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| GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst-In Gedenken an David Alexander Kann | |
Kann, D. A.1; Agayeva, S.2; Aivazyan, V.3,4; Alishov, S.2; Andrade, C. M.5; Antier, S.6; Baransky, A.7; Bendjoya, P.8; Benkhaldoun, Z.9; Beradze, S.3,4; Berezin, D.10,11; Boer, M.6; Broens, E.12; Brunier, S.8; Bulla, M.13,14,15; Burkhonov, O.16; Burns, E.17; Chen, Y.18 ; Chen, Y. P.18; Conti, M.19; Coughlin, M. W.5; Cui, W. W.18; Daigne, F.20; Delaveau, B.21; Devillepoix, H. A. R.22; Dietrich, T.23,24; Dornic, D.25; Dubois, F.26,27; Ducoin, J. G.20; Durand, E.21; Duverne, P. A.28; Eggenstein, H. B.29; Ehgamberdiev, S.16,30; Fouad, A.31; Freeberg, M.32; Froebrich, D.33; Ge, M. Y.18; Gervasoni, S.6; Godunova, V.10,11; Gokuldass, P.34; Gurbanov, E.2; Han, D. W.18; Hasanov, E.2; Hello, P.35; Hussenot-Desenonges, T.35; Inasaridze, R.3,4; Iskandar, A.36; Ismailov, N.2; Janati, A.9; du Laz, T. J.35; Jia, S. M.18; Karpov, S.37; Kaeouach, A.38; Kiendrebeogo, R. W.5,6,39; Klotz, A.40,41; Kneip, R.42; Kochiashvili, N.3; Kunert, N.23; Lekic, A.21; Leonini, S.19; Li, C. K.18; Li, W.18; Li, X. B.18; Liao, J. Y.18; Logie, L.26,27; Lu, F. J.18; Mao, J.43,44,45; Marchais, D.46; Menard, R.47; Morris, D.48; Natsvlishvili, R.3; Nedora, V.24; Noonan, K.48; Noysena, K.49; Orange, N. B.50; Pang, P. T. H.51,52; Peng, H. W.53; Pellouin, C.20; Peloton, J.35; Pradier, T.54; Pyshna, O.7; Rajabov, Y.16; Rau, S.26,27; Rinner, C.9; Rivet, J. P.8; Romanov, F. D.55; Rosi, P.19; Rupchandani, V. A.56,57; Serrau, M.58; Shokry, A.31; Simon, A.59,60; Smith, K.48; Sokoliuk, O.7,10; Soliman, M.61; Song, L. M.18; Takey, A.31; Tillayev, Y.16,30; Ramirez, L. M. T.19; Melo, I. T.62; Turpin, D.63; Postigo, A. D.6; Vanaverbeke, S.26,27; Vasylenko, V.59,60; Vernet, D.64; Vidadi, Z.2; Wang, C.65; Wang, J.18; Wang, L. T.36; Wang, X. F.53,66; Xiong, S. L.18; Xu, Y. P.18; Xue, W. C.18; Zeng, X.67; Zhang, S. N.18; Zhao, H. S.18; Zhao, X. F.18
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| 2023-05-01 | |
| Source Publication | Astrophysical Journal Letters
 |
| ISSN | 2041-8205 |
| Volume | 948Issue:2Pages:L12 |
| Contribution Rank | 36 |
| Abstract | Object GRB 221009A is the brightest gamma-ray burst (GRB) detected in more than 50 yr of study. In this paper, we present observations in the X-ray and optical domains obtained by the GRANDMA Collaboration and the Insight Collaboration. We study the optical afterglow with empirical fitting using the GRANDMA+HXMT-LE data sets augmented with data from the literature up to 60 days. We then model numerically using a Bayesian approach, and we find that the GRB afterglow, extinguished by a large dust column, is most likely behind a combination of a large Milky Way dust column and moderate low-metallicity dust in the host galaxy. Using the GRANDMA+HXMT-LE+XRT data set, we find that the simplest model, where the observed afterglow is produced by synchrotron radiation at the forward external shock during the deceleration of a top-hat relativistic jet by a uniform medium, fits the multiwavelength observations only moderately well, with a tension between the observed temporal and spectral evolution. This tension is confirmed when using the augmented data set. We find that the consideration of a jet structure (Gaussian or power law), the inclusion of synchrotron self-Compton emission, or the presence of an underlying supernova do not improve the predictions. Placed in the global context of GRB optical afterglows, we find that the afterglow of GRB 221009A is luminous but not extraordinarily so, highlighting that some aspects of this GRB do not deviate from the global known sample despite its extreme energetics and the peculiar afterglow evolution. |
| Keyword | optical light-curve supernova 2003dh extinction map star merger pre-swift long emission grb-030329 telescope evolution Astronomy & Astrophysics |
| Subtype | Article |
| DOI | 10.3847/2041-8213/acc8d0 |
| Indexed By | SCI |
| Language | 英语 |
| WOS ID | WOS:000992639300001 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6643 |
| Collection | 光学天文与技术应用研究室 |
| Affiliation | 1.Hessian Research Cluster ELEMENTS, Giersch Science Center, Max-von-Laue-Straße 12, Goethe University Frankfurt, Campus Riedberg, D-60438 Frankfurt am Main, Germany; grandma-l@in2p3.fr; 2.N. Tusi Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, settl.Y. Mammadaliyev, AZ 5626, Shamakhy, Azerbaijan; 3.E. Kharadze Georgian National Astrophysical Observatory, Mt. Kanobili, Abastumani, 0301, Adigeni, Georgia; 4.Samtskhe-Javakheti State University, Rustaveli Str. 113, Akhaltsikhe, 0080, Georgia; 5.School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA; 6.Artemis, Observatoire de la Côte d’Azur, Université Côte d’Azur, Boulevard de l’Observatoire, F-06304 Nice, France; 7.Astronomical Observatory of Taras Shevchenko National University of Kyiv, Observatorna Str. 3, Kyiv, 04053, Ukraine; 8.Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS UMR 7293 Laboratoire Lagrange, F 06108 Nice,France; 9.Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, FSSM, Cadi Ayyad University, Av. Prince My Abdellah, BP 2390 Marrakesh, Morocco; 10.Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Acad. Zabolotnoho Str., Kyiv, 03143, Ukraine; 11.ICAMER Observatory, National Academy of Sciences of Ukraine, 27 Acad. Zabolotnoho Str., 03143 Kyiv, Ukraine; 12.Vereniging Voor Sterrenkunde, Balen-Neetlaan 18A, B-2400, Mol, Belgium; 13.Department of Physics and Earth Science, University of Ferrara, via Saragat 1, I-44122 Ferrara, Italy; 14.INFN, Sezione di Ferrara, via Saragat 1, I-44122 Ferrara, Italy; 15.INAF, Osservatorio Astronomico d’Abruzzo, via Mentore Maggini snc, I-64100 Teramo, Italy; 16.Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy Str. 33, Tashkent 100052, Uzbekistan; 17.Department of Physics & Astronomy, Louisiana State University, Baton Rouge, LA 70803, USA; 18.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People’s Republic of China xiongsl@ihep.ac.cn; 19.Montarrenti Observatory, S.S. 73 Ponente, I-53018 Sovicille, Siena, Italy; 20.Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France; 21.Institut Polytechnique des Sciences Avancées IPSA, 63 bis Boulevard de Brandebourg, F-94200 Ivry-sur-Seine, France; 22.Space Science & Technology Centre, School of Earth and Planetary Sciences, Curtin University, GPO Box U1987, Perth, WA 6845, Australia; 23.Institute for Physics and Astronomy, University of Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, D-14476 Potsdam, Germany; 24.Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, D-14476 Potsdam, Germany; 25.CPPM, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France; 26.AstroLAB IRIS, Provinciaal Domein “De Palingbeek”, Verbrandemolenstraat 5, B-8902 Zillebeke, Ieper, Belgium; 27.Vereniging Voor Sterrenkunde (VVS), Oostmeers 122 C, B-8000 Brugge, Belgium; 28.Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France; 29.Volkssternwarte Paderborn, Im Schlosspark 13, D-33104 Paderborn, Germany; 30.National University of Uzbekistan, 4 University Str., Tashkent 100174, Uzbekistan; 31.National Research Institute of Astronomy and Geophysics (NRIAG), 1 El-marsad St., 11421 Helwan, Cairo, Egypt; 32.KNC, AAVSO, Hidden Valley Observatory (HVO), Colfax, WI, USA; iTelescope, New Mexico Skies Observatory, Mayhill, NM, USA; 33.School of Physics and Astronomy, University of Kent, Canterbury CT2 7NH, UK; 34.Department of Aerospace, Physics, and Space Sciences, Florida Institute of Technology, Melbourne, FL 32901, USA; 35.IJCLab, Univ Paris-Saclay, CNRS/IN2P3, Orsay, France; 36.Xinjiang Astronomical Observatory (XAO), Chinese Academy of Sciences, Urumqi, 830011, People’s Republic of China; 37.CEICO, Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, CZ-182 21, Praha, Czech Republic; 38.Oukaimeden Observatory, Cadi Ayyad University, High Atlas Observatory, Morocco; 39.Laboratoire de Physique et de Chimie de l’Environnement, Université Joseph KI-ZERBO, Ouagadougou, Burkina Faso; 40.IRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F-31400 Toulouse, France; 41.Université Paul Sabatier Toulouse III, Université de Toulouse, 118 Route de Narbonne, F-31400 Toulouse, France; 42.K26 / Contern Observatory (private obs.), 1, beim Schmilberbour, 5316 Contern, Luxembourg; 43.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, People’s Republic of China; 44.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, 100012 Beijing, People’s Republic of China; 45.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, People’s Republic of China; 46.Observatoire du Crous des Gats, F-31550 Cintegabelle, France; 47.Club d’astronomie Mont-Tremblant, 545 Chemin Saint-Bernard, Mont-Tremblant, QC, J8E 1S8, Canada; 48.University of the Virgin Islands, United States Virgin Islands 00802, USA; 49.National Astronomical Research Institute of Thailand (Public Organization), 260, Moo 4, T. Donkaew, A. Mae Rim, Chiang Mai, 50180, Thailand; 50.OrangeWave Innovative Science, LLC, Moncks Corner, SC 29461, USA; 51.Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands; 52.Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, The Netherlands; 53.Physics Department, Tsinghua University, Beijing, 100084, People’s Republic of China; 54.Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France; 55.AAVSO Observer; Pobedy Street, House 7, Flat 60, Yuzhno-Morskoy, Nakhodka, Primorsky Krai 692954, Russia; 56.Brown University, Providence, RI 02912, USA; 57.American University of Sharjah, Sharjah, UAE; 58.Société Astronomique de France, Observatoire de Dauban, F-04150 Banon, France; 59.Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, Glushkova Ave., 4, Kyiv, 03022, Ukraine; 60.National Center Junior Academy of Sciences of Ukraine, Dehtiarivska St. 38-44, Kyiv, 04119, Ukraine; 61.Department of Astronomy and Meteorology, Faculty of Science, Al-Azhar University, 11884 Nasr City, Cairo, Egypt; 62.INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy; 63.Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191, Gif-sur-Yvette, France; 64.Observatoire de la Côte d’Azur, CNRS, UMS Galilée, France; 65.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China; 66.Beijing Planetarium, Beijing Academy of Science and Technology, Beijing, 100044, People’s Republic of China; 67.Center for Astronomy and Space Sciences, China Three Gorges University, Yichang 443000, People’s Republic of China |
| Recommended Citation GB/T 7714 | Kann, D. A.,Agayeva, S.,Aivazyan, V.,et al. GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst-In Gedenken an David Alexander Kann[J]. Astrophysical Journal Letters,2023,948(2):L12. |
| APA | Kann, D. A..,Agayeva, S..,Aivazyan, V..,Alishov, S..,Andrade, C. M..,...&Zhao, X. F..(2023).GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst-In Gedenken an David Alexander Kann.Astrophysical Journal Letters,948(2),L12. |
| MLA | Kann, D. A.,et al."GRANDMA and HXMT Observations of GRB 221009A: The Standard Luminosity Afterglow of a Hyperluminous Gamma-Ray Burst-In Gedenken an David Alexander Kann".Astrophysical Journal Letters 948.2(2023):L12. |
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| Kann-2023-GRANDMA an（3161KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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