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Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022
Melo, I. Tosta e1; Ducoin, J.-G.2; Vidadi, Z.3; Andrade, C.4; Rupchandani, V.5; Agayeva, S.3; Abdelhadi, J.6; Abe, L.7; Aguerre, O.8; Aivazyan, V.9,10; Alishov, S.3; Antier, S.11; Bai JM(白金明)12,48; Baransky, A.13; Bednarz, S.14; Bendjoya, Ph.7; Benkhaldoun, Z.6; Beradze, S.9,10; Bizouard, M. A.11; Bhardwaj, U.16; Blazek, M.17; Boër, M.11; Broens, E.18; Burkhonov, O.19; Christensen, N.11; Cooke, J.20; Corradi, W.21; Coughlin, M. W.4; Culino, T.11; Daigne, F.2,22; Dornic, D.23; Duverne, P.-A.24,35; Ehgamberdiev, S.19,25; Eymar, L.26; Fouad, A.27; Freeberg, M.28; Gendre, B.29,30; Guo, F.31; Gokuldass, P.32; Guessoum, N.33; Gurbanov, E.3; Hainich, R.34; Hasanov, E.3; Hello, P.35; Inasaridze, R.9,10; Iskandar, A.36,37; Ismailov, N.3; Janati, A.38; Laz, T. Jegou du39; Kann, D. A.(40,†); Karpov, S.41; Kiendrebeogo, R. W.4,11,42; Klotz, A.43,44; Kneip, R.45; Kochiashvili, N.9; Kaeouach, A.38; Kruiswijk, K.46; Lamoureux, M.46; Leroy, N.35; Lin, W. L.47; Mao JR(毛基荣)12,48; Marchais, D.49; Mašek, M.17; Midavaine, T.50; Moller, A.20; Morris, D.51; Natsvlishvili, R.9; Navarete, F.52; Guelbenzu, A. Nicuesa53; Noonan, K.51; Noysena, K.54; Oksanen, A.55; Orange, N. B.56; Pellouin, C.2; Peloton, J.35; Peng, H. W.47; Pilloix, M.57; Popowicz, A.58; Pradier, T.59; Pyshna, O.60; Raaijmakers, G.16; Rajabov, Y.19; Rau, A.61; Rinner, C.62; Rivet, J.-P.7; Ryh, A. S.27; Sabil, M.6; Sadibekova, T.19,63; Sasaki, N.21; Serrau, M.64; Simon, A.65,66; Shokry, A.27; Smith, K.51; Sokoliuk, O.13,67; Song, X.68; Takey, A.27; Thierry, P.43; Tillayev, Y.19,25; Turpin, D.63; Postigo, A. de Ugarte11; Vasylenko, V.65,66; Vernet, D.69; Wang, L.70; Vachier, F.43; Vignes, J. P.71; Wang, X. F.47,68; Zeng, X.70; Zhang, J.73; Zhu YJ(朱远俊)12,15,68,72
发表期刊ASTRONOMY & ASTROPHYSICS
2024-02-13
卷号682
DOI10.1051/0004-6361/202347938
产权排序第12完成单位
收录类别SCI ; EI
关键词methods: data analysis telescopes gamma-ray burst: general
摘要Aims. We present a campaign designed to train the Global Rapid Advanced Network Devoted to the Multi-messenger Addicts (GRANDMA) network and its infrastructure to follow up on transient alerts and detect their early afterglows. In preparation for O4 II campaign, we focused on gamma-ray burst (GRB) alerts since they are expected to serve as the electromagnetic counterpart of gravitational-wave events. Our goal was to improve our response to the alerts and to start prompt observations as soon as possible, so that we may better prepare the GRANDMA network for the fourth observational run of LIGO-Virgo-Kagra (launched at the end of May 2023) and future missions such as SM. Methods. We set up a dedicated infrastructure and organized a rota of follow-up advocates (FAs) to guarantee round-the-clock assistance to our telescope teams, with an aim to receive, manage, and send out observational plans to our partner telescopes. To ensure a large number of observations, we focused on Swift GRBs whose localization errors were generally smaller than the GRANDMA telescopes' field of view. This allowed us to bypass the transient identification process and focus on the reaction time and efficiency of the network. Results. During the 'Ready for O4 II' phase, 11 Swift/INTEGRAL GRB triggers were selected. Of these, nine fields had been observed and three afterglows had been detected (GRB 220403B, GRB 220427A, GRB 220514A) with 17 GRANDMA telescopes and 17 amateur astronomers from the citizen science project Kilonova-Catcher. Here, we highlight the GRB 220427A analysis, where our long-term follow-up of the host galaxy allowed us to obtain a photometric redshift of z = 0.82 +/- 0.09 and its lightcurve evolution, as well as to fit the decay slope of the afterglows and study the properties of the host galaxy. Conclusions. During this eight-week-long GRB follow-up campaign, we successfully fulfilled our goal of training telescope teams for O4 and improving the associated technical toolkits. For seven of the GRB alerts, our network was able to start the first observations less than one hour after the GRB trigger time. We also characterized the network efficiency to observe GRB afterglow given the resulting time delay and limiting magnitude, and to its light curve evolution based on the observation of GRB 220427A.
资助项目European Union funds - NextGenerationEU; Centre National d'Etudes Spatiales (CNES); le-de-France Region within the framework of the Domaine d'Interet Majeur-Astrophysique et Conditions d'Apparition de la Vie (DIM-ACAV); IdEx Universite de Paris Cite[ANR-18-IDEX-0001]; CNRS through the MITI interdisciplinary programs; CSI-Recherche Universite Cpte d'Azur; National Science Foundation[CZ.02.1.01/0.0/0.0/15_003/0000437]; National Science Foundation[11673062]; Science, Technology & Innovation Funding Authority (STDF)[45779]; Leibniz-Prize[HA 1850/28-1]; Scholar Program of Beijing Academy of Science and Technology; European Structural and Investment Fund; Tencent Xplorer Prize; Czech Ministry of Education, Youth and Sports; High-Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China; NOIRLab; National Natural Science Foundation of China (NSFC)[LM2023047]; National Natural Science Foundation of China (NSFC)[2023YFE0101200]; Ministry of Education of the Czech Republic; National Key R&D program of China for Intergovernmental Scientific and Technological Innovation Cooperation Project[12288102]; National Key R&D Program of China; Yunnan Revitalization Talent Support Program (YunLing Scholar Award); NSFC; Capes; CNPq; Fapemig; UFMG; UEA; National Science Foundation of China (NSFC)[11633002]; National Science Foundation of China (NSFC)[12090044]; National Science Foundation of China (NSFC)[DZ:BS202002]; National Science Foundation of China (NSFC)[11803076]; Ma Huateng Foundation;
项目资助者European Union funds - NextGenerationEU ; Centre National d'Etudes Spatiales (CNES) ; le-de-France Region within the framework of the Domaine d'Interet Majeur-Astrophysique et Conditions d'Apparition de la Vie (DIM-ACAV) ; IdEx Universite de Paris Cite[ANR-18-IDEX-0001] ; CNRS through the MITI interdisciplinary programs ; CSI-Recherche Universite Cpte d'Azur ; National Science Foundation[CZ.02.1.01/0.0/0.0/15_003/0000437, 11673062] ; Science, Technology & Innovation Funding Authority (STDF)[45779] ; Leibniz-Prize[HA 1850/28-1] ; Scholar Program of Beijing Academy of Science and Technology ; European Structural and Investment Fund ; Tencent Xplorer Prize ; Czech Ministry of Education, Youth and Sports ; High-Level Talent-Heaven Lake Program of Xinjiang Uygur Autonomous Region of China ; NOIRLab ; National Natural Science Foundation of China (NSFC)[LM2023047, 2023YFE0101200] ; Ministry of Education of the Czech Republic ; National Key R&D program of China for Intergovernmental Scientific and Technological Innovation Cooperation Project[12288102] ; National Key R&D Program of China ; Yunnan Revitalization Talent Support Program (YunLing Scholar Award) ; NSFC ; Capes ; CNPq ; Fapemig ; UFMG ; UEA ; National Science Foundation of China (NSFC)[11633002, 12090044, DZ:BS202002, 11803076] ; Ma Huateng Foundation ; [LM2023032] ; [12033003] ; [12203029] ; [2022YFE0126200] ; [PHY-2308862] ; [OAC-2117997]
语种英语
学科领域天文学
文章类型Article
出版者EDP SCIENCES S A
出版地17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE
ISSN0004-6361
URL查看原文
WOS记录号WOS:001161915800001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]GAMMA-RAY BURST ; MULTI-MESSENGER OBSERVATIONS ; X-RAY ; HOST GALAXIES ; HUBBLE CONSTANT ; LIGHT CURVES ; AFTERGLOW ; EMISSION ; CONSTRAINTS ; MASS
EI入藏号20240815613362
EI主题词Efficiency
EI分类号657.2 Extraterrestrial Physics and Stellar Phenomena - 913.1 Production Engineering - 931.3 Atomic and Molecular Physics - 931.5 Gravitation, Relativity and String Theory - 932.1 High Energy Physics
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文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26521
专题南方基地
信息中心
星系类星体研究组
作者单位1.Department of Physics and Astronomy, University of Catania, 95125 Catania, Italy;
2.Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, 75014 Paris, France;
3.N. Tusi Shamakhy Astrophysical Observatory Azerbaijan National Academy of Sciences, settl.Y. Mammadaliyev, 5626 Shamakhy, AZ, Azerbaijan;
4.School of Physics and Astronomy, University of Minnesota, Minneapolis, MI 55455, USA;
5.Brown University, Providence, RI 02912, USA;
6.Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University Av. Prince My Abdellah, 2390 Marrakesh, BP, Morocco;
7.Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire J.-L. Lagrange, Boulevard de l’Observatoire, 06304 Nice, France;
8.OCA, 14 rue Saint-Hubert, 60560 Orry-la-Ville, France;
9.E. Kharadze Georgian National Astrophysical Observatory, Mt.Kanobili, Abastumani, 0301 Adigeni, Georgia;
10.Samtskhe-Javakheti State University, Rustaveli Str. 113, Akhaltsikhe, 0080 Georgia;
11.Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Artemis, Boulevard de l’Observatoire, 06304 Nice, France;
12.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011 Yunnan Province, PR China;
13.Astronomical Observatory Taras Shevshenko National University of Kyiv, Observatorna str. 3, Kyiv, 04053 Ukraine;
14.Silesian University of Technology, Faculty of Automatic Control, Electronics and Computer Science, Akademicka 16, 44-100 Gliwice, Poland;
15.Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux, Nice, France;
16.GRAPPA, Anton Pannekoek Institute for Astronomy and Institute of High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands;
17.FZU – Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha, Czech Republic;
18.Vereniging or Sterrenkunde, Balen-Neetlaan 18A, 2400 Mol, Belgium;
19.Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy str. 33, Tashkent, 100052 Uzbekistan;
20.Centre for Astrophysics and Supercomputing, Swinburne University of Technology, ARC Centre of Excellence for Gravitational Wave Discovery 685 (OzGrav), Hawthorn, Victoria, 3122 Australia;
21.Laboratório Nacional de Astrofísica, R. dos Estados Unidos, 154 – Nações, Itajubá, MG, 37504-364 Brazil;
22.Institut Universitaire de France, Ministère de l’Enseignement Supérieur et de la Recherche, 75231 Paris, France;
23.CPPM, Aix-Marseille Univ., CNRS/IN2P3, CPPM, Marseille, France;
24.Université Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France;
25.National University of Uzbekistan, 4 University str., Tashkent, 100174 Uzbekistan;
26.Artemis, Boulevard de l’Observatoire, 06304 Nice, France;
27.National Research Institute of Astronomy and Geophysics (NRIAG), 1 El-marsad St., 11421 Helwan, Cairo, Egypt;
28.KNC, AAVSO, Hidden Valley Observatory(H), Colfax, WI.; iTelescope, NMS, Mayhill NM, USA;
29.Department of Physics, University of Western Australia, Crawley, WA, 6009 Australia;
30.Australia ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), Australia;
31.Physics Department and Astronomy Department, Tsinghua University, Beijing, 100084 PR China;
32.Department of Aerospace, Physics, and Space Sciences, Florida Institute of Technology, Melbourne, FL, 32901 USA;
33.American University of Sharjah, Physics Department, PO Box 26666 Sharjah, UAE;
34.Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, 14476 Potsdam, Germany;
35.IJCLab, Université Paris-Saclay, CNRS/IN2P3, Orsay, France;
36.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang, 830011 PR China;
37.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, 100049 PR China;
38.Oukaimeden Observatory HAO Telescope, Oukaimeden, Morocco;
39.Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA, 91125 USA;
40.Hessian Research Cluster ELEMENTS, Giersch Science Center, Max-n-Laue-Straße 12, Goethe University Frankfurt, Campus Riedberg, 60438 Frankfurt am Main, Germany;
41.CEICO, Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, 182 21 Praha, Czech Republic;
42.Laboratoire de Physique et de Chimie de l’Environnement, Université Joseph Ki-Zerbo, Ouagadougou, Burkina Faso;
43.IRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Édouard Belin, 31400 Toulouse, France;
44.Université Paul-Sabatier Toulouse III, Université de Toulouse, 118 route de Narbonne, 31400 Toulouse, France;
45.K26 / Contern Observatory (private obs.), 1, beim Schmilberbour, 5316 Contern, Luxembourg;
46.Centre for Cosmology, Particle Physics and Phenomenology – CP3, Universite Catholique de Louvain, 1348 Louvain-la-Neuve, Belgium;
47.Physics Department and Astronomy Department, Tsinghua University Beijing, 100084, PR China; Beijing Planetarium, Beijing Academy of Science and Technology, Beijing, 100044 PR China;
48.Key Laboratory for the Structure and Elution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, PR China;
49.Observatoire du Crous des Gats, 31550 Cintegabelle, France;
50.Société Astronomique de France, 3 rue Beethoven, 75016 Paris, France;
51.University of the Virgin Islands, United States Virgin Islands, Islands, 00802 USA;
52.SOAR Telescope/NSF’s NOIRLab, Avda Juan Cisternas 1500, La Serena, Chile;
53.Thüringer Landessternwarte Tautenburg, 07778 Tautenburg, Germany;
54.National Astronomical Research Institute of Thailand (Public Organization), 260, Moo 4, T. Donkaew, A. Mae Rim, Chiang Mai, 50180 Thailand;
55.Hankasalmi Observatory, Jyvaskylan Sirius ry, Verkkoniementie 30, 40950 Muurame, Finland;
56.OrangeWave Innovative Science, LLC, Moncks Corner, SC, 29461 USA;
57.Artemis, Observatoire de la Côte d’Azur, Université Côte d’Azur, Boulevard de l’Observatoire, 06304 Nice, France;
58.Silesian University of Technology, Department of Electronics, Electrical Engineering and Microelectronics, Akademicka 16, 44-100 Gliwice, Poland;
59.Université de Strasbourg, CNRS, IPHC UMR 7178, 67000 Strasbourg, France;
60.Astronomical Observatory of Taras Shevchenko National University of Kyiv, Observatorna Str. 3, Kyiv, 04053 Ukraine;
61.Max-Planck-Institut für extraterrestrische Physik, Gießenbachstraße 1, 85748 Garching, Germany;
62.Oukaimeden Observatory (MOSS), Oukaimeden, Morocco;
63.Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191 Gif-sur-Yvette, France;
64.Société Astronomique de France, Observatoire de Dauban, 04150 Banon, France;
65.Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, Glushkova ave. 4, Kyiv, 03022 Ukraine;
66.National Center Junior academy of sciences of Ukraine, 38-44, Dehtiarivska St., Kyiv, 04119 Ukraine;
67.Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Acad. Zabolotnoho Str., Kyiv, 03143 Ukraine;
68.Beijing Planetarium, Beijing Academy of Science and Technology, Beijing, 100044 PR China;
69.Observatoire de la Côte d’Azur, Université Côte d’Azur, CNRS, UMS, Galilée, France;
70.Xinjiang Astronomical Observatory, 150 Science 1-Street, Urumqi, Xinjiang, 830011 PR China;
71.KNC Deep Sky Chile Observatory, Chile;
72.Physics department and Tsinghua Center for Astrophysics, Tsinghua University, Beijing, 100084 PR China;
73.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, A20, Datun Road, Chaoyang District, Beijing, 100012 PR China
推荐引用方式
GB/T 7714		 Melo, I. Tosta e,Ducoin, J.-G.,Vidadi, Z.,et al. Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022[J]. ASTRONOMY & ASTROPHYSICS,2024,682.
APA Melo, I. Tosta e.,Ducoin, J.-G..,Vidadi, Z..,Andrade, C..,Rupchandani, V..,...&朱远俊.(2024).Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022.ASTRONOMY & ASTROPHYSICS,682.
MLA Melo, I. Tosta e,et al."Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022".ASTRONOMY & ASTROPHYSICS 682(2024).
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