6533b830fe1ef96bd1296775

RESEARCH PRODUCT

The advanced Virgo longitudinal control system for the O2 observing run

D. VerkindtJan HarmsV. DattiloS. AntierTomasz BulikA. PasqualettiAlessandro LongoNicolas Sanchis-gualB. L. SwinkelsSebastiano BernuzziFrançois BonduF. BadaraccoYann BouffanaisO. HalimA. BrilletF. BrighentiK. W. TsangM. VardaroAniello GradoAlessandro NagarG. GrecoF. RobinetM. BoerD. BuskulicE. CuocoM. Llorens-monteagudoFausto AcerneseM. CieślarShubhanshu TiwariM. MontaniH. J. BultenA. PeregoM. MantovaniC. PalombaS. AscenziA. SurP. PuppoEttore MajoranaF. MessinaF. MessinaA. SamajdarA. KrólakB. D'angeloS. KoleyR. PedurandR. PedurandJ. M. Gonzalez CastroD. PascucciM. BitossiM. BranchesiTristan BriantMandar PatilM. PunturoPatrick Das GuptaM. EisenmannV. FafoneF. Di RenzoE. GeninF. BaldacciniWolfango PlastinoF. RicciDavid Jonathan HofmanOlivier MinazzoliF. ClevaM. PichotYing GuoArchisman GhoshFelice SorrentinoM. CroquetteMarco BazzanL. PinardF. GarufiA. R. WilliamsonM. RazzanoV. HuiA. PerrecaG. GemmeAnthony A. AmatoN. Van BakelM. DragoG. BogaertR. De RosaI. NardecchiaB. A. BoomR. MetzdorffA. GrimaldiV. ManganoGianpietro CagnoliGiuseppe IntiniC. De RossiL. RollandAlessandro BertoliniI. KhanValérie MartinezF. MartelliJosé A. FontF. L. LindeD. RosińskaCesare BarbieriCesare BarbieriA. IessDaniele A. SteerInnocenzo M. PintoFabrizio BaronePatrice HelloG. PagliaroliSteven BloemenJ. P. ZendriN. ManT. ZelenovaF. VetranoJ.-g. DucoinE. Chassande-mottinSylvain MarsatR. C. WaletVincenzo PierroD. FiorucciN. SinghI. Di PalmaS. Di PaceStefan GrimmA. SinghalL. ReiGijs NelemansA. K. ZadrożnyL. MilanoV. BoschiAlejandro Torres-fornéW. Del PozzoEnrico CalloniP. F. CohadonH. HeitmannL. SalconiPiotr JaranowskiPiero RettegnoM. GranataL. AielloI. MaksimovicG. HemmingD. HuetM. Van BeuzekomIsabel Cordero-carriónT. HarderR. GouatyA. Lartaux-vollardA. KutyniaJ. Casanueva DiazI. FerranteC. Van Den BroeckG. KoekoekP. BaconA. Di LietoD. LaghiM. LorenziniA. MasserotS. KatsanevasJ. NeilsonBenoit SassolasM. VasúthThibaut JacqminM. MerzouguiB. PatricelliMaurizio CanepaAntonio MarquinaE. M. SantosP. LeaciTanja HindererMiguel-ángel AloyN. LetendreMatteo BreschiFabien KéfélianI. BelahceneR. CavalieriJ. BrooksF. Di GiovanniF. CarbognaniStanislav BabakD. BersanettiSamuel DelégliseL. Di FioreAntoine HeidmannA. BastiM. BarsugliaFangchen FengJ.-p. CoulonFrancesco PannaraleM. C. TringaliM. BawajPaul J. GrootRosalba FittipaldiV. SequinoR. J. G. JonkerJ.-d. FournierA. RocchiA. ChincariniC. MichelJ. M. IsacMarica ValentiniL. TrozzoJ. F. J. Van Den BrandR. PassaquietiTania RegimbauA. PaoliA. MacquetTim DietrichN. ArnaudM. TaccaMartin ObergaulingerGiovanni CarapellaG. CianiI. FioriJ. MeidamM. GosselinS. CaudillP. RapagnaniSamaya NissankeGregorio CarulloM. A. BizouardG. A. ProdiF. PiergiovanniC. BuyRosa PoggianiV. FreyJ.-y. VinetN. RadulescuM. DavierSilvia CorezziF. CavalierE. CocciaS. FarinonE. Mejuto VillaC. Di GiorgioC. PérigoisD. SentenacO. SauterM. ArèneDániel BartaF. NoceraVincenzo FiumaraM. ColpiM. ColpiO. J. PiccinniA. BozziM. BejgerM. BejgerM. TonelliM. BischiL. MereniF. PaolettiM. AgathosF. TravassoP. RuggiMichela MapelliGunnar RiemenschneiderA. MianiSheon ChuaR. BonnandL. ErricoF. FidecaroG. M. GuidiFilip MorawskiG. BallardinM. Di GiovanniD. CorreR. De PietriR. De PietriRocco RomanoG. PaganoO. S. SalafiaO. S. SalafiaO. S. SalafiaFabrizio BobbaF. AubinG. StrattaM. De LaurentisA. MillerL. Van Der SchaafPablo Cerdá-duránB. MoursA. ChiummoS. MastrogiovanniLuca GammaitoniM. RomanelliG. LosurdoG. G. FronzéM. K. M. BaderO. ChaibiS. FrascaL. ContiGor OganesyanT. Di GirolamoEdward K. PorterF. MuciacciaAnupam SharmaNelson ChristensenC. StachieB. IdzkowskiV. LorietteS. D'antonioNandita KhetanA. GennaiDavid CohenD. PassuelloA. CironeE. CesariniF. MarionN. LeroyM. SieniawskaFabio MarchesoniP. GruningMario SperaD. LumacaGeert RaaijmakersOfelia DuranteA. AlloccaDavid A. NicholsSamuele CorteseM. WasJ. BairdH. VoccaA. ViceréRiccardo CiolfiPeter T. H. PangL. NaticchioniF. FrasconiR. FlaminioC. LazzaroPatricia SchmidtA. TrovatoG. VedovatoBruno GiacomazzoG. CellaC. BradaschiaC. NguyenP. AstoneY. MinenkovF. CiprianoP. PopolizioG. PillantD. EstevezJerome DegallaixC. Casentini

subject

neutron star: binaryPhysics::Instrumentation and DetectorsAstronomycavity: opticalSuspended optical cavities01 natural sciencesGravitational wave detectorsoff-lineGravitational wave detectors; Interferometer; Suspended optical cavities; Control loopsControl loopSuspended optical cavitieLIGOInterferometer010303 astronomy & astrophysicsdetectorsSettore FIS/01Physics[PHYS]Physics [physics]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsGravitational wave detectors Interferometer Suspended optical cavities Control loopsGravitational wave detectorUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradecontrol systemGravitational wavelongitudinalAstrophysics::High Energy Astrophysical PhenomenainterferometerAstrophysics::Cosmology and Extragalactic Astrophysicscontrol loops; gravitational wave detectors; interferometer; suspended optical cavitiesgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescence0103 physical sciencesControl loops[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and AstrophysicssensitivityLIGOgravitational radiation detectordetector: sensitivityNeutron star* Automatic Keywords *VIRGOblack hole: binaryControl systemgravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

description

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.

yearjournalcountryeditionlanguage
2020-03-01
10.1016/j.astropartphys.2019.07.005https://hal.science/hal-02491265