{"paper":{"title":"Characterization of the Virgo Seismic Environment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"A. Basti, A. Belletoile, A. Brillet, A. Chincarini, A. Chiummo, A. Colla, A. Conte, A. Dietz, A. Di Lieto, A. Di Virgilio, A. Gennai, A. Giazotto, A. Heidmann, A. Krolak, A. Masserot, A. Morgia, A. Pasqualetti, A. Rocchi, A. Toncelli, A. Vicere, A. Zadrozny, B. Bouhou, B. Canuel, B. Mours, B. Sassolas, B. Swinkels, C. Bradaschia, C. Buy, C. Greverie, C. Michel, C. N. Colacino, C. Palomba, C. Van Den Broeck, D. Buskulic, D. Passuello, D. Rosinska, D. Sentenac, D. S. Rabeling, D. Verkindt, E. Calloni, E. Cesarini, E. Chassande-Mottin, E. Coccia, E. Cuoco, E. Genin, E. Majorana, E. Tournefier, F. Acernese, F. Barone, F. Bondu, F. Carbognani, F. Cavalier, F. Cleva, F. Fidecaro, F. Frasconi, F. Garufi, F. Marchesoni, F. Marion, F. Martelli, F. Nocera, F. Paoletti, F. Piergiovanni, F. Ricci, F. Robinet, F. Travasso, F. Vetrano, G. A. Prodi, G. Ballardin, G. Cagnoli, G. Cella, G. Debreczeni, G. Endroczi, G. Gemme, G. Losurdo, G. M. Guidi, G. Pagliaroli, G. Persichetti, G. Vajente, G. Vedovato, H. Heitmann, H. J. Bulten, H. Vocca, I. Ferrante, I. Fiori, I. Kowalska, I. Maksimovic, I. Racz, J. Colas, J.-D. Fournier, J.-F. Hayau, J. F. J. van den Brand, J. Franc, J. Marque, J.-P. Coulon, J.-P. Zendri, J.-Y. Vinet, L. A. Forte, L. Bonelli, L. Bosi, L. Di Fiore, L. Gammaitoni, L. Milano, L. Naticchioni, L. Palladino, L. Pinard, L. Rolland, L. Sperandio, L. Taffarello, M. A. Bizouard, M. Barsuglia, M. Bebronne, M. Bitossi, M. Blom, M. Branchesi, M. Colombini, M. Coughlin, M. Davier, M. Del Prete, M. Di Paolo Emilio, M. Drago, M. E. Gaspar, M. Galimberti, M.G. Beker, M. Granata, M. Lorenzini, M. Mantovani, M. Mohan, M. Parisi, M. Pietka, M. Prato, M. Punturo, M. Tacca, M. Tonelli, M. Vasuth, M. Vavoulidis, M. Was, M. Yvert, N. Leroy, N. Letendre, N. Liguori, N. Man, N. Morgado, O. Chaibi, O. Torre, P. Astone, P.-F. Cohadon, P. Hello, P. Jaranowski, P. Puppo, P. Rapagnani, P. Ruggi, R. Bonnand, R. Cavalieri, R. Day, R. De Rosa, R. Flaminio, R. Gouaty, R. L. Ward, R. Passaquieti, R. Poggiani, R. Romano, R. Sturani, S. Braccini, S. DAntonio, S. Frasca, S. Mosca, S. van der Putten, S. Vitale, T. Briant, T. Bulik, T. G. F. Li, The Virgo Collaboration: T. Accadia, Th. S. Bauer, T. Regimbau, V. Boschi, V. Brisson, V. Dattilo, V. Fafone, V. Loriette, V. Re, W. Del Pozzo, Y. Minenkov","submitted_at":"2011-08-08T02:35:08Z","abstract_excerpt":"The Virgo gravitational wave detector is an interferometer (ITF) with 3km arms located in Pisa, Italy. From July to October 2010, Virgo performed its third science run (VSR3) in coincidence with the LIGO detectors. Despite several techniques adopted to isolate the interferometer from the environment, seismic noise remains an important issue for Virgo. Vibrations produced by the detector infrastructure (such as air conditioning units, water chillers/heaters, pumps) are found to affect Virgo's sensitivity, with the main coupling mechanisms being through beam jitter and scattered light processes."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.1598","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}