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GRANDMA observations of advanced LIGO's and advanced Virgo's third observational campaign
Antier, S.1; Agayeva, S.2; Almualla, M.3; Awiphan, S.4; Baransky, A.5,6; Barynova, K.5,6; Beradze, S.7,8; Blazek, M.9; Boer, M.10; Burkhonov, O.11; Christensen, N.10; Coleiro, A.1; Corre, D.12; Coughlin, M. W.13; Crisp, H.14; Dietrich, T.15; Ducoin, J-G12; Duverne, P-A12; Marchal-Duval, G.12; Gendre, B.14; Gokuldass, P.16; Eggenstein, H. B.17; Eymar, L.10; Hello, P.12; Howell, E. J.14; Ismailov, N.2; Kann, D. A.9; Karpov, S.18; Klotz, A.19,20; Kochiashvili, N.7; Lachaud, C.1; Leroy, N.12; Lin, W. L.21; Li, W. X.21; Masek, M.18; Mo, J.21; Menard, R.1; Morris, D.16; Noysena, K.19,20; Orange, N. B.22; Prouza, M.18; Rattanamala, R.23; Sadibekova, T.11,24; Saint-Gelais, D.1; Serrau, M.1; Simon, A.25; Stachie, C.10; Thone, C. C.9; Tillayev, Y.11,26; Turpin, D.24; de Ugarte Postigo, A.9; Vasylenko, V.25; Vidadi, Z.2; Was, M.27; Wang, X. F.21,22; Zhang JJ(张居甲)28; Zhang, T. M.29; Zhang, X. H.21
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2020-10-01
Volume497Issue:4Pages:5518-5539
DOI10.1093/mnras/staa1846
Contribution Rank第28完成单位
Indexed BySCI
Keywordgravitational waves methods: observational stars: neutron
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 deg(2) 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.

Funding ProjectAustralian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)[CE170100004] ; Australian Research Council DECRA Fellowship[DE170100891] ; Ramon y Cajal fellowships[RyC-2012-09975] ; Ramon y Cajal fellowships[RyC-2012-09984] ; Spanish Ministry of Economy and Competitiveness[AYA2017-89384-P] ; CNES Postdoctoral Fellowship at Laboratoire AstroParticule et Cosmologie ; Programme National Hautes Energies (PNHE) ; CNES postdoctoral program ; Ministry of Innovative Development[FA-Atech-2018-392] ; Ministry of Innovative Development[VA-FA-F-2-010] ; Shota Rustaveli National Science Foundation (SRNSF)[PHDF/18-1327] ; Institut National des Sciences de l'Univers, CNRS, France ; CNES ; European Structural and Investment Fund ; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/16 013/0001402] ; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/16 013/0001403] ; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/15 003/0000437] ; NASA-MUREP-MIRO grant[NNX15AP95A] ; NASA-EPSCoR grant[NNX13AD28A] ; NSF EiR AST Award[1901296] ; IdEx Universite de Paris[ANR-18-IDEX-0001] ; Spanish research project[RTI2018-098104-J-I00] ; [PTA2016-13192-I]
Funding OrganizationAustralian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)[CE170100004] ; Australian Research Council DECRA Fellowship[DE170100891] ; Ramon y Cajal fellowships[RyC-2012-09975, RyC-2012-09984] ; Spanish Ministry of Economy and Competitiveness[AYA2017-89384-P] ; CNES Postdoctoral Fellowship at Laboratoire AstroParticule et Cosmologie ; Programme National Hautes Energies (PNHE) ; CNES postdoctoral program ; Ministry of Innovative Development[FA-Atech-2018-392, VA-FA-F-2-010] ; Shota Rustaveli National Science Foundation (SRNSF)[PHDF/18-1327] ; Institut National des Sciences de l'Univers, CNRS, France ; CNES ; European Structural and Investment Fund ; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/16 013/0001402, CZ.02.1.01/0.0/0.0/16 013/0001403, CZ.02.1.01/0.0/0.0/15 003/0000437] ; NASA-MUREP-MIRO grant[NNX15AP95A] ; NASA-EPSCoR grant[NNX13AD28A] ; NSF EiR AST Award[1901296] ; IdEx Universite de Paris[ANR-18-IDEX-0001] ; Spanish research project[RTI2018-098104-J-I00] ; [PTA2016-13192-I]
Language英语
Subject Area天文学 ; 天体物理学 ; 实测天体物理学 ; 恒星与银河系 ; 恒星天文学
MOST Discipline Catalogue理学::天文学
SubtypeArticle
PublisherOXFORD UNIV PRESS
Publication PlaceGREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
WOS IDWOS:000587739300110
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordCOUNTERPARTS ; LIMITS ; MASS
Citation statistics
Cited Times:21[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/23921
Collection南方基地
中国科学院天体结构与演化重点实验室
Corresponding AuthorAntier, S.
Affiliation1.CNRS, Astroparticule et Cosmologie, Universit´e 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 Astrof´ısica de Andaluc´ıa (IAA-CSIC), Glorieta de la Astronom´ıa 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 f¨ur Physik und Astronomie, Universit¨at 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, Universit´e de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F- 31400 Toulouse, France
20.Universit´e Paul Sabatier Toulouse III, Universit´e 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, D´epartement d’Astrophysique, Astrophysique, Instrumentation et Mod´elisation de Paris-Saclay, Universit´e Paris-Saclay, F-91191 Gifsur- 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, Universit´e SavoieMont 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
Recommended Citation
GB/T 7714
Antier, S.,Agayeva, S.,Almualla, M.,et al. GRANDMA observations of advanced LIGO's and advanced Virgo's third observational campaign[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,497(4):5518-5539.
APA Antier, S..,Agayeva, S..,Almualla, M..,Awiphan, S..,Baransky, A..,...&Zhang, X. H..(2020).GRANDMA observations of advanced LIGO's and advanced Virgo's third observational campaign.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,497(4),5518-5539.
MLA Antier, S.,et al."GRANDMA observations of advanced LIGO's and advanced Virgo's third observational campaign".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 497.4(2020):5518-5539.
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