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

被引:72
作者
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-G [12 ]
Duverne, P-A [12 ]
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 ,22 ]
Li, W. X. [21 ,22 ]
Masek, M. [18 ]
Mo, J. [21 ,22 ]
Menard, R. [1 ]
Morris, D. [16 ]
Noysena, K. [19 ,20 ]
Orange, N. B. [23 ]
Prouza, M. [18 ]
Rattanamala, R. [24 ]
Sadibekova, T. [11 ,25 ]
Saint-Gelais, D. [1 ]
Serrau, M. [1 ]
Simon, A. [26 ]
Stachie, C. [10 ]
Thone, C. C. [9 ]
Tillayev, Y. [11 ,27 ]
Turpin, D. [25 ]
机构
[1] Univ Paris, Astroparticule & Cosmol, CNRS, F-75013 Paris, France
[2] Azerbaijan Natl Acad Sci, N Tusi Shamakhy Astrophys Observ, AZ-5626 Shamakhy, Azerbaijan
[3] Amer Univ Sharjah, Phys Dept, POB 26666, Sharjah, U Arab Emirates
[4] Natl Astron Res Inst Thailand, 260,Moo 4, Chiang Mai 50180, Thailand
[5] Taras Shevshenko Natl Univ Kyiv, Astron Observ, Observ Str 3, UA-04053 Kiev, Ukraine
[6] Taras Shevchenko Natl Univ Kyiv, Nucl Phys Dept, 60 Volodymyrska Str, UA-01601 Kiev, Ukraine
[7] E Kharadze Georgian Natl Astrophys Observ, GE-0301 Adigeni, Georgia
[8] Samtskhe Javakheti State Univ, Rustaveli Str 113, GE-0080 Akhaltsikhe, Georgia
[9] CSIC, Inst Astrofis Andalucia IAA, Glorieta Astron S-N, E-18008 Granada, Spain
[10] ARTEMIS UMR 7250 UCA CNRS OCA, Blvd Observ,CS 34229, F-06304 Nice 4, France
[11] Uzbek Acad Sci, Ulugh Beg Astron Inst, Astron Str 33, Tashkent 100052, Uzbekistan
[12] Univ Paris Saclay, CNRS, IN2P3, IJCLab, F-91898 Orsay, France
[13] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[14] Univ Western Australia, OzGrav UWA, Sch Phys, M013,35 Stirling Highway, Crawley, WA 6009, Australia
[15] Univ Potsdam, Inst Phys & Astron, Haus 28,Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany
[16] Univ Virgin Isl, Coll Sci & Math, 2 John Brewers Bay, St Thomas, VI 00802 USA
[17] Volkssternwarte Paderborn eV, Schlosspk 13, D-33104 Paderborn, Germany
[18] Czech Acad Sci, FZU Inst Phys, Prague, Czech Republic
[19] UPS, CNRS, Univ Toulouse, IRAP, 14 Ave Edouard Belin, F-31400 Toulouse, France
[20] Univ Paul Sabatier Kulouse III, Univ Toulouse, 118 Route Narbonne, F-31400 Toulouse, France
[21] Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China
[22] Tsinghua Univ, Astron Dept, Beijing 100084, Peoples R China
[23] OrangeWave Innovat Sci LLC, Moncks Corner, SC 29461 USA
[24] Chiang Mai Univ, Fac Sci, Dept Phys & Mat Sci, Chiang Mai 50200, Thailand
[25] Univ Paris Saclay, Dept Astrophys Astrophys Instrumentat & Modelisat, CEA, CNRS, F-91191 Gif Sur Yvette, France
[26] Taras Shevchenko Natl Univ Kyiv, Astron & Space Phys Dept, 60 Volodymyrska Str, UA-01601 Kiev, Ukraine
[27] Natl Univ Uzbekistan, 4 Univ Str, Tashkent 100174, Uzbekistan
[28] Univ Savoie Mt Blanc, Univ Grenoble Alpes, Lab Annecy Phys Particules LAPP, CNRS,IN2P3, F-74941 Annecy, France
[29] Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China
[30] Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
基金
澳大利亚研究理事会; 美国国家科学基金会;
关键词
gravitational waves; methods: observational; stars: neutron; COUNTERPARTS; LIMITS; MASS; 1ST;
D O I
10.1093/mnras/staa1846
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:5518 / 5539
页数:22
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