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Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During the August 2017 science run, Advanced Virgo detected its first gravitational wave signal, with the binary black hole merger, GW170729. This paper describes the control of the longitudinal degrees of freedom in the Advanced Virgo instrument during the O2 science run and the process that brought the detector from an uncontrolled, non-resonant state to its target working point.

The advanced Virgo longitudinal control system for the O2 observing run

Barone F.;Bertolini A.;Bobba F.;Bozzi A.;Canepa M.;Carapella G.;Cesarini E.;Cirone A.;Corezzi S.;Di Giorgio C.;Di Giovanni F.;Di Lieto A.;Drago M.;Ferrante I.;Fittipaldi R.;Granata M.;Grimaldi A.;Khan I.;Laghi D.;Mantovani M.;Messina F.;Miller A.;Pagano G.;Romano R.;Sharma A.;Spera M.;Tiwari S.;Tonelli M.;
2020

Abstract

Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During the August 2017 science run, Advanced Virgo detected its first gravitational wave signal, with the binary black hole merger, GW170729. This paper describes the control of the longitudinal degrees of freedom in the Advanced Virgo instrument during the O2 science run and the process that brought the detector from an uncontrolled, non-resonant state to its target working point.
Campo DC Valore Lingua
dc.authority.ancejournal ASTROPARTICLE PHYSICS en
dc.authority.orgunit Istituto Superconduttori, materiali innovativi e dispositivi - SPIN - Sede Secondaria Fisciano en
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dc.collection.id.s b3f88f24-048a-4e43-8ab1-6697b90e068e *
dc.collection.name 01.01 Articolo in rivista *
dc.contributor.appartenenza ASR - Unità Pianificazione, Programmazione e Biblioteca Centrale *
dc.contributor.appartenenza ASR - Unità Comunicazione *
dc.contributor.appartenenza Area di Ricerca NAPOLI 1 *
dc.contributor.appartenenza Dipartimento di Scienze del Sistema Terra e Tecnologie per l'Ambiente - DSSTTA *
dc.contributor.appartenenza Istituto Nanoscienze - NANO *
dc.contributor.appartenenza Istituto Nazionale di Ottica - INO *
dc.contributor.appartenenza Istituto Officina dei Materiali - IOM - *
dc.contributor.appartenenza Istituto Superconduttori, materiali innovativi e dispositivi - SPIN *
dc.contributor.appartenenza Istituto Superconduttori, materiali innovativi e dispositivi - SPIN - Sede Secondaria Fisciano *
dc.contributor.appartenenza Istituto di Calcolo e Reti ad Alte Prestazioni - ICAR *
dc.contributor.appartenenza Istituto di Chimica dei Composti OrganoMetallici - ICCOM - *
dc.contributor.appartenenza Istituto di Geologia Ambientale e Geoingegneria - IGAG *
dc.contributor.appartenenza Istituto di Ricerca per la Protezione Idrogeologica - IRPI - Sede Secondaria Padova *
dc.contributor.appartenenza Istituto di Ricerca sugli Ecosistemi Terrestri - IRET - Sede Secondaria Pisa *
dc.contributor.appartenenza Istituto di Scienze dell'Atmosfera e del Clima - ISAC *
dc.contributor.appartenenza Istituto di Struttura della Materia - ISM - Sede Roma Tor Vergata *
dc.contributor.appartenenza Istituto di linguistica computazionale "Antonio Zampolli" - ILC *
dc.contributor.appartenenza Istituto per il Rilevamento Elettromagnetico dell'Ambiente - IREA *
dc.contributor.appartenenza Istituto per la Microelettronica e Microsistemi - IMM *
dc.contributor.appartenenza Istituto per la Protezione Sostenibile delle Piante - IPSP *
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dc.date.accessioned 2024/12/06 14:51:21 -
dc.date.available 2024/12/06 14:51:21 -
dc.date.firstsubmission 2024/12/06 14:06:08 *
dc.date.issued 2020 -
dc.date.submission 2024/12/06 14:29:50 *
dc.description.abstracteng Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During the August 2017 science run, Advanced Virgo detected its first gravitational wave signal, with the binary black hole merger, GW170729. This paper describes the control of the longitudinal degrees of freedom in the Advanced Virgo instrument during the O2 science run and the process that brought the detector from an uncontrolled, non-resonant state to its target working point. -
dc.description.allpeople Acernese, F.; Agathos, M.; Aiello, L.; Allocca, A.; Aloy, M. A.; Amato, A.; Antier, S.; Arene, M.; Arnaud, N.; Ascenzi, S.; Astone, P.; Aubin, F.; Babak, S.; Bacon, P.; Badaracco, F.; Bader, M. K. M.; Baird, J.; Baldaccini, F.; Ballardin, G.; Barbieri, C.; Barone, F.; Barsuglia, M.; Barta, D.; Basti, A.; Bawaj, M.; Bazzan, M.; Bejger, M.; Belahcene, I.; Bernuzzi, S.; Bersanetti, D.; Bertolini, A.; Bischi, M.; Bitossi, M.; Bizouard, M. A.; Bloemen, S.; Bobba, F.; Boer, M.; Bogaert, G.; Bondu, F.; Bonnand, R.; Boom, B. A.; Boschi, V.; Bouffanais, Y.; Bozzi, A.; Bradaschia, C.; Branchesi, M.; Breschi, M.; Briant, T.; Brighenti, F.; Brillet, A.; Brooks, J.; Bulik, T.; Bulten, H. J.; Buskulic, D.; Buy, C.; Cagnoli, G.; Calloni, E.; Canepa, M.; Carapella, G.; Carbognani, F.; Carullo, G.; Casanueva Diaz, J.; Casentini, C.; Caudill, S.; Cavalier, F.; Cavalieri, R.; Cella, G.; Cerda-Duran, P.; Cesarini, E.; Chaibi, O.; Chassande-Mottin, E.; Chincarini, A.; Chiummo, A.; Christensen, N.; Chua, S.; Ciani, G.; Cieslar, M.; Ciolfi, R.; Cipriano, F.; Cirone, A.; Cleva, F.; Coccia, E.; Cohadon, P. -F.; Cohen, D.; Colpi, M.; Conti, L.; Cordero-Carrion, I.; Corezzi, S.; Corre, D.; Cortese, S.; Coulon, J. -P.; Croquette, M.; Cuoco, E.; Dangelo, B.; D'Antonio, S.; Dattilo, V.; Davier, M.; Degallaix, J.; De Laurentis, M.; Deleglise, S.; Del Pozzo, W.; De Pietri, R.; De Rosa, R.; De Rossi, C.; Dietrich, T.; Di Fiore, L.; Di Giorgio, C.; Di Giovanni, F.; Di Giovanni, M.; Di Girolamo, T.; Di Lieto, A.; Di Pace, S.; Di Palma, I.; Di Renzo, F.; Drago, M.; Ducoin, J. -G.; Durante, O.; Eisenmann, M.; Errico, L.; Estevez, D.; Fafone, V.; Farinon, S.; Feng, F.; Ferrante, I.; Fidecaro, F.; Fiori, I.; Fiorucci, D.; Fittipaldi, R.; Fiumara, V.; Flaminio, R.; Font, J. A.; Fournier, J. -D.; Frasca, S.; Frasconi, F.; Frey, V.; Fronze, G.; Gammaitoni, L.; Garufi, F.; Gemme, G.; Genin, E.; Gennai, A.; Ghosh, A.; Giacomazzo, B.; Gonzalez Castro, J. M.; Gosselin, M.; Gouaty, R.; Grado, A.; Granata, M.; Greco, G.; Grimaldi, A.; Grimm, S. J.; Groot, P.; Gruning, P.; Guidi, G. M.; Guo, Y.; Gupta, P.; Halim, O.; Harder, T.; Harms, J.; Heidmann, A.; Heitmann, H.; Hello, P.; Hemming, G.; Hinderer, T.; Hofman, D.; Huet, D.; Hui, V.; Idzkowski, B.; Iess, A.; Intini, G.; Isac, J. -M.; Jacqmin, T.; Jaranowski, P.; Jonker, R. J. G.; Katsanevas, S.; Kefelian, F.; Khan, I.; Khetan, N.; Koekoek, G.; Koley, S.; Krolak, A.; Kutynia, A.; Laghi, D.; Lartaux-Vollard, A.; Lazzaro, C.; Leaci, P.; Leroy, N.; Letendre, N.; Linde, F.; Llorens-Monteagudo, M.; Longo, A.; Lorenzini, M.; Loriette, V.; Losurdo, G.; Lumaca, D.; Macquet, A.; Majorana, E.; Maksimovic, I.; Man, N.; Mangano, V.; Mantovani, M.; Mapelli, M.; Marchesoni, F.; Marion, F.; Marquina, A.; Marsat, S.; Martelli, F.; Martinez, V.; Masserot, A.; Mastrogiovanni, S.; Meidam, J.; Mejuto Villa, E.; Mereni, L.; Merzougui, M.; Messina, F.; Metzdorff, R.; Miani, A.; Michel, C.; Milano, L.; Miller, A.; Minazzoli, O.; Minenkov, Y.; Montani, M.; Morawski, F.; Mours, B.; Muciaccia, F.; Nagar, A.; Nardecchia, I.; Naticchioni, L.; Neilson, J.; Nelemans, G.; Nguyen, C.; Nichols, D.; Nissanke, S.; Nocera, F.; Obergaulinger, M.; Oganesyan, G.; Pagano, G.; Pagliaroli, G.; Palomba, C.; Pang, P. T. H.; Pannarale, F.; Paoletti, F.; Paoli, A.; Pascucci, D.; Pasqualetti, A.; Passaquieti, R.; Passuello, D.; Patil, M.; Patricelli, B.; Pedurand, R.; Perego, A.; Perigois, C.; Perreca, A.; Piccinni, O. J.; Pichot, M.; Piergiovanni, F.; Pierro, V.; Pillant, G.; Pinard, L.; Pinto, I. M.; Plastino, W.; Poggiani, R.; Popolizio, P.; Porter, E. K.; Prodi, G. A.; Punturo, M.; Puppo, P.; Raaijmakers, G.; Radulescu, N.; Rapagnani, P.; Razzano, M.; Regimbau, T.; Rei, L.; Rettegno, P.; Ricci, F.; Riemenschneider, G.; Robinet, F.; Rocchi, A.; Rolland, L.; Romanelli, M.; Romano, R.; Rosinska, D.; Ruggi, P.; Salafia, O. S.; Salconi, L.; Samajdar, A.; Sanchis-Gual, N.; Santos, E.; Sassolas, B.; Sauter, O.; Schmidt, P.; Sentenac, D.; Sequino, V.; Sharma, A.; Sieniawska, M.; Singh, N.; Singhal, A.; Sorrentino, F.; Spera, M.; Stachie, C.; Steer, D. A.; Stratta, G.; Sur, A.; Swinkels, B. L.; Tacca, M.; Tiwari, S.; Tonelli, M.; Torres-Forne, A.; Travasso, F.; Tringali, M. C.; Trovato, A.; Trozzo, L.; Tsang, K. W.; Valentini, M.; van Bakel, N.; van Beuzekom, M.; van den Brand, J. F. J.; Van Den Broeck, C.; van der Schaaf, L.; Vardaro, M.; Vasuth, M.; Vedovato, G.; Verkindt, D.; Vetrano, F.; Vicere, A.; Vinet, J. -Y.; Vocca, H.; Walet, R.; Was, M.; Williamson, A. R.; Zadrozny, A.; Zelenova, T.; Zendri, J. -P. -
dc.description.allpeopleoriginal Acernese F.; Agathos M.; Aiello L.; Allocca A.; Aloy M.A.; Amato A.; Antier S.; Arene M.; Arnaud N.; Ascenzi S.; Astone P.; Aubin F.; Babak S.; Bacon P.; Badaracco F.; Bader M.K.M.; Baird J.; Baldaccini F.; Ballardin G.; Barbieri C.; Barone F.; Barsuglia M.; Barta D.; Basti A.; Bawaj M.; Bazzan M.; Bejger M.; Belahcene I.; Bernuzzi S.; Bersanetti D.; Bertolini A.; Bischi M.; Bitossi M.; Bizouard M.A.; Bloemen S.; Bobba F.; Boer M.; Bogaert G.; Bondu F.; Bonnand R.; Boom B.A.; Boschi V.; Bouffanais Y.; Bozzi A.; Bradaschia C.; Branchesi M.; Breschi M.; Briant T.; Brighenti F.; Brillet A.; Brooks J.; Bulik T.; Bulten H.J.; Buskulic D.; Buy C.; Cagnoli G.; Calloni E.; Canepa M.; Carapella G.; Carbognani F.; Carullo G.; Casanueva Diaz J.; Casentini C.; Caudill S.; Cavalier F.; Cavalieri R.; Cella G.; Cerda-Duran P.; Cesarini E.; Chaibi O.; Chassande-Mottin E.; Chincarini A.; Chiummo A.; Christensen N.; Chua S.; Ciani G.; Cieslar M.; Ciolfi R.; Cipriano F.; Cirone A.; Cleva F.; Coccia E.; Cohadon P.-F.; Cohen D.; Colpi M.; Conti L.; Cordero-Carrion I.; Corezzi S.; Corre D.; Cortese S.; Coulon J.-P.; Croquette M.; Cuoco E.; DAngelo B.; D'Antonio S.; Dattilo V.; Davier M.; Degallaix J.; De Laurentis M.; Deleglise S.; Del Pozzo W.; De Pietri R.; De Rosa R.; De Rossi C.; Dietrich T.; Di Fiore L.; Di Giorgio C.; Di Giovanni F.; Di Giovanni M.; Di Girolamo T.; Di Lieto A.; Di Pace S.; Di Palma I.; Di Renzo F.; Drago M.; Ducoin J.-G.; Durante O.; Eisenmann M.; Errico L.; Estevez D.; Fafone V.; Farinon S.; Feng F.; Ferrante I.; Fidecaro F.; Fiori I.; Fiorucci D.; Fittipaldi R.; Fiumara V.; Flaminio R.; Font J.A.; Fournier J.-D.; Frasca S.; Frasconi F.; Frey V.; Fronze G.; Gammaitoni L.; Garufi F.; Gemme G.; Genin E.; Gennai A.; Ghosh A.; Giacomazzo B.; Gonzalez Castro J.M.; Gosselin M.; Gouaty R.; Grado A.; Granata M.; Greco G.; Grimaldi A.; Grimm S.J.; Groot P.; Gruning P.; Guidi G.M.; Guo Y.; Gupta P.; Halim O.; Harder T.; Harms J.; Heidmann A.; Heitmann H.; Hello P.; Hemming G.; Hinderer T.; Hofman D.; Huet D.; Hui V.; Idzkowski B.; Iess A.; Intini G.; Isac J.-M.; Jacqmin T.; Jaranowski P.; Jonker R.J.G.; Katsanevas S.; Kefelian F.; Khan I.; Khetan N.; Koekoek G.; Koley S.; Krolak A.; Kutynia A.; Laghi D.; Lartaux-Vollard A.; Lazzaro C.; Leaci P.; Leroy N.; Letendre N.; Linde F.; Llorens-Monteagudo M.; Longo A.; Lorenzini M.; Loriette V.; Losurdo G.; Lumaca D.; Macquet A.; Majorana E.; Maksimovic I.; Man N.; Mangano V.; Mantovani M.; Mapelli M.; Marchesoni F.; Marion F.; Marquina A.; Marsat S.; Martelli F.; Martinez V.; Masserot A.; Mastrogiovanni S.; Meidam J.; Mejuto Villa E.; Mereni L.; Merzougui M.; Messina F.; Metzdorff R.; Miani A.; Michel C.; Milano L.; Miller A.; Minazzoli O.; Minenkov Y.; Montani M.; Morawski F.; Mours B.; Muciaccia F.; Nagar A.; Nardecchia I.; Naticchioni L.; Neilson J.; Nelemans G.; Nguyen C.; Nichols D.; Nissanke S.; Nocera F.; Obergaulinger M.; Oganesyan G.; Pagano G.; Pagliaroli G.; Palomba C.; Pang P.T.H.; Pannarale F.; Paoletti F.; Paoli A.; Pascucci D.; Pasqualetti A.; Passaquieti R.; Passuello D.; Patil M.; Patricelli B.; Pedurand R.; Perego A.; Perigois C.; Perreca A.; Piccinni O.J.; Pichot M.; Piergiovanni F.; Pierro V.; Pillant G.; Pinard L.; Pinto I.M.; Plastino W.; Poggiani R.; Popolizio P.; Porter E.K.; Prodi G.A.; Punturo M.; Puppo P.; Raaijmakers G.; Radulescu N.; Rapagnani P.; Razzano M.; Regimbau T.; Rei L.; Rettegno P.; Ricci F.; Riemenschneider G.; Robinet F.; Rocchi A.; Rolland L.; Romanelli M.; Romano R.; Rosinska D.; Ruggi P.; Salafia O.S.; Salconi L.; Samajdar A.; Sanchis-Gual N.; Santos E.; Sassolas B.; Sauter O.; Schmidt P.; Sentenac D.; Sequino V.; Sharma A.; Sieniawska M.; Singh N.; Singhal A.; Sorrentino F.; Spera M.; Stachie C.; Steer D.A.; Stratta G.; Sur A.; Swinkels B.L.; Tacca M.; Tiwari S.; Tonelli M.; Torres-Forne A.; Travasso F.; Tringali M.C.; Trovato A.; Trozzo L.; Tsang K.W.; Valentini M.; van Bakel N.; van Beuzekom M.; van den Brand J.F.J.; Van Den Broeck C.; van der Schaaf L.; Vardaro M.; Vasuth M.; Vedovato G.; Verkindt D.; Vetrano F.; Vicere A.; Vinet J.-Y.; Vocca H.; Walet R.; Was M.; Williamson A.R.; Zadrozny A.; Zelenova T.; Zendri J.-P. en
dc.description.fulltext restricted en
dc.description.numberofauthors 334 -
dc.identifier.doi 10.1016/j.astropartphys.2019.07.005 en
dc.identifier.isi WOS:000501416000001 -
dc.identifier.scopus 2-s2.0-85072763494 en
dc.identifier.source scopus *
dc.identifier.uri https://hdl.handle.net/20.500.14243/516176 -
dc.language.iso eng en
dc.relation.volume 116 en
dc.subject.keywords Control loops -
dc.subject.keywords Gravitational wave detectors -
dc.subject.keywords Interferometer -
dc.subject.keywords Suspended optical cavities -
dc.subject.singlekeyword Control loops *
dc.subject.singlekeyword Gravitational wave detectors *
dc.subject.singlekeyword Interferometer *
dc.subject.singlekeyword Suspended optical cavities *
dc.title The advanced Virgo longitudinal control system for the O2 observing run en
dc.type.driver info:eu-repo/semantics/article -
dc.type.full 01 Contributo su Rivista::01.01 Articolo in rivista it
dc.type.miur 262 -
iris.isi.extIssued 2020 -
iris.isi.extTitle The advanced Virgo longitudinal control system for the O2 observing run -
iris.isi.ideLinkStatusDate 2025/01/17 12:32:59 *
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iris.orcid.lastModifiedDate 2025/01/27 21:58:01 *
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iris.scopus.extIssued 2020 -
iris.scopus.extTitle The advanced Virgo longitudinal control system for the O2 observing run -
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iris.unpaywall.doi 10.1016/j.astropartphys.2019.07.005 *
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iris.unpaywall.pdfurl https://www.sciencedirect.com/science/article/pii/S0927650519301835 *
isi.authority.ancejournal ASTROPARTICLE PHYSICS###0927-6505 *
isi.category BU *
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isi.date.issued 2020 *
isi.description.abstracteng Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During the August 2017 science run, Advanced Virgo detected its first gravitational wave signal, with the binary black hole merger, GW170729. This paper describes the control of the longitudinal degrees of freedom in the Advanced Virgo instrument during the O2 science run and the process that brought the detector from an uncontrolled, non-resonant state to its target working point. (C) 2019 Elsevier B.V. All rights reserved. *
isi.description.allpeopleoriginal Acernese, F; Agathos, M; Aiello, L; Allocca, A; Aloy, MA; Amato, A; Antier, S; Arène, M; Arnaud, N; Ascenzi, S; Astone, P; Aubin, F; Babak, S; Bacon, P; Badaracco, F; Bader, MKM; Baird, J; Baldaccini, F; Ballardin, G; Barbieri, C; Barone, F; Barsuglia, M; Barta, D; Basti, A; Bawaj, M; Bazzan, M; Bejger, M; Belahcene,; Bernuzzi, S; Bersanetti, D; Bertolini, A; Bischi, M; Bitossi, M; Bizouard, MA; Bloemen, S; Bobba, F; Boer, M; Bogaert, G; Bondu, F; Bonnand, R; Boom, BA; Boschi,; Bouffanais, Y; Bozzi, A; Bradaschia, C; Branchesi, M; Breschi, M; Briant, T; Brighenti, F; Brillet, A; Brooks, J; Bulik, T; Bulten, HJ; Buskulic, D; Buy, C; Cagnoli, G; Calloni, E; Canepa, M; Carapella, G; Carbognani, F; Carullo, G; Diaz, JC; Casentini, C; Caudill, S; Cavalier, F; Cavalieri, R; Cella, G; Cerdá-Durán, P; Cesarini, E; Chaibi, O; Chassande-Mottin, E; Chincarini, A; Chiummo, A; Christensen, N; Chua, S; Ciani, G; Cieslar, M; Ciolfi, R; Cipriano, F; Cirone, A; Cleva, F; Coccia, E; Cohadon, PF; Cohen, D; Colpi, M; Conti, L; Cordero-Carrión,; Corezzi, S; Corre, D; Cortese, S; Coulon, JP; Croquette, M; Cuoco, E; DAngelo, B; D'Antonio, S; Dattilo,; Davier, M; Degallaix, J; De Laurentis, M; Deléglise, S; Del Pozzo, W; De Pietri, R; De Rosa, R; De Rossi, C; Dietrich, T; Di Fiore, L; Di Giorgio, C; Di Giovanni, F; Di Giovanni, M; Di Girolamo, T; Di Lieto, A; Di Pace, S; Di Palma,; Di Renzo, F; Drago, M; Ducoin, JG; Durante, O; Eisenmann, M; Errico, L; Estevez, D; Fafone,; Farinon, S; Feng, F; Ferrante,; Fidecaro, F; Fiori,; Fiorucci, D; Fittipaldi, R; Fiumara,; Flaminio, R; Font, JA; Fournier, JD; Frasca, S; Frasconi, F; Frey,; Fronzé, G; Gammaitoni, L; Garufi, F; Gemme, G; Genin, E; Gennai, A; Ghosh, A; Giacomazzo, B; Castro, JMG; Gosselin, M; Gouaty, R; Grado, A; Granata, M; Greco, G; Grimaldi, A; Grimm, SJ; Groot, P; Gruning, P; Guidi, GM; Guo, Y; Gupta, P; Halim, O; Harder, T; Harms, J; Heidmann, A; Heitmann, H; Hello, P; Hemming, G; Hinderer, T; Hofman, D; Huet, D; Hui,; Idzkowski, B; Iess, A; Intini, G; Isac, JM; Jacqmin, T; Jaranowski, P; Jonker, RJG; Katsanevas, S; Kéfélian, F; Khan,; Khetan, N; Koekoek, G; Koley, S; Królak, A; Kutynia, A; Laghi, D; Lartaux-Vollard, A; Lazzaro, C; Leaci, P; Leroy, N; Letendre, N; Linde, F; Llorens-Monteagudo, M; Longo, A; Lorenzini, M; Loriette,; Losurdo, G; Lumaca, D; Macquet, A; Majorana, E; Maksimovic,; Man, N; Mangano,; Mantovani, M; Mapelli, M; Marchesoni, F; Marion, F; Marquina, A; Marsat, S; Martelli, F; Martinez,; Masserot, A; Mastrogiovanni, S; Meidam, J; Villa, EM; Mereni, L; Merzougui, M; Messina, F; Metzdorff, R; Miani, A; Michel, C; Milano, L; Miller, A; Minazzoli, O; Minenkov, Y; Montani, M; Morawski, F; Mours, B; Muciaccia, F; Nagar, A; Nardecchia,; Naticchioni, L; Neilson, J; Nelemans, G; Nguyen, C; Nichols, D; Nissanke, S; Nocera, F; Obergaulinger, M; Oganesyan, G; Pagano, G; Pagliaroli, G; Palomba, C; Pang, PTH; Pannarale, F; Paoletti, F; Paoli, A; Pascucci, D; Pasqualetti, A; Passaquieti, R; Passuello, D; Patil, M; Patricelli, B; Pedurand, R; Perego, A; Périgois, C; Perreca, A; Piccinni, OJ; Pichot, M; Piergiovanni, F; Pierro,; Pillant, G; Pinard, L; Pinto, IM; Plastino, W; Poggiani, R; Popolizio, P; Porter, EK; Prodi, GA; Punturo, M; Puppo, P; Raaijmakers, G; Radulescu, N; Rapagnani, P; Razzano, M; Regimbau, T; Rei, L; Rettegno, P; Ricci, F; Riemenschneider, G; Robinet, F; Rocchi, A; Rolland, L; Romanelli, M; Romano, R; Rosinska, D; Ruggi, P; Salafia, OS; Salconi, L; Samajdar, A; Sanchis-Gual, N; Santos, E; Sassolas, B; Sauter, O; Schmidt, P; Sentenac, D; Sequino,; Sharma, A; Sieniawska, M; Singh, N; Singhal, A; Sorrentino, F; Spera, M; Stachie, C; Steer, DA; Stratta, G; Sur, A; Swinkels, BL; Tacca, M; Tiwari, S; Tonelli, M; Torres-Forné, A; Travasso, F; Tringali, MC; Trovato, A; Trozzo, L; Tsang, KW; Valentini, M; van Bakel, N; van Beuzekom, M; van den Brand, JFJ; Van Den Broeck, C; van der Schaaf, L; Vardaro, M; Vasúth, M; Vedovato, G; Verkindt, D; Vetrano, F; Viceré, A; Vinet, JY; Vocca, H; Walet, R; Was, M; Williamson, AR; Zadrozny, A; Zelenova, T; Zendri, JP; *
isi.document.sourcetype WOS.SCI *
isi.document.type Article *
isi.document.types Article *
isi.identifier.doi 10.1016/j.astropartphys.2019.07.005 *
isi.identifier.eissn 1873-2852 *
isi.identifier.isi WOS:000501416000001 *
isi.journal.journaltitle ASTROPARTICLE PHYSICS *
isi.journal.journaltitleabbrev ASTROPART PHYS *
isi.language.original English *
isi.publisher.place RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS *
isi.relation.volume 116 *
isi.title The advanced Virgo longitudinal control system for the O2 observing run *
scopus.authority.ancejournal ASTROPARTICLE PHYSICS###0927-6505 *
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scopus.date.issued 2020 *
scopus.description.abstracteng Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During the August 2017 science run, Advanced Virgo detected its first gravitational wave signal, with the binary black hole merger, GW170729. This paper describes the control of the longitudinal degrees of freedom in the Advanced Virgo instrument during the O2 science run and the process that brought the detector from an uncontrolled, non-resonant state to its target working point. *
scopus.description.allpeopleoriginal Acernese F.; Agathos M.; Aiello L.; Allocca A.; Aloy M.A.; Amato A.; Antier S.; Arene M.; Arnaud N.; Ascenzi S.; Astone P.; Aubin F.; Babak S.; Bacon P.; Badaracco F.; Bader M.K.M.; Baird J.; Baldaccini F.; Ballardin G.; Barbieri C.; Barone F.; Barsuglia M.; Barta D.; Basti A.; Bawaj M.; Bazzan M.; Bejger M.; Belahcene I.; Bernuzzi S.; Bersanetti D.; Bertolini A.; Bischi M.; Bitossi M.; Bizouard M.A.; Bloemen S.; Bobba F.; Boer M.; Bogaert G.; Bondu F.; Bonnand R.; Boom B.A.; Boschi V.; Bouffanais Y.; Bozzi A.; Bradaschia C.; Branchesi M.; Breschi M.; Briant T.; Brighenti F.; Brillet A.; Brooks J.; Bulik T.; Bulten H.J.; Buskulic D.; Buy C.; Cagnoli G.; Calloni E.; Canepa M.; Carapella G.; Carbognani F.; Carullo G.; Casanueva Diaz J.; Casentini C.; Caudill S.; Cavalier F.; Cavalieri R.; Cella G.; Cerda-Duran P.; Cesarini E.; Chaibi O.; Chassande-Mottin E.; Chincarini A.; Chiummo A.; Christensen N.; Chua S.; Ciani G.; Cieslar M.; Ciolfi R.; Cipriano F.; Cirone A.; Cleva F.; Coccia E.; Cohadon P.-F.; Cohen D.; Colpi M.; Conti L.; Cordero-Carrion I.; Corezzi S.; Corre D.; Cortese S.; Coulon J.-P.; Croquette M.; Cuoco E.; DAngelo B.; D'Antonio S.; Dattilo V.; Davier M.; Degallaix J.; De Laurentis M.; Deleglise S.; Del Pozzo W.; De Pietri R.; De Rosa R.; De Rossi C.; Dietrich T.; Di Fiore L.; Di Giorgio C.; Di Giovanni F.; Di Giovanni M.; Di Girolamo T.; Di Lieto A.; Di Pace S.; Di Palma I.; Di Renzo F.; Drago M.; Ducoin J.-G.; Durante O.; Eisenmann M.; Errico L.; Estevez D.; Fafone V.; Farinon S.; Feng F.; Ferrante I.; Fidecaro F.; Fiori I.; Fiorucci D.; Fittipaldi R.; Fiumara V.; Flaminio R.; Font J.A.; Fournier J.-D.; Frasca S.; Frasconi F.; Frey V.; Fronze G.; Gammaitoni L.; Garufi F.; Gemme G.; Genin E.; Gennai A.; Ghosh A.; Giacomazzo B.; Gonzalez Castro J.M.; Gosselin M.; Gouaty R.; Grado A.; Granata M.; Greco G.; Grimaldi A.; Grimm S.J.; Groot P.; Gruning P.; Guidi G.M.; Guo Y.; Gupta P.; Halim O.; Harder T.; Harms J.; Heidmann A.; Heitmann H.; Hello P.; Hemming G.; Hinderer T.; Hofman D.; Huet D.; Hui V.; Idzkowski B.; Iess A.; Intini G.; Isac J.-M.; Jacqmin T.; Jaranowski P.; Jonker R.J.G.; Katsanevas S.; Kefelian F.; Khan I.; Khetan N.; Koekoek G.; Koley S.; Krolak A.; Kutynia A.; Laghi D.; Lartaux-Vollard A.; Lazzaro C.; Leaci P.; Leroy N.; Letendre N.; Linde F.; Llorens-Monteagudo M.; Longo A.; Lorenzini M.; Loriette V.; Losurdo G.; Lumaca D.; Macquet A.; Majorana E.; Maksimovic I.; Man N.; Mangano V.; Mantovani M.; Mapelli M.; Marchesoni F.; Marion F.; Marquina A.; Marsat S.; Martelli F.; Martinez V.; Masserot A.; Mastrogiovanni S.; Meidam J.; Mejuto Villa E.; Mereni L.; Merzougui M.; Messina F.; Metzdorff R.; Miani A.; Michel C.; Milano L.; Miller A.; Minazzoli O.; Minenkov Y.; Montani M.; Morawski F.; Mours B.; Muciaccia F.; Nagar A.; Nardecchia I.; Naticchioni L.; Neilson J.; Nelemans G.; Nguyen C.; Nichols D.; Nissanke S.; Nocera F.; Obergaulinger M.; Oganesyan G.; Pagano G.; Pagliaroli G.; Palomba C.; Pang P.T.H.; Pannarale F.; Paoletti F.; Paoli A.; Pascucci D.; Pasqualetti A.; Passaquieti R.; Passuello D.; Patil M.; Patricelli B.; Pedurand R.; Perego A.; Perigois C.; Perreca A.; Piccinni O.J.; Pichot M.; Piergiovanni F.; Pierro V.; Pillant G.; Pinard L.; Pinto I.M.; Plastino W.; Poggiani R.; Popolizio P.; Porter E.K.; Prodi G.A.; Punturo M.; Puppo P.; Raaijmakers G.; Radulescu N.; Rapagnani P.; Razzano M.; Regimbau T.; Rei L.; Rettegno P.; Ricci F.; Riemenschneider G.; Robinet F.; Rocchi A.; Rolland L.; Romanelli M.; Romano R.; Rosinska D.; Ruggi P.; Salafia O.S.; Salconi L.; Samajdar A.; Sanchis-Gual N.; Santos E.; Sassolas B.; Sauter O.; Schmidt P.; Sentenac D.; Sequino V.; Sharma A.; Sieniawska M.; Singh N.; Singhal A.; Sorrentino F.; Spera M.; Stachie C.; Steer D.A.; Stratta G.; Sur A.; Swinkels B.L.; Tacca M.; Tiwari S.; Tonelli M.; Torres-Forne A.; Travasso F.; Tringali M.C.; Trovato A.; Trozzo L.; Tsang K.W.; Valentini M.; van Bakel N.; van Beuzekom M.; van den Brand J.F.J.; Van Den Broeck C.; van der Schaaf L.; Vardaro M.; Vasuth M.; Vedovato G.; Verkindt D.; Vetrano F.; Vicere A.; Vinet J.-Y.; Vocca H.; Walet R.; Was M.; Williamson A.R.; Zadrozny A.; Zelenova T.; Zendri J.-P. *
scopus.differences scopus.subject.keywords *
scopus.document.type ar *
scopus.document.types ar *
scopus.identifier.doi 10.1016/j.astropartphys.2019.07.005 *
scopus.identifier.pui 2003171256 *
scopus.identifier.scopus 2-s2.0-85072763494 *
scopus.journal.sourceid 26764 *
scopus.language.iso eng *
scopus.publisher.name Elsevier B.V. *
scopus.relation.article 102386 *
scopus.relation.volume 116 *
scopus.subject.keywords Control loops; Gravitational wave detectors; Interferometer; Suspended optical cavities; *
scopus.title The advanced Virgo longitudinal control system for the O2 observing run *
scopus.titleeng The advanced Virgo longitudinal control system for the O2 observing run *
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