학술논문

The Virgo O3 run and the impact of the environment
Document Type
Working Paper
Author
Acernese, F.Agathos, M.Ain, A.Albanesi, S.Allocca, A.Amato, A.Andrade, T.Andres, N.Andrés-Carcasona, M.Andrić, T.Ansoldi, S.Antier, S.Apostolatos, T.Appavuravther, E. Z.Arène, M.Arnaud, N.Assiduo, M.Melo, S. Assis de SouzaAstone, P.Aubin, F.Avgitas, T.Babak, S.Badaracco, F.Bader, M. K. M.Bagnasco, S.Baird, J.Baka, T.Ballardin, G.Baltus, G.Banerjee, B.Barbieri, C.Barneo, P.Barone, F.Barsuglia, M.Barta, D.Basti, A.Bawaj, M.Bazzan, M.Beirnaert, F.Bejger, M.Belahcene, I.Benedetto, V.Berbel, M.Bernuzzi, S.Bersanetti, D.Bertolini, A.Bhardwaj, U.Bianchi, A.Bini, S.Bischi, M.Bitossi, M.Bizouard, M. -A.Bobba, F.Boër, M.Bogaert, G.Boldrini, M.Bonavena, L. D.Bondu, F.Bonnand, R.Boom, B. A.Boschi, V.Boudart, V.Bouffanais, Y.Bozzi, A.Bradaschia, C.Branchesi, M.Breschi, M.Briant, T.Brillet, A.Brooks, J.Bruno, G.Bucci, F.Bulik, T.Bulten, H. J.Buskulic, D.Buy, C.Cabras, G.Cabrita, R.Cagnoli, G.Calloni, E.Canepa, M.Canevarolo, S.Cannavacciuolo, M.Capocasa, E.Carapella, G.Carbognani, F.Caredda, E.Carpinelli, M.Carullo, G.Diaz, J. CasanuevaCasentini, C.Caudill, S.Cavalier, F.Cavalieri, R.Cella, G.Cerdá-Durán, P.Cesarini, E.Chaibi, W.Chanial, P.Chassande-Mottin, E.Chaty, S.Chiadini, F.Chiarini, G.Chierici, R.Chincarini, A.Chiofalo, M. L.Chiummo, A.Christensen, N.Ciani, G.Ciecielag, P.Cieślar, M.Cifaldi, M.Ciolfi, R.Cipriano, F.Clesse, S.Cleva, F.Coccia, E.Codazzo, E.Cohadon, P. -F.Cohen, D. E.Colombo, A.Colpi, M.Conti, L.Cordero-Carrión, I.Corezzi, S.Corre, D.Cortese, S.Coughlin, M.Coulon, J. -P.Croquette, M.Cudell, J. R.Cuoco, E.Curyło, M.Dabadie, P.Canton, T. DalDall'Osso, S.Dálya, G.D'Angelo, B.Danilishin, S.D'Antonio, S.Dattilo, V.Davier, M.Degallaix, J.De Laurentis, M.Deléglise, S.De Lillo, F.Dell'Aquila, D.Del Pozzo, W.De Matteis, F.Depasse, A.De Pietri, R.De Rosa, R.De Rossi, C.De Simone, R.Di Fiore, L.Di Giorgio, C.Di Giovanni, F.Di Giovanni, M.Di Girolamo, T.Di Lieto, A.Di Michele, A.Di Pace, S.Di Palma, I.Di Renzo, F.D'Onofrio, L.Drago, M.Ducoin, J. -G.Dupletsa, U.Durante, O.D'Urso, D.Duverne, P. -A.Eisenmann, M.Errico, L.Estevez, D.Fabrizi, F.Faedi, F.Fafone, V.Farinon, S.Favaro, G.Fays, M.Fenyvesi, E.Ferrante, I.Fidecaro, F.Figura, P.Fiori, A.Fiori, I.Fittipaldi, R.Fiumara, V.Flaminio, R.Font, J. A.Frasca, S.Frasconi, F.Freise, A.Freitas, O.Fronzé, G. G.Gamba, R.Garaventa, B.Garufi, F.Gemme, G.Gennai, A.Ghosh, ArchismanGiacomazzo, B.Giacoppo, L.Giri, P.Gissi, F.Giunchi, C.Gkaitatzis, S.Goncharov, B.Gosselin, M.Gouaty, R.Grado, A.Granata, M.Granata, V.Greco, G.Grignani, G.Grimaldi, A.Grimm, S. J.Gruning, P.Guerra, D.Guidi, G. M.Guixé, G.Guo, Y.Gupta, P.Haegel, L.Halim, O.Hannuksela, O.Harder, T.Haris, K.Harms, J.Haskell, B.Heidmann, A.Heitmann, H.Hello, P.Hemming, G.Hennes, E.Hild, S.Hofman, D.Hui, V.Idzkowski, B.Iess, A.Iosif, P.Jacqmin, T.Jacquet, P. -E.Janquart, J.Janssens, K.Jaranowski, P.Juste, V.Kalaghatgi, C.Karathanasis, C.Katsanevas, S.Kéfélian, F.Khetan, N.Koekoek, G.Koley, S.Kolstein, M.Królak, A.Kuijer, P.Lagabbe, P.Laghi, D.Lalleman, M.Lamberts, A.La Rosa, I.Lartaux-Vollard, A.Lazzaro, C.Leaci, P.Lemaître, A.Lenti, M.Leonova, E.Leroy, N.Letendre, N.Leyde, K.Linde, F.London, L.Longo, A.Portilla, M. LopezLorenzini, M.Loriette, V.Losurdo, G.Lumaca, D.Macquet, A.Magazzù, C.Magnozzi, M.Majorana, E.Maksimovic, I.Man, N.Mangano, V.Mantovani, M.Mapelli, M.Marchesoni, F.Pina, D. MarínMarion, F.Marquina, A.Marsat, S.Marteau, J.Martelli, F.Martinez, M.Martinez, V.Masserot, A.Mastrogiovanni, S.Meijer, Q.Menendez-Vazquez, A.Mereni, L.Merzougui, M.Miani, A.Michel, C.Milano, L.Miller, A.Miller, B.Milotti, E.Minenkov, Y.Mir, Ll. M.Miravet-Tenés, M.Montani, M.Morawski, F.Mours, B.Mow-Lowry, C. M.Muciaccia, F.Mukherjee, SuvodipMukund, N.Musenich, R.Nagar, A.Napolano, V.Nardecchia, I.Narola, H.Naticchioni, L.Neilson, J.Nguyen, C.Nissanke, S.Nitoglia, E.Nocera, F.Oganesyan, G.Olivetto, C.Olivieri, M.Pagano, G.Pagliaroli, G.Palomba, C.Pang, P. T. H.Pannarale, F.Paoletti, F.Paoli, A.Paolone, A.Pappas, G.Pascucci, D.Pasqualetti, A.Passaquieti, R.Passuello, D.Patricelli, B.Pedurand, R.Pegoraro, M.Perego, A.Pereira, A.Périgois, C.Perreca, A.Perriès, S.Pesios, D.Phukon, K. S.Piccinni, O. J.Pichot, M.Piendibene, M.Piergiovanni, F.Pierini, L.Pierro, V.Pillant, G.Pillas, M.Pilo, F.Pinard, L.Pinto, I. M.Pinto, M.Piotrzkowski, K.Placidi, A.Placidi, E.Plastino, W.Poggiani, R.Polini, E.Porter, E. K.Poulton, R.Pracchia, M.Pradier, T.Principe, M.Prodi, G. A.Prosposito, P.Puecher, A.Punturo, M.Puosi, F.Puppo, P.Raaijmakers, G.Radulesco, N.Rapagnani, P.Razzano, M.Regimbau, T.Rei, L.Rettegno, P.Revenu, B.Reza, A.Ricci, F.Riemenschneider, G.Rinaldi, S.Robinet, F.Rocchi, A.Rolland, L.Romanelli, M.Romano, R.Romero, A.Ronchini, S.Rosa, L.Rosińska, D.Roy, S.Rozza, D.Ruggi, P.Salafia, O. S.Salconi, L.Salemi, F.Samajdar, A.Sanchis-Gual, N.Sanuy, A.Sassolas, B.Sayah, S.Schmidt, S.Seglar-Arroyo, M.Sentenac, D.Sequino, V.Setyawati, Y.Sharma, A.Shcheblanov, N. S.Sieniawska, M.Silenzi, L.Singh, N.Singha, A.Sipala, V.Soldateschi, J.Sordini, V.Sorrentino, F.Sorrentino, N.Soulard, R.Spagnuolo, V.Spera, M.Spinicelli, P.Stachie, C.Steer, D. A.Steinlechner, J.Steinlechner, S.Stergioulas, N.Stratta, G.Suchenek, M.Sur, A.Swinkels, B. L.Szewczyk, P.Tacca, M.Tanasijczuk, A. J.Martín, E. N. Tapia SanTaranto, C.Thorne, K.Tonelli, M.Torres-Forné, A.Melo, I. Tosta eTrapananti, A.Travasso, F.Tringali, M. C.Troiano, L.Trovato, A.Trozzo, L.Tsang, K. W.Turbang, K.Turconi, M.Utina, A.Valentini, M.van Bakel, N.van Beuzekom, M.van Dael, M.Brand, J. F. J. van denBroeck, C. Van Denvan Haevermaet, H.van Heijningen, J. V.van Remortel, N.Vardaro, M.Vasúth, M.Vedovato, G.Verkindt, D.Verma, P.Vetrano, F.Viceré, A.Vinet, J. -Y.Virtuoso, A.Vocca, H.Walet, R. C.Was, M.Zadrożny, A.Zelenova, T.Zendri, J. -P.
Source
Subject
General Relativity and Quantum Cosmology
Astrophysics - Instrumentation and Methods for Astrophysics
Language
Abstract
Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient sensitivity worsening and gaps in data taking. During the one year-long third Observing Run (O3: from April 01, 2019 to March 27, 2020), the Virgo Collaboration collected a statistically significant dataset, used in this article to study the response of the detector to a variety of environmental conditions. We correlated environmental parameters to global detector performance, such as observation range, duty cycle and control losses. Where possible, we identified weaknesses in the detector that will be used to elaborate strategies in order to improve Virgo robustness against external disturbances for the next data taking period, O4, currently planned to start at the end of 2022. The lessons learned could also provide useful insights for the design of the next generation of ground-based interferometers.
Comment: 49 pages, 27 figures. Published in Classical and Quantum Grav