Multiband analyses of the bright GRB 230812B and the associated SN2023pel

doi:10.1093/mnras/stae503

YNAO OpenIR > 南方基地

	Multiband analyses of the bright GRB 230812B and the associated SN2023pel
	Hussenot-Desenonges, T 1; Wouters, T 2,3; Guessoum, N 4; Abdi, I 4; Abulwfa, A 5; Adami, C 6; Fernández, J F Agüí 7; Ahumada, T 8; Aivazyan, V 9,10; Akl, D 4; Anand, S 8; Andrade, C M 11; Antier, S 12; Ata, S A 5; D’Avanzo, P 13; Azzam, Y A 5; Baransky, A 14; Basa, S 6; Blazek, M 15,16; Bendjoya, P 17; Beradze, S 9,10; Boumis, P 18; Bremer, M 19; Brivio, R 13,20; Buat, V 6; Bulla, M 21,22,23; Burkhonov, O 24; Burns, E 25; Cenko, S B 26,27; Coughlin, M W 11; Corradi, W 28; Daigne, F 29; Dietrich, T 30,31; Dornic, D 32; Ducoin, J -G 29,32; Duverne, P -A 33; Elhosseiny, E G 5; Elnagahy, F I 5; El-Sadek, M A 5; Ferro, M 13,20; Floc’h, E Le 34; Freeberg, M 35; Fynbo, J P U 36,37; Götz, D 34; Gurbanov, E 38; Hamed, G M 5; Hasanov, E 38; Healy, B F 11; Heintz, K E 36,37; Hello, P 1; Inasaridze, R 9,10; Iskandar, A 39; Ismailov, N 38; Izzo, L 40,41; Jhawar, S 30; Laz, T Jegou du 42; Kamel, T M 5; Karpov, S 15; Klotz, A 43,44; Koulouridis, E 18; Kuin, N P 45; Kochiashvili, N 9; Leonini, S 46; Lu KX(卢开兴)47 ; Malesani, D B 36,37,48; Mašek, M 49; Mao JR(毛基荣)47,50,51 ; Melandri, A 13,52; Mihov, B M 53; Natsvlishvili, R 9; Navarete, F 54; Nedora, V 31; Nicolas, J 12; Odeh, M 12; Palmerio, J 55; Pang, P T H 2,3; Pasquale, M De 56; Peng, H W 57; Pormente, S 12; Peloton, J 1; Pradier, T 58; Pyshna, O 14; Rajabov, Y 24; Rakotondrainibe, N A 6; Rivet, J -P 17; Rousselot, L 12; Saccardi, A 55; Sasaki, N 28; Schneider, B 59; Serrau, M 60; Shokry, A 5; Slavcheva-Mihova, L 53; Simon, A 61,62; Sokoliuk, O 14,63; Srinivasaragavan, G 26,27,64; Strausbaugh, R 65; Takey, A 5; Tanvir, N R 66; Thöne, C C 67; Tillayev, Y 24,68; Melo, I Tosta e 69; Turpin, D 34; Postigo, A de Ugarte 6,12; Vasylenko, V 61,62; Vergani, S D 55; Vidadi, Z 38; Xu, D 51; Wang, L T 39; Wang, X F 57,70; Winters, J M 19; Zhang XL(张西亮)47 ; Zhu, Z 51,71
发表期刊	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2024-04-05
卷号	530 期号:1 页码:1-19
DOI	10.1093/mnras/stae503
产权排序	第47完成单位
收录类别	SCI ; EI
关键词	methods: statistical techniques: photometric techniques: spectroscopic gamma-ray burst: individual: GRB 230812B gamma-ray bursts transients: supernovae
摘要	GRB 230812B is a bright and relatively nearby (z = 0.36) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray, ultraviolet, optical, infrared, and submillimetre bands from the GRANDMA (Global Rapid Advanced Network for Multimessenger Addicts) network of observatories and from observational partners. Adding complementary data from the literature, we then derive essential physical parameters associated with the ejecta and external properties (i.e. the geometry and environment) of the GRB and compare with other analyses of this event. We spectroscopically confirm the presence of an associated supernova, SN2023pel, and we derive a photospheric expansion velocity of v similar to 17 x 10(3) km s(-1). We analyse the photometric data first using empirical fits of the flux and then with full Bayesian inference. We again strongly establish the presence of a supernova in the data, with a maximum (pseudo-)bolometric luminosity of 5.75 x 10(42) erg s(-1), at 15.76(-1.21)(+0.81) days (in the observer frame) after the trigger, with a half-max time width of 22.0 days. We compare these values with those of SN1998bw, SN2006aj, and SN2013dx. Our best-fit model favours a very low density environment (log(10)(n(ISM)/cm(-3))=-2.38(-1.60)(+1.45)) and small values for the jet's core angle theta(core)=1.54(-0.81)(+1.02) deg and viewing angle theta(obs)=0.76(-0.76)(+1.29) deg. GRB 230812B is thus one of the best observed afterglows with a distinctive supernova bump.
资助项目	CNRS; Netherlands Organization for Scientific Research (NWO); Programme National Hautes Energies (PNHE); National Science Foundation[PHY-2347628]; National Science Foundation[OAC-2117997]; National Science Foundation[2138259]; National Science Foundation[2138286]; National Science Foundation[2138307]; National Science Foundation[2137603]; National Science Foundation[2138296]; Preparing for Astrophysics with LSST Program - Heising-Simons Foundation[2021-2975]; Science, Technology & Innovation Funding Authority (STDF)[45779]; European Structural and Investment Fund; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/15_003/0000437]; UKSA Swift; American University of Sharjah (UAE)[FRG22-C-S68]; Ministry of Education of the Czech Republic[LM2023032]; Ministry of Education of the Czech Republic[LM2023047]; National Key R & D Program of China[2023YFE0101200]; Yunnan Revitalization Talent Support Program (YunLing Scholar Award); NSFC[12393813]; European Research Council (ERC) under the European Union[101071865]; Ile-de-France Region within the framework of the Domaine d'Interet Majeur-Astrophysique et Conditions d'Apparition de la Vie (DIM-ACAV); NOIRLab; IdEx Universite de Paris Cite[ANR-18-IDEX-0001]; Paris-Saclay, IJCLAB; INSU/CNRS (France); MPG (Germany); IGN (Spain); Danish National Research Foundation
项目资助者	CNRS ; Netherlands Organization for Scientific Research (NWO) ; Programme National Hautes Energies (PNHE) ; National Science Foundation[PHY-2347628, OAC-2117997, 2138259, 2138286, 2138307, 2137603, 2138296] ; Preparing for Astrophysics with LSST Program - Heising-Simons Foundation[2021-2975] ; Science, Technology & Innovation Funding Authority (STDF)[45779] ; European Structural and Investment Fund ; Czech Ministry of Education, Youth and Sports[CZ.02.1.01/0.0/0.0/15_003/0000437] ; UKSA Swift ; American University of Sharjah (UAE)[FRG22-C-S68] ; Ministry of Education of the Czech Republic[LM2023032, LM2023047] ; National Key R & D Program of China[2023YFE0101200] ; Yunnan Revitalization Talent Support Program (YunLing Scholar Award) ; NSFC[12393813] ; European Research Council (ERC) under the European Union[101071865] ; Ile-de-France Region within the framework of the Domaine d'Interet Majeur-Astrophysique et Conditions d'Apparition de la Vie (DIM-ACAV) ; NOIRLab ; IdEx Universite de Paris Cite[ANR-18-IDEX-0001] ; Paris-Saclay, IJCLAB ; INSU/CNRS (France) ; MPG (Germany) ; IGN (Spain) ; Danish National Research Foundation
语种	英语
学科领域	天文学 ; 星系与宇宙学
文章类型	Article
出版者	OXFORD UNIV PRESS
出版地	GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN	0035-8711
URL	查看原文
WOS记录号	WOS:001202100700001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	GAMMA-RAY BURST ; LIGHT CURVES ; DATA RELEASE ; X-RAY ; AFTERGLOWS ; SUPERNOVA ; SWIFT ; LONG ; EMISSION ; SPECTRA
EI入藏号	20241515900382
EI主题词	Supernovae
EI分类号	657.2 Extraterrestrial Physics and Stellar Phenomena - 723.4.1 Expert Systems - 921.4 Combinatorial Mathematics, Includes Graph Theory, Set Theory - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics - 941.4 Optical Variables Measurements
引用统计	被引频次：1[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/27058
专题	南方基地中国科学院天体结构与演化重点实验室星系类星体研究组
作者单位	1.IJCLab, Univ Paris-Saclay, CNRS/IN2P3 Orsay, 91405, France; 2.Nikhef, Science Park 105, NL-1098 XG Amsterdam, the Netherlands; 3.Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, NL-3584 CC Utrecht, the Netherlands; 4.Physics Department, American University of Sharjah, Sharjah, 26666, UAE; 5.National Research Institute of Astronomy and Geophysics (NRIAG), 1 El-marsad St., 11421 Helwan, Cairo, Egypt; 6.Aix Marseille Univ, CNRS, CNES, 13388 LAM Marseille, France; 7.Instituto de Astrofísica de Andalucía, Glorieta de la Astronomía s/n, E-18008 Granada, Spain; 8.Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA; 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.School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA; 12.Observatoire de la Côte d’Azur, Université Côte d’Azur, Boulevard de l’Observatoire, F-06304 Nice, France; 13.INAF–Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate (LC), Italy; 14.Astronomical Observatory of Taras Shevchenko National University of Kyiv, Observatorna Str. 3, UA-04053 Kyiv, Ukraine; 15.CEICO, Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, CZ-182 21 Praha, Czech Republic; 16.Centro Astronómico Hispano en Andalucía, Observatorio de Calar Alto, Sierra de los Filabres, E-04550 Gérgal, Almería, Spain; 17.Laboratoire J.-L. Lagrange, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, F-06304 Nice, France; 18.National Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, GR-15236 Penteli, Greece; 19.Institut de Radioastronomie Millimétrique, Saint-Martin-d'Hères, 38406, France; 20.Università degli Studi dell’Insubria, Dipartimento di Scienza e Alta Tecnologia, Via Valleggio 11, I-22100 Como, Italy; 21.Department of Physics and Earth Science, University of Ferrara, via Saragat 1, I-44122 Ferrara, Italy; 22.INFN, Sezione di Ferrara, via Saragat 1, I-44122 Ferrara, Italy; 23.INAF, Osservatorio Astronomico d’Abruzzo, via Mentore Maggini snc, I-64100 Teramo, Italy; 24.Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy Str. 33, Tashkent 100052, Uzbekistan; 25.Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803, USA; 26.Astrophysics Science Division, NASA Goddard Space Flight Center, 8800 Greenbelt Rd, Greenbelt, MD 20771, USA; 27.Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA; 28.Laboratório Nacional de Astrofísica - LNA, Rua Estados Unidos, 154 Itajubá - MG CEP 37504-364, Brazil; 29.Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98 bis bd Arago, F-75014 Paris, France; 30.Institute for Physics and Astronomy, University of Potsdam, Haus 28, Karl-Liebknecht-Str. 24/25, D-14476 Potsdam, Germany; 31.Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, D-14476 Potsdam, Germany; 32.Aix Marseille Univ, CNRS/IN2P3, CPPM, 13288 Marseille, France; 33.Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France; 34.Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France; 35.KNC, AAVSO, Hidden Valley Observatory (HVO), Colfax, WI, 54730, USA; iTelescope, New Mexico Skies Observatory, Mayhill, NM, 88339, USA; 36.Cosmic Dawn Center (DAWN), 2200 Copenhagen, Denmark; 37.Niels Bohr Institute, University of Copenhagen, Jagtvej 128, DK-2200 Copenhagen N, Denmark; 38.N. Tusi Shamakhy Astrophysical Observatory, Ministry of Science and Education, settl. Y. Mammadaliyev, AZ-5626 Shamakhy, Azerbaijan; 39.Xinjiang Astronomical Observatory (XAO), Chinese Academy of Sciences, Urumqi 830011, P. R. China; 40.INAF–Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Napoli, Italy; 41.DARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 128, DK-2200 Copenhagen N, Denmark; 42.Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA; 43.IRAP, Université de Toulouse, CNRS, UPS, 14 Avenue Edouard Belin, F-31400 Toulouse, France; 44.Université Paul Sabatier Toulouse III, Université de Toulouse, 118 Route de Narbonne, F-31400 Toulouse, France; 45.Mullard Space Science Laboratory, University College London, Holmbury St. Mary Dorking RH5 6NT, UK; 46.Montarrenti Observatory, S. S. 73 Ponente, I-53018 Sovicille, Siena, Italy; 47.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, P. R. China; 48.Department of Astrophysics/IMAPP, Radboud University, NL-6525 AJ Nijmegen, the Netherlands; 49.FZU–Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, CZ-182 21 Praha, Czech Republic; 50.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, 100012 Beijing, P. R. China; 51.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, P. R. China; 52.INAF–Osservatorio Astronomico di Roma, Via di Frascati 33, I-00040 Monte Porzio Catone (RM), Italy; 53.Institute of Astronomy and NAO, Bulgarian Academy of Sciences, 72 Tsarigradsko Chaussee Blvd., 1784 Sofia, Bulgaria; 54.SOAR Telescope/NSF’s NOIRLab Avda Juan Cisternas 1500, 1700000 La Serena, Chile; 55.GEPI, Observatoire de Paris, Université PSL, CNRS, 5 place Jules Janssen, F-92190 Meudon, France; 56.Mathematics, Informatics, Physics and Earth Science Department, University of Messina, Via F.D. D’Alcontres 31, Polo Papardo, I-98166 Messina, Italy; 57.Physics Department, Tsinghua University, Beijing 100084, P. R. China; 58.Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France; 59.Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Ave, Cambridge, MA 02139, USA; 60.Société Astronomique de France, Observatoire de Dauban, F-04150 Banon, France; 61.Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv, Glushkova Ave., 4, UA-03022 Kyiv, Ukraine; 62.National Center Junior Academy of Sciences of Ukraine, Dehtiarivska St. 38-44, UA-04119 Kyiv, Ukraine; 63.Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Acad. Zabolotnoho Str., UA-03143 Kyiv, Ukraine; 64.Department of Astronomy, University of Maryland, College Park, MD 20742, USA; 65.Department of Physics, Eastern Illinois University, Charleston, IL 61920, USA; 66.Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK; 67.Astronomical Institute of the Czech Academy of Sciences (ASU-CAS), Fricova 298, CZ-251 65 Ondřejov, Czech Republic; 68.National University of Uzbekistan, Department of Astronomy and Atmospheric Physics, 4 University Str., Tashkent 100174, Uzbekistan; 69.Department of Physics and Astronomy, University of Catania, Via Santa Sofia 64, I-95123 Catania, Italy; 70.Beijing Planetarium, Beijing Academy of Science and Technology, Beijing 100044, P. R. China; 71.Department of Astronomy, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China
推荐引用方式 GB/T 7714	Hussenot-Desenonges, T,Wouters, T,Guessoum, N,et al. Multiband analyses of the bright GRB 230812B and the associated SN2023pel[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,530(1):1-19.
APA	Hussenot-Desenonges, T.,Wouters, T.,Guessoum, N.,Abdi, I.,Abulwfa, A.,...&Zhu, Z.(2024).Multiband analyses of the bright GRB 230812B and the associated SN2023pel.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,530(1),1-19.
MLA	Hussenot-Desenonges, T,et al."Multiband analyses of the bright GRB 230812B and the associated SN2023pel".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 530.1(2024):1-19.

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