The first six months of the Advanced LIGO’s and Advanced Virgo’s third observing run with GRANDMA

Author:

Antier S1ORCID,Agayeva S2,Aivazyan V34,Alishov S2,Arbouch E5,Baransky A6,Barynova K7,Bai J M8,Basa S9,Beradze S34,Bertin E5,Berthier J10,Blažek M11,Boër M12ORCID,Burkhonov O13,Burrell A14,Cailleau A15,Chabert B1416,Chen J C17,Christensen N12,Coleiro A1,Cordier B18,Corre D19,Coughlin M W20ORCID,Coward D14,Crisp H14,Delattre C10,Dietrich T21,Ducoin J-G19,Duverne P-A19,Marchal-Duval G19,Gendre B14ORCID,Eymar L12,Fock-Hang P10,Han X22,Hello P19,Howell E J14ORCID,Inasaridze R34,Ismailov N2,Kann D A11,Kapanadze G34,Klotz A1516,Kochiashvili N3,Lachaud C1,Leroy N19,Le Van Su A9,Lin W L23,Li W X23,Lognone P19,Marron R1,Mo J23,Moore J14,Natsvlishvili R3,Noysena K1215,Perrigault S10,Peyrot A10,Samadov D2,Sadibekova T1318,Simon A24,Stachie C12,Teng J P10,Thierry P10,Thöne C C11,Tillayev Y13,Turpin D22ORCID,de Ugarte Postigo A11,Vachier F10,Vardosanidze M34,Vasylenko V24,Vidadi Z2,Wang X F23,Wang C J8,Wei J22,Yan S Y23,Zhang J C23,Zhang J J8,Zhang X H23

Affiliation:

1. APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/lrfu, Obs de Paris, Sorbonne, 75013 Paris Cité, France

2. N.Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Mamedaliyev, AZ 5626 Shamakhy, Azerbaijan

3. E.Kharadze Abastumani Astrophysical Observatory Mt.Kanobili, Ilia State University, Abastumani, 0301 Adigeni, Georgia

4. Samtskhe-Javakheti State University, Rustaveli Str. 113, Akhaltsikhe 0080, Georgia

5. UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, F-75014 Paris, France

6. Astronomical Observatory, Taras Shevshenko National University of Kyiv, Observatorna str. 3, Kyiv UA-04053, Ukraine

7. Nuclear Physics Department, Taras Shevchenko National University of Kyiv, 60 Volodymyrska str., Kyiv UA-01601, Ukraine

8. Yunnan Astronomical Observatories/Chinese Academy of Science, Kunming 650011, China

9. Laboratoire d’Astrophysique de Marseille, UMR 7326, CNRS, Université d’Aix Marseille, 38, rue Frédéric Joliot-Curie,Marseille, France

10. AGORA Observatoire des Makes, AGORA, 18 Rue Georges Bizet, Observatoire des Makes, F-97421 La Rivière, France

11. Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, E-18008 Granada, Spain

12. ARTEMIS UMR 7250 UCA CNRS OCA, Boulevard de l’Observatoire, CS 34229, 06304 Nice CEDEX 04, France

13. Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy str. 33, Tashkent 100052, Uzbekistan

14. OzGrav-UWA, University of Western Australia, School of Physics, M013, 35 Stirling Highway, Crawley, WA 6009, Australia

15. IRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F-31400 Toulouse, France

16. Université Paul Sabatier Toulouse III, Université de Toulouse, 118 Route de Narbonne, F-31400 Toulouse, France

17. WuZhou University, Wuzhou, Guangxi 543000, China

18. AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif-sur-Yvette, France

19. LAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, France

20. California Institute of Technology, 1200 East California Blvd, MC 249-17, Pasadena, CA 91125, USA

21. Nikhef, Science Park, NL-1098 XG Amsterdam, the Netherlands

22. National Astronomical Observatories/Chinese Academy of Science 20A Datun Road, Beijing 100012, China

23. Physics Department and Astronomy Department, Tsinghua University, Beijing 100084, China

24. Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, 60 Volodymyrska str., Kyiv UA-01601, Ukraine

Abstract

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.

Funder

Australian Research Council

Ministry of Economy and Competitiveness

California Institute of Technology

CNES

Université Sorbonne Paris Cité

Chinese Academy of Sciences

Ministry of Innovative Development

Shota Rustaveli National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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