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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-Chariol, O.8; Aivazyan, V.9,10; Alishov, S.3; Antier, S.11; Bai, J. -M.12,51; Baransky, A.13; Bednarz, S.14; Bendjoya, Ph.7; Benkhaldoun, Z.6; Beradze, S.9,10; Bizouard, M. A.11; Bhardwaj, U.16,17; Blazek, M.18; Bor, M.11; Broens, E.19; Burkhonov, O.20; Christensen, N.11; Cooke, J.21; Corradi, W.22; Coughlin, M. W.4; Culino, T.11; Daigne, F.2,23; Dornic, D.24; Duverne, P. -A.25,38; Ehgamberdiev, S.20,26; Eymar, L.27; Fouad, A.28; Freeberg, M.29,30; Gendre, B.31,32; Guo, F.33,34 ; Gokuldass, P.35; Guessoum, N.36; Gurbanov, E.3; Hainich, R.37; Hasanov, E.3; Hello, P.38; Inasaridze, R.9,10; Iskandar, A.39,40; Ismailov, N.3; Janati, A.41; Jegou du Laz, T.42; Kann, D. A.43; Karpov, S.44; Kiendrebeogo, R. W.4,11,45; Klotz, A.46,47; Kneip, R.48; Kochiashvili, N.9; Kaeouach, A.41; Kruiswijk, K.49; Lamoureux, M.49; Leroy, N.38; Lin, W. L.33,34,50; Mao, J.12,51; Marchais, D.52; Masek, M.18; Midavaine, T.53; Moller, A.21; Morris, D.54; Natsvlishvili, R.9; Navarete, F.55; Nicuesa Guelbenzu, A.56; Noonan, K.54; Noysena, K.57; Oksanen, A.58; Orange, N. B.59; Pellouin, C.2; Peloton, J.38; Peng, H. W.33,34,50; Pilloix, M.60; Popowicz, A.61; Pradier, T.62; Pyshna, O.63; Raaijmakers, G.16,17; Rajabov, Y.20; Rau, A.64; Rinner, C.65; Rivet, J. -p.7; Ryh, A. S.28; Sabil, M.6; Sadibekova, T.20,66; Sasaki, N.22; Serrau, M.67; Simon, A.68,69; Shokry, A.28; Smith, K.54; Sokoliuk, O.13,70; Song, X.71; Takey, A.28; Thierry, P.46; Tillayev, Y.20,26; Turpin, D.66; de Ugarte Postigo, A.11; Vasylenko, V.68,69; Vernet, D.72; Wang, L.73; Vachier, F.46; Vignes, J. P.74; Wang, X. F.33,34,50,71; Zeng, X.73; Zhang, J.76; Zhu, Y.12,15,33,71,75
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| 2024-02-13 | |
| Source Publication | ASTRONOMY & ASTROPHYSICS
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| ISSN | 0004-6361 |
| Volume | 682Pages:A141 |
| Contribution Rank | 36 |
| Abstract | 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. |
| Keyword | methods: data analysis telescopes gamma-ray burst: general |
| DOI | 10.1051/0004-6361/202347938 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | GAMMA-RAY BURST ; MULTI-MESSENGER OBSERVATIONS ; X-RAY ; HOST GALAXIES ; HUBBLE CONSTANT ; LIGHT CURVES ; AFTERGLOW ; EMISSION ; CONSTRAINTS ; MASS |
| Funding Project | 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 ; [LM2023032] ; [12033003] ; [12203029] ; [2022YFE0126200] ; [PHY-2308862] ; [OAC-2117997] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001161915800001 |
| Publisher | EDP SCIENCES S A |
| Funding Organization | 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 ; CNRS through the MITI interdisciplinary programs ; CSI-Recherche Universite Cpte d'Azur ; National Science Foundation ; Science, Technology & Innovation Funding Authority (STDF) ; Leibniz-Prize ; 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) ; Ministry of Education of the Czech Republic ; National Key R&D program of China for Intergovernmental Scientific and Technological Innovation Cooperation Project ; 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) ; Ma Huateng Foundation |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5844 |
| Collection | 光学天文与技术应用研究室_变星研究团组 科研仪器设备产出_利用南山1米大视场望远镜（NOWT）观测数据的文章 |
| Corresponding Author | Melo, I. Tosta e; Ducoin, J. -G. |
| Affiliation | 1.Univ Catania, Dept Phys & Astron, I-95125 Catania, Italy 2.Sorbonne Univ, Inst Astrophys Paris, CNRS, UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France 3.Azerbaijan Natl Acad Sci, N Tusi Shamakhy Astrophys Observ, AZ-5626 Shamakhy, Azerbaijan 4.Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA 5.Brown Univ, Providence, RI 02912 USA 6.Cadi Ayyad Univ, Oukaimeden Observ, High Energy Phys & Astrophys Lab, FSSM, Av Prince My Abdallah, Marrakech 2390, Morocco 7.Univ Cote dAzur, CNRS, Observ Cote dAzur, Lab JL Lagrange, Blvd Observ, F-06304 Nice, France 8.OCA, 14 Rue St Hubert, F-60560 Orry La Ville, France 9.E Kharadze Georgian Natl Astrophys Observ, Abastumani 0301, Adigeni, Georgia 10.Samtskhe Javakheti State Univ, Rustaveli Str 113, Akhaltsikhe 0080, Georgia 11.Univ Cote Azur, Observ Cote Azur, CNRS, Artemis, Blvd Observ, F-06304 Nice, France 12.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China 13.Taras Shevshenko Natl Univ Kyiv, Astron Observ, Observatorna Str 3, UA-04053 Kiev, Ukraine 14.Silesian Tech Univ, Fac Automat Control Elect & Comp Sci, Akad 16, PL-44100 Gliwice, Poland 15.Astrophys Relativiste Theories Experiences Metrol, Nice, France 16.Univ Amsterdam, Anton Pannekoek Inst Astron, GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands 17.Univ Amsterdam, Inst High Energy Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands 18.Czech Acad Sci, FZU Inst Phys, Na Slovance 1999-2, Prague 18221, Czech Republic 19.Vereniging Sterrenkunde, Balen Neetlaan 18A, B-2400 Mol, Belgium 20.Uzbek Acad Sci, Ulugh Beg Astron Inst, Astron Str 33, Tashkent 100052, Uzbekistan 21.Swinburne Univ Technol, Ctr Astrophys & Supercomp, ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic 3122, Australia 22.Lab Nacl Astrofis, R Estados Unidos 154, BR-37504364 Itajuba, MG, Brazil 23.Minist Enseignement Super & Rech, Inst Univ France, F-75231 Paris, France 24.Aix Marseille Univ, CPPM, CNRS IN2P3, Marseille, France 25.Univ Paris Cite, CNRS, Astroparticule & Cosmol, F-75013 Paris, France 26.Natl Univ Uzbekistan, 4 Univ Str, Tashkent 100174, Uzbekistan 27.Artemis, Blvd Observ, F-06304 Nice, France 28.Natl Res Inst Astron & Geophys NRIAG, 1 El Marsad St, Cairo 11421, Egypt 29.Hidden Valley Observ H, KNC, AAVSO, Colfax, WI USA 30.iTelescope, NMS, Mayhill, NM USA 31.Univ Western Australia, Dept Phys, Crawley, WA 6009, Australia 32.Australia ARC Ctr Excellence Gravitat Wave Discove, Crawley, Australia 33.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China 34.Tsinghua Univ, Astron Dept, Beijing 100084, Peoples R China 35.Florida Inst Technol, Dept Aerosp Phys & Space Sci, Melbourne, FL 32901 USA 36.Amer Univ Sharjah, Phys Dept, POB 26666, Sharjah, U Arab Emirates 37.Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany 38.Univ Paris Saclay, IJCLab, CNRS IN2P3, Orsay, France 39.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 40.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 41.Oukaimeden Observ HAO Telescope, Oukaimeden, Morocco 42.CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA 43.Goethe Univ Frankfurt, Giersch Sci Ctr, Hessian Res Cluster ELEMENTS, Max N Laue Str 12,Campus Riedberg, D-60438 Frankfurt, Germany 44.Czech Acad Sci, Inst Phys, CEICO, Na Slovance 1999-2, Prague 18221, Czech Republic 45.Univ Joseph Ki Zerbo, Lab Phys & Chim Environm, Ouagadougou, Burkina Faso 46.Univ Toulouse, CNRS, UPS, IRAP, 14 Ave Edouard Belin, F-31400 Toulouse, France 47.Univ Paul Sabatier Toulouse III, Univ Toulouse, 118 Route Narbonne, F-31400 Toulouse, France 48.K26 Contern Observ Private Obs, 1 Beim Schmilberbour, L-5316 Contern, Luxembourg 49.Catholic Univ Louvain, Ctr Cosmol Particle Phys & Phenomenol CP3, B-1348 Louvain La Neuve, Belgium 50.Beijing Acad Sci & Technol, Beijing Planetarium, Beijing 100044, Peoples R China 51.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China 52.Observ Crous Gats, F-31550 Cintegabelle, France 53.Soc Astron France, 3 Rue Beethoven, F-75016 Paris, France 54.Univ Virgin Isl, St Thomas, VI 00802 USA 55.SOAR Telescope NSFs NOIRLab, Avda Juan Cisternas 1500, La Serena, Chile 56.Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany 57.Natl Astron Res Inst Thailand Publ Org, 260,Moo 4, Chiang Mai 50180, Thailand 58.Hankasalmi Observ, Jyvaskylan Sirius Ry, Verkkoniementie 30, Muurame 40950, Finland 59.OrangeWave Innovat Sci LLC, Moncks Corner, SC 29461 USA 60.Univ Cote dAzur, Observ Cote dAzur, CNRS, Blvd Observ, F-06304 Nice, France 61.Silesian Tech Univ, Dept Elect Elect Engn & Microelect, Akad 16, PL-44100 Gliwice, Poland 62.Univ Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France 63.Taras Shevchenko Natl Univ Kyiv, Astron Observ, Observ Str 3, UA-04053 Kiev, Ukraine 64.Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany 65.Oukaimeden Observ MOSS, Oukaimeden, Morocco 66.Univ Paris Saclay, Univ Paris Cite, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France 67.Soc Astron France, Observ Dauban, F-04150 Banon, France 68.Taras Shevchenko Natl Univ Kyiv, Astron & Space Phys Dept, Glushkova Ave 4, UA-03022 Kiev, Ukraine 69.Natl Ctr Jr Acad Sci Ukraine, 38-44 Dehtiarivska Str, UA-04119 Kiev, Ukraine 70.Natl Acad Sci Ukraine, Main Astron Observ, 27 Acad Zabolotnoho Str, UA-03143 Kiev, Ukraine 71.Beijing Acad Sci & Technol, Beijing Planetarium, Beijing 100044, Peoples R China 72.Univ Cote dAzur, Observ Cote dAzur, CNRS, UMS, Galilee, France 73.Chinese Acad Sci, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China 74.KNC Deep Sky Chile Observ, Santigo, Chile 75.Tsinghua Univ, Tsinghua Ctr Astrophys, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China 76.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China |
| Recommended Citation 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:A141. |
| APA | Melo, I. Tosta e.,Ducoin, J. -G..,Vidadi, Z..,Andrade, C..,Rupchandani, V..,...&Zhu, Y..(2024).Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022.ASTRONOMY & ASTROPHYSICS,682,A141. |
| 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):A141. |
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