The first six months of the Advanced LIGO’s and Advanced Virgo’s third observing run with GRANDMA
S. AntierAPC, Univ. Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne, 75013 Paris Cité, FranceS. AgayevaN.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, AzerbaijanV. AivazyanE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaS. AlishovN.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, AzerbaijanEmmanuel ArbouchUPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, F-75014 Paris, FranceA. BaranskyAstronomical Observatory, Taras Shevshenko National University of Kyiv, Observatorna str. 3, Kyiv UA-04053, UkraineK. BarynovaNuclear Physics Department, Taras Shevchenko National University of Kyiv, 60 Volodymyrska str., Kyiv UA-01601, UkraineJ. M. BaiYunnan Astronomical Observatories/Chinese Academy of Science, Kunming 650011, ChinaS. BasaLaboratoire d’Astrophysique de Marseille, UMR 7326, CNRS, Université d’Aix Marseille, 38, rue Frédéric Joliot-Curie,Marseille, FranceS. BeradzeE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaE. BertinUPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, F-75014 Paris, FranceJ. BerthierM. BłażekInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, SpainM. BoërARTEMIS UMR 7250 UCA CNRS OCA, Boulevard de l’Observatoire, CS 34229, 06304 Nice CEDEX 04, FranceО. БурхоновUlugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy str. 33, Tashkent 100052, UzbekistanA. G. BurrellOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaA. CailleauIRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F-31400 Toulouse, FranceB. ChabertOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaJ. C. ChenWuZhou University, Wuzhou, Guangxi 543000, ChinaN. ChristensenARTEMIS UMR 7250 UCA CNRS OCA, Boulevard de l’Observatoire, CS 34229, 06304 Nice CEDEX 04, FranceA. ColeiroAPC, Univ. Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne, 75013 Paris Cité, FranceB. CordierAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, FranceD. CorreLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceM. W. CoughlinCalifornia Institute of Technology, 1200 East California Blvd, MC 249-17, Pasadena, CA 91125, USAD. M. CowardOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaH. CrispARC Centre of Excellence for Gravitational Wave DiscoveryC. DelattreTim DietrichNikhef, Science Park, NL-1098 XG Amsterdam, the NetherlandsJ.-G. DucoinLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceP.-A. DuverneLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceG Marchal-DuvalLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceB. GendreOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaL. EymarARTEMIS UMR 7250 UCA CNRS OCA, Boulevard de l’Observatoire, CS 34229, 06304 Nice CEDEX 04, FranceP. Fock-HangX. H. HanNational Astronomical Observatories/Chinese Academy of Science 20A Datun Road, Beijing 100012, ChinaP. HelloLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceE. J. HowellOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaR. InasaridzeE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaН. З. ИсмаиловN.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, AzerbaijanД. А. КаннInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, SpainG. V. KapanadzeE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaA. KlotzIRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F-31400 Toulouse, FranceN. KochiashviliE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaC. LachaudAPC, Univ. Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne, 75013 Paris Cité, FranceN. LeroyLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceA Le Van SuLaboratoire d’Astrophysique de Marseille, UMR 7326, CNRS, Université d’Aix Marseille, 38, rue Frédéric Joliot-Curie,Marseille, FranceWenbin LinPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaWenxiong LiPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaP. LognoneLAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, FranceR. MarronAPC, Univ. Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne, 75013 Paris Cité, FranceJ. MoPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaJ. MooreOzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, AustraliaR. NatsvlishviliE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaK. NoysenaObservatoire de la Côte d’AzurS. PerrigaultA. PeyrotD. SamadovN.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, AzerbaijanT. SadibekovaAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, FranceA. SimonAstronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, 60 Volodymyrska str., Kyiv UA-01601, UkraineC. StachieARTEMIS UMR 7250 UCA CNRS OCA, Boulevard de l’Observatoire, CS 34229, 06304 Nice CEDEX 04, FranceJ. P. TengP. ThierryC. C. ThöneInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, SpainYusufjon TillayevUlugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy str. 33, Tashkent 100052, UzbekistanD. TurpinNational Astronomical Observatories/Chinese Academy of Science 20A Datun Road, Beijing 100012, ChinaA. de Ugarte PostigoInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, SpainF. VachierM. VardosanidzeE.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, GeorgiaV. VasylenkoAstronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, 60 Volodymyrska str., Kyiv UA-01601, UkraineZ. VidadiN.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, AzerbaijanX. F. WangPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaC. J. WangYunnan Astronomical Observatories/Chinese Academy of Science, Kunming 650011, ChinaJ. Y. WeiNational Astronomical Observatories/Chinese Academy of Science 20A Datun Road, Beijing 100012, ChinaShengyu YanPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaJ. C. ZhangPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaJ. J. ZhangPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, ChinaXianfei ZhangPhysics Department and Astronomy Department, Tsinghua University, Beijing 100084, China
ABI
Аннотация
ABSTRACT We present the Global Rapid Advanced Network Devoted to the Multi-messenger Addicts (GRANDMA). The network consists of 21 telescopes with both photometric and spectroscopic facilities. They are connected together thanks to a dedicated infrastructure. The network aims at coordinating the observations of large sky position estimates of transient events to enhance their follow-up and reduce the delay between the initial detection and optical confirmation. The GRANDMA programme mainly focuses on follow-up of gravitational-wave alerts to find and characterize the electromagnetic counterpart during the third observational campaign of the Advanced LIGO and Advanced Virgo detectors. But it allows for follow-up of any transient alerts involving neutrinos or gamma-ray bursts, even those with poor spatial localization. We present the different facilities, tools, and methods we developed for this network and show its efficiency using observations of LIGO/Virgo S190425z, a binary neutron star merger candidate. We furthermore report on all GRANDMA follow-up observations performed during the first six months of the LIGO–Virgo observational campaign, and we derive constraints on the kilonova properties assuming that the events’ locations were imaged by our telescopes.
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