A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015 | |
Pandey, S. B.1; Hu, Y.2; Castro-Tirado, Ao J.2,3; Pozanenko, A. S.12,13,36; Sánchez-Ramírez, R.2,38; Gorosabel, J.2,4,5; Guziy, S.2,6,7; Jelinek, M.2,9; Tello, J. C.2; Jeong, S.2,8; Oates, S. R.2,41; Zhang, B.-B.2,39,40; Mazaeva, E. D.12; Volnova, A. A.12; Minaev, P. Yu.12; Eerten, H. J.42; García, M. D.2,9; Pérez-Ramírez, D.10; Bremer, M.11; Winters, J.-M.11; Park, I. H.8; Nicuesa Guelbenzu, A.14; Klose, S.14; Moskvitin, A.15; Sokolov, V. V.15; Sonbas, E.16; Ayala, A.2; Cepa, J.17; Butler, N.18; Troja, E.19; Chernenko, A. M.12; Molkov, S. V.12; Volvach, A. E.20; Inasaridze, R. Ya.21,43; Egamberdiyev, Sh. A.22; Burkhonov, O.22; Reva, I. V.23; Polyakov, K. A.24; Matkin, A. A.25; Ivanov, A. L.26; Molotov, I.37; Guver, T.27; Watson, A. M.44; Kutyrev, A.19; Lee, W. H.44; Fox, O.30; Littlejohns, O.18; Cucchiara, A.19; Gonzalez, J.44; Richer, M. G.28; Zúñiga, C. G.28; Tanvir, N. R.29; Bloom, J. S.30; Prochaska, J. X.31; Gehrels, N.19; Moseley, H.19; Diego, J. A.44; Ramírez-Ruiz, E.31; Klunko, E. V.32; Fan YF(范玉峰)33![]() ![]() ![]() ![]() ![]() | |
发表期刊 | Monthly Notices of the Royal Astronomical Society
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2019-03-13 | |
卷号 | 485期号:4页码:5294-5318 |
DOI | 10.1093/mnras/stz530 |
产权排序 | 第33完成单位 |
收录类别 | SCI ; EI |
关键词 | gamma-rays: general X-ray: bursts techniques: photometric radiation mechanims : non-thermalonova |
摘要 | We investigate the prompt emission and the afterglow properties of short-duration gamma-ray burst (sGRB) 130603B and another eight sGRB events during 2012-2015, observed by several multiwavelength facilities including the Gran Canarias Telescope 10.4 m telescope. Prompt emission high energy data of the events were obtained by INTEGRAL-SPI-ACS, Swift-BAT, and Fermi-GBM satellites. The prompt emission data by INTEGRAL in the energy range of 0.1-10 MeV for sGRB 130603B, sGRB 140606A, sGRB 140930B, sGRB 141212A, and sGRB 151228A do not show any signature of the extended emission or precursor activity and their spectral and temporal properties are similar to those seen in case of other short bursts. For sGRB 130603B, our new afterglow photometric data constrain the pre-jet-break temporal decay due to denser temporal coverage. For sGRB 130603B, the afterglow light curve, containing both our new and previously published photometric data is broadly consistent with the ISM afterglow model. Modeling of the host galaxies of sGRB 130603B and sGRB 141212A using the LePHARE software supports a scenario in which the environment of the burst is undergoing moderate star formation activity. From the inclusion of our late-time data for eight other sGRBs we are able to: place tight constraints on the non-detection of the afterglow, host galaxy, or any underlying 'kilonova' emission. Our late-time afterglow observations of the sGRB 170817A/GW170817 are also discussed and compared with the sub-set of sGRBs. © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society |
资助项目 | Junta de Andalucia[P07-TIC-03094] ; Spanish Ministry[AYA2012-39727-C03-01] ; Spanish Ministry[201571718R] ; Spanish Science Ministry 'Centro de Excelencia SeveroOchoa' Program[SEV-2017-0709] ; Max-Planck-Institut for Astronomie ; FEDER[xa52] ; FEDER[s14dd001] ; FEDER[s14dd002] ; FEDER[s14dd006] ; BRICS[DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017] ; INSU/CNRS (France) ; MPG (Germany) ; IGN (Spain) ; Leverhulme Trust Early Career Fellowship[NRF-2014R1A6A3A03057484] ; Leverhulme Trust Early Career Fellowship[NRF-2015R1D1A4A01020961] ; Scientific and Technological Research Council of Turkey (TUBITAK)[112T224] ; TUBITAK[10CT100-95] ; RFBR[17-02-01388] ; RFBR[17-51-44018] ; RFBR[1752-80139] ; RSCF[18-12-00522] ; National Thousand Young Talents program of China ; National Key Research and Development Program of China[2018YFA0404204] ; National Key Research and Development Program of China[RUSTAVELI/FR/379/6-300/14] ; Universidad Nacional Autonoma de Mexico ; Teledyne Scientific and Imaging ; NASA[NNX09AH71G] ; NASA[NNX09AT02G] ; NASA[NNX10AI27G] ; NASA[NNX12AE66G] ; CONACyT[INFR-2009-01-122785] ; CONACyT[CB2008-101958] ; UNAM PAPIIT[IN113810] ; UC MEXUS-CONACyT grant[CN 09-283] ; ASI (Italian Space Agency)[2015-046R.0] ; European Union Horizon 2020 Programme under the AHEAD project[NRF-2015R1D1A4A01020961] ; European Union Horizon 2020 Programme under the AHEAD project[654215] ; STFC[ST/P006892/1] ; STFC[ST/S006176/1] ; STFC[ST/S000453/1] Funding Source: UKRI |
项目资助者 | Junta de Andalucia[P07-TIC-03094] ; Spanish Ministry[AYA2012-39727-C03-01, 201571718R] ; Spanish Science Ministry 'Centro de Excelencia SeveroOchoa' Program[SEV-2017-0709] ; Max-Planck-Institut for Astronomie ; FEDER[xa52, s14dd001, s14dd002, s14dd006] ; BRICS[DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017] ; INSU/CNRS (France) ; MPG (Germany) ; IGN (Spain) ; Leverhulme Trust Early Career Fellowship[NRF-2014R1A6A3A03057484, NRF-2015R1D1A4A01020961] ; Scientific and Technological Research Council of Turkey (TUBITAK)[112T224] ; TUBITAK[10CT100-95] ; RFBR[17-02-01388, 17-51-44018, 1752-80139] ; RSCF[18-12-00522] ; National Thousand Young Talents program of China ; National Key Research and Development Program of China[2018YFA0404204, RUSTAVELI/FR/379/6-300/14] ; Universidad Nacional Autonoma de Mexico ; Teledyne Scientific and Imaging ; NASA[NNX09AH71G, NNX09AT02G, NNX10AI27G, NNX12AE66G] ; CONACyT[INFR-2009-01-122785, CB2008-101958] ; UNAM PAPIIT[IN113810] ; UC MEXUS-CONACyT grant[CN 09-283] ; ASI (Italian Space Agency)[2015-046R.0] ; European Union Horizon 2020 Programme under the AHEAD project[NRF-2015R1D1A4A01020961, 654215] ; STFC[ST/P006892/1, ST/S006176/1, ST/S000453/1] Funding Source: UKRI |
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 University Press |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
ISSN | 0035-8711 |
URL | 查看原文 |
WOS记录号 | WOS:000474880400063 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | GAMMA-RAY BURSTS ; NEUTRON-STAR ; LIGHT CURVES ; ELECTROMAGNETIC COUNTERPART ; INTERSTELLAR EXTINCTION ; SPECTRAL EVOLUTION ; EXTENDED EMISSION ; AFTERGLOW ; NUCLEOSYNTHESIS ; KILONOVA |
EI入藏号 | 20221612001588 |
EI主题词 | Stars |
EI分类号 | 657.2 Extraterrestrial Physics and Stellar Phenomena - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics - 941.4 Optical Variables Measurements |
引用统计 | |
文献类型 | 期刊论文 |
版本 | 出版稿 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/25185 |
专题 | 南方基地 星系类星体研究组 |
通讯作者 | Pandey, S. B.; Zhang, B.-B. |
作者单位 | 1.Aryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital, 263 002, India; 2.Instituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, Granada, E-18008, Spain; 3.Unidad Asociada Departamento de Ingeniería de Sistemas y Automática, E.T.S. de Ingenieros Industriales, Universidad de Málaga, E-29071, Spain; 4.Unidad Asociada Grupo Ciencias Planetarias UPV/EHU-IAA/CSIC, Departamento de Fisica Aplicada I, E.T.S., Universidad del Pais Vasco UPV/EHU, Bilbao, E-48071, Spain; 5.Ikerbasque, Basque Foundation for Science, Bilbao, E-48013, Spain; 6.Nikolaev National University, Nikolska 24, Nikolaev, 54030, Ukraine; 7.Nikolaev Astronomical Observatory, Nikolaev, Ukraine; 8.Institute for Science and Technology in Space, SungKyunKwan University, Suwon, 16419, Korea, Republic of; 9.Astronomical Institute of the Academy of Sciences, Boní II 1401, Praha 4, CZ-14100, Czech Republic; 10.Universidad de Jaén, Campus Las Lagunillas, s/n, Jaén, E-23071, Spain; 11.Institute de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, Saint Martin d'Hères, F-38406, France; 12.Space Research Institute, Moscow, Russia; 13.National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow, Russia; 14.Thuringer Landessternwarte, Tautenburg, Germany; 15.Special Astrophysical Observatory, Nizhniy Arkhyz, Zelenchukskiy Region, Karachai-Cherkessian, 369167, Russia; 16.Department of Physics, University of Adiyaman, Adiyaman, 02040, Turkey; 17.Instituto de Astrofsica ´ de Canarias (IAC), Vía L'actea s/n, Santa Cruz de La Laguna, Tenerife, 38205, Spain; 18.School of Earth and Space Exploration, Arizona State University, Tempe, AZ, 85287, United States; 19.NASA, Goddard Space Flight Center, Greenbelt, MD, 20771, United States; 20.Radio Astronomy Laboratory of the Crimean Astrophysical Observatory, Katsiveli, Crimea, Russia; 21.Kharadze Abastumani Astrophysical Observatory of Ilya State University, K. Cholokashvili Ave. 3/5, Tbilisi, 0162, Georgia; 22.Ulugh Beg Astronomical Institute, Uzbek Academy of Sciences, Tashkent, Uzbekistan; 23.Fesenkov Astrophysical Institute, Almaty, Kazakhstan; 24.Astronomical Scientific Center, Moscow, Russia; 25.Ussuriysk Astrophysical Observatory of Far-East Department of Russian Academy of Sciences, Ussuriysk, Russia; 26.Kuban State University, Krasnodar, Russia; 27.Istanbul University Science Faculty, Department of Astronomy and Space Sciences, University-Istanbul, 34119, Turkey; 28.Instituto de Astronomia, UNAM, Unidad Academica en Ensenada, Ensenada, 22860, Mexico; 29.University of Leicester, Department of Physics and Astronomy, Leicester Institute of Space and Earth Observation, University Road, Leicester, LE1 7RH, United Kingdom; 30.Astronomy Department, University of California, Berkeley, CA, 94720-7450, United States; 31.Department of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA, 95064, United States; 32.Institute of Solar-Terrestrial Physics, Irkutsk, Russia; 33.Yunnan Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, Kunming, Yunnan, 650011, China; 34.Beijing National Astronomical Observatory, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, China; 35.Center of Astronomy and Geophysics, Mongolian Academy of Sciences, Ulaanbaatar, Mongolia; 36.National Research University Higher School of Economics, Moscow, 101000, Russia; 37.Keldysh Institute of Applied Mathematics, Moscow, Russia; 38.INAF - Istituto di Astrofisica e Planetologia Spaziali, Via Fosso del Cavaliere 100, Roma, 00133, Italy; 39.Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing, 210093, China; 40.School of Astronomy and Space Science, Nanjing University, Nanjing, 210093, China; 41.Department of Physics, University of Warwick, Coventry, CV4 7AL, United Kingdom; 42.Department of Physics, University of Bath, Claverton Down, Bath, BA2 7AY, United Kingdom; 43.Samtskhe Javakheti State University, Rustaveli st.113, Akhaltsikhe, GA, 0080, United States; 44.Instituto de Astronomía, Universidad Nacional Autónoma de Mèxico, Apartado Postal 70-264, México, CDMX, 04510, Mexico |
推荐引用方式 GB/T 7714 | Pandey, S. B.,Hu, Y.,Castro-Tirado, Ao J.,et al. A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015[J]. Monthly Notices of the Royal Astronomical Society,2019,485(4):5294-5318. |
APA | Pandey, S. B..,Hu, Y..,Castro-Tirado, Ao J..,Pozanenko, A. S..,Sánchez-Ramírez, R..,...&Valeev, A. F..(2019).A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015.Monthly Notices of the Royal Astronomical Society,485(4),5294-5318. |
MLA | Pandey, S. B.,et al."A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015".Monthly Notices of the Royal Astronomical Society 485.4(2019):5294-5318. |
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