GRANDMA observations of advanced LIGO’s and advanced Virgo’s third observational campaign

Author:

Antier S1ORCID,Agayeva S2,Almualla M3,Awiphan S4,Baransky A56,Barynova K56,Beradze S78,Blažek M9ORCID,Boër M10ORCID,Burkhonov O11,Christensen N10,Coleiro A1,Corre D12,Coughlin M W13ORCID,Crisp H14,Dietrich T15,Ducoin J-G12,Duverne P-A12,Marchal-Duval G12,Gendre B14ORCID,Gokuldass P16,Eggenstein H B17,Eymar L10,Hello P12,Howell E J14ORCID,Ismailov N2,Kann D A9,Karpov S18,Klotz A1920,Kochiashvili N7,Lachaud C1,Leroy N12,Lin W L21,Li W X21,Mašek M18,Mo J21,Menard R1,Morris D16,Noysena K1920,Orange N B22,Prouza M18,Rattanamala R23,Sadibekova T1124,Saint-Gelais D1,Serrau M1,Simon A25,Stachie C10,Thöne C C9,Tillayev Y1126,Turpin D24ORCID,Postigo A de Ugarte9,Vasylenko V25,Vidadi Z2,Was M27,Wang X F21,Zhang J J28,Zhang T M29,Zhang X H21

Affiliation:

1. CNRS, Astroparticule et Cosmologie , Université de Paris, F-75013 Paris, France

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

3. Physics Department , American University of Sharjah, P.O. Box 26666, Sharjah, UAE

4. National Astronomical Research Institute of Thailand, 260, Moo 4, T. Donkaew, A. Mae Rim, Chiang Mai 50180, Thailand

5. Astronomical Observatory Taras Shevshenko National University of Kyiv, Observatorna str. 3, Kyiv 04053, Ukraine

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

7. E. Kharadze Georgian National Astrophysical Observatory, Mt.Kanobili, Abastumani, 0301 Adigeni, Georgia

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

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

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

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

12. IJCLab, Univ Paris-Saclay, CNRS/IN2P3, F-91898 Orsay, France

13. School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA

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

15. Institut für Physik und Astronomie, Universität Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, D-14476 Potsdam, Germany

16. University of the Virgin Islands , College of Science and Math, 2 John Brewer’s Bay, St. Thomas, VI 00802, USA

17. Volkssternwarte Paderborn e.V. Im Schlosspark 13, D-33104 Paderborn – Schloss Neuhaus, Germany

18. FZU – Institute of Physics of the Czech Academy of Sciences, Prague, Czech Republic

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

20. Université Paul Sabatier Toulouse III, Université de Toulouse, 118 route de Narbonne, F-31400 Toulouse, France

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

22. OrangeWave Innovative Science, LLC, Moncks Corner, SC 29461, USA

23. Department of Physics and Materials Science, Faculty of Science, Chiang Mai University, Chiang Mai 50200, Thailand

24. CNRS, CEA, Département d’Astrophysique, Astrophysique, Instrumentation et Modélisation de Paris-Saclay, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France

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

26. National University of Uzbekistan, 4 University str., Tashkent 100174, Uzbekistan

27. Laboratoire d’Annecy de Physique des Particules (LAPP), Univ. Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France

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

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

Abstract

ABSTRACT GRANDMA (Global Rapid Advanced Network Devoted to the Multi-messenger Addicts) is a network of 25 telescopes of different sizes, including both photometric and spectroscopic facilities. The network aims to coordinate follow-up observations of gravitational-wave (GW) candidate alerts, especially those with large localization uncertainties, to reduce the delay between the initial detection and the optical confirmation. In this paper, we detail GRANDMA’s observational performance during Advanced LIGO/Advanced Virgo Observing Run 3 (O3), focusing on the second part of O3; this includes summary statistics pertaining to coverage and possible astrophysical origin of the candidates. To do so, we quantify our observation efficiency in terms of delay between GW candidate trigger time, observations, and the total coverage. Using an optimized and robust coordination system, GRANDMA followed-up about 90 per cent of the GW candidate alerts, that is 49 out of 56 candidates. This led to coverage of over 9000 deg2 during O3. The delay between the GW candidate trigger and the first observation was below 1.5 h for 50 per cent of the alerts. We did not detect any electromagnetic counterparts to the GW candidates during O3, likely due to the very large localization areas (on average thousands of degrees squares) and relatively large distance of the candidates (above 200 Mpc for 60 per cent of binary neutron star, BNS candidates). We derive constraints on potential kilonova properties for two potential BNS coalescences (GW190425 and S200213t), assuming that the events’ locations were imaged.

Funder

Australian Research Council

CNES

SRNSF

NASA

MIRO

EPSCoR

NSF

AST

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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