. Chassande
AU - Chincarini, A.
AU - Cleva, F.
AU - Coccia, E.
AU - Colacino, C. N.
AU - Colas, J.
AU - Colla, A.
AU - Colombini, M.
AU - Corsi, A.
AU - Coulon, J. P.
AU - Cuoco, E.
AU - D'Antonio, S.
AU - Dattilo, V.
AU - Davier, M.
AU - Day, R.
AU - De Rosa, R.
AU - Debreczeni, G.
AU - Del Prete, M.
AU - Di Fiore, L.
AU - Di Lieto, A.
AU - Di Paolo Emilio, M.
AU - Di Virgilio, A.
AU - Dietz, A.
AU - Drago, M.
AU - Fafone, V.
AU - Ferrante, I.
AU - Fidecaro, F.
AU - Fiori, I.
AU - Flaminio, R.
AU - Fournier, J. D.
AU - Franc, J.
AU - Frasca, S.
AU - Frasconi, F.
AU - Freise, A.
AU - Galimberti, M.
AU - Gammaitoni, L.
AU - Garufi, F.
AU - Gáspár, M. E.
AU - Gemme, G.
AU - Genin, E.
AU - Gennai, A.
AU - Giazotto, A.
AU - Gouaty, R.
AU - Granata, M.
AU - Greverie, C.
AU - Guidi, G. M.
AU - Hayau, J. F.
AU - Heitmann, H.
AU - Hello, P.
AU - Hild, S.
AU - Huet, D.
AU - Jaranowski, P.
AU - Kowalska, I.
AU - Królak, A.
AU - Leroy, N.
AU - Letendre, N.
AU - Li, T. G.F.
AU - Lorenzini, M.
AU - Loriette, V.
AU - Losurdo, G.
AU - Majorana, E.
AU - Maksimovic, I.
AU - Man, N.
AU - Mantovani, M.
AU - Marchesoni, F.
AU - Marion, F.
AU - Marque, J.
AU - Martelli, F.
AU - Masserot, A.
AU - Michel, C.
AU - Milano, L.
AU - Minenkov, Y.
AU - Mohan, M.
AU - Morgado, N.
AU - Morgia, A.
AU - Mosca, S.
AU - Moscatelli, V.
AU - Mours, B.
AU - Neri, I.
AU - Nocera, F.
AU - Pagliaroli, G.
AU - Palladino, L.
AU - Palomba, C.
AU - Paoletti, F.
AU - Pardi, S.
AU - Parisi, M.
AU - Pasqualetti, A.
AU - Passaquieti, R.
AU - Passuello, D.
AU - Persichetti, G.
AU - Pichot, M.
AU - Piergiovanni, F.
AU - Pietka, M.
AU - Pinard, L.
AU - Poggiani, R.
AU - Prato, M.
AU - Prodi, G. A.
AU - Punturo, M.
AU - Puppo, P.
AU - Rabeling, D. S.
AU - Rácz, I.
AU - Rapagnani, P.
AU - Re, V.
AU - Regimbau, T.
AU - Ricci, F.
AU - Robinet, F.
AU - Rocchi, A.
AU - Rolland, L.
AU - Romano, R.
AU - Rosińska, D.
AU - Ruggi, P.
AU - Sassolas, B.
AU - Sentenac, D.
AU - Sperandio, L.
AU - Sturani, R.
AU - Swinkels, B. L.
AU - Toncelli, A.
AU - Tonelli, M.
AU - Torre, O.
AU - Tournefier, E.
AU - Travasso, F.
AU - Vajente, G.
AU - Van Den Brand, J. F.J.
AU - Van Der Putten, S.
AU - Vasuth, M.
AU - Vavoulidis, M.
AU - Vedovato, G.
AU - Verkindt, D.
AU - Vetrano, F.
AU - Viceré, A.
AU - Vinet, J. Y.
AU - Vocca, H.
AU - Was, M.
AU - Yvert, M.
N1 - Copyright: Copyright 2018 Elsevier B.V., All rights reserved.
PY - 2010/10/7
Y1 - 2010/10/7
N2 - Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is backscattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with a large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer.
AB - Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is backscattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with a large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer.
UR - http://www.scopus.com/inward/record.url?scp=78649628833&partnerID=8YFLogxK
U2 - 10.1088/0264-9381/27/19/194011
DO - 10.1088/0264-9381/27/19/194011
M3 - Article
AN - SCOPUS:78649628833
VL - 27
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
SN - 0264-9381
IS - 19
M1 - 194011
ER -