A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015
S. B. PandeyAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263 002, IndiaY. D. HuInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainA. J. Castro‐TiradoInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainA. PozanenkoNational Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow, RussiaR. Sánchez-RamírezINAF - Istituto di Astrofisica e Planetologia Spaziali, Via Fosso del Cavaliere 100, 00133 Roma, ItalyJ. GorosabelIkerbasque, Basque Foundation for Science, Bilbao, E-48013, SpainS. GuziyInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainM. JelínekAstronomical Institute of the Academy of Sciences, Boční II 1401, CZ-14100 Praha 4, Czech RepublicJ. C. TelloInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainS. JeongInstitute for Science and Technology in Space, SungKyunKwan University, Suwon 16419, KoreaS. R. OatesDepartment of Physics, University of Warwick, Coventry CV4 7AL, UKB-B ZhangInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainE. MazaevaSpace Research institute, Moscow, RussiaA. VolnovaSpace Research institute, Moscow, RussiaP. Yu. MinaevSpace Research institute, Moscow, RussiaH J van EertenDepartment of Physics, University of Bath, Claverton Down, Bath BA2 7AY, UKM. D. Caballero‐GarcíaAstronomical Institute of the Academy of Sciences, Boční II 1401, CZ-14100 Praha 4, Czech RepublicD. Pérez-RamírezUniversidad de Jaén, Campus Las Lagunillas, s/n, Jaén, E-23071, SpainMichael BremerInstitute de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, F-38406 Saint Martin d’Hères, FranceJ-M WintersInstitute de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, F-38406 Saint Martin d’Hères, FranceIl Han ParkInstitute for Science and Technology in Space, SungKyunKwan University, Suwon 16419, KoreaA. Nicuesa GuelbenzuThuringer Landessternwarte, Tautenburg, GermanyS. KloseThuringer Landessternwarte, Tautenburg, GermanyА. С. МосквитинSpecial Astrophysical Observatory, Nizhniy Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Respublic, 369167, RussiaВ. В. СоколовSpecial Astrophysical Observatory, Nizhniy Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Respublic, 369167, RussiaЭ. СонбасDepartment of Physics, University of Adiyaman, 02040 Adiyaman, TurkeyA. AyalaInstituto de Astrofisica de Andalucia (IAA-CSIC), Glorieta de la Astronomia s/n, E-18008, Granada, SpainJ. CepaInstituto de Astrofśica de Canarias (IAC), Vía L’actea s/n, 38205 Santa Cruz de La Laguna, Tenerife, SpainN. ButlerSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USAE. TrojaNASA, Goddard Space Flight Center, Greenbelt, MD 20771, USAA. ChernenkoSpace Research institute, Moscow, RussiaS. MolkovSpace Research institute, Moscow, RussiaA. E. VolvachRadio Astronomy Laboratory of the Crimean Astrophysical Observatory, Katsiveli, CrimeaR. InasaridzeKharadze Abastumani Astrophysical Observatory of Ilya State University, K. Cholokashvili Ave. 3/5, Tbilisi 0162, GeorgiaSh. A. EgamberdiyevUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Tashkent, UsbekistanО. БурхоновUlugh Beg Astronomical InstituteI. RevaFesenkov Astrophysical Institute, Almaty, KazakhstanK. A. PolyakovA. MatkinUssuriysk Astrophysical observatory of Far-East Department of Russian Academy of Sciences, Ussuriysk, RussiaA. IvanovKuban State University, Krasnodar, RussiaI. MolotovKeldysh Institute of Applied Mathematics, Moscow, RussiaTolga GüverIstanbul University Science Faculty, Department of Astronomy and Space Sciences, 34119, University-Istanbul, TurkeyA. M. WatsonInstituto de Astronomía, Universidad Nacional Autónoma de Mèxico, Apartado Postal 70-264, 04510 México, CDMX, MexicoA. KutyrevNASA, Goddard Space Flight Center, Greenbelt, MD 20771, USAWilliam H. LeeInstituto de Astronomía, Universidad Nacional Autónoma de Mèxico, Apartado Postal 70-264, 04510 México, CDMX, MexicoO. FoxAstronomy Department, University of California, Berkeley, CA 94720-7450, USAO. LittlejohnsSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USAAntonino CucchiaraNASA, Goddard Space Flight Center, Greenbelt, MD 20771, USAJ. González‐HernándezInstituto de Astronomía, Universidad Nacional Autónoma de Mèxico, Apartado Postal 70-264, 04510 México, CDMX, MexicoM. G. RicherInstituto de Astronomia, UNAM, Unidad Academica en Ensenada. Ensenada 22860 MexicoC. Román-ZúñigaInstituto de Astronomia, UNAM, Unidad Academica en Ensenada. Ensenada 22860 MexicoN. R. TanvirUniversity of Leicester, Department of Physics & Astronomy and Leicester Institute of Space & Earth Observation, University Road, Leicester LE1 7RH, UKJ. S. BloomAstronomy Department, University of California, Berkeley, CA 94720-7450, USAJ. X. ProchaskaDepartment of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA 95064, USAN. GehrelsNASA, Goddard Space Flight Center, Greenbelt, MD 20771, USAH. MoseleyNASA, Goddard Space Flight Center, Greenbelt, MD 20771, USAJ. A. de DiegoInstituto de Astronomía, Universidad Nacional Autónoma de Mèxico, Apartado Postal 70-264, 04510 México, CDMX, MexicoE. Ramírez-RuizDepartment of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA 95064, USAE. KlunkoInstitute of Solar-Terrestrial Physics, Irkutsk, RussiaY. L. FanYunnan National Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, 650011 Kunming, Yunnan, ChinaXiaohong ZhaoYunnan National Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, 650011 Kunming, Yunnan, ChinaJ. M. BaiYunnan National Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, 650011 Kunming, Yunnan, ChinaChunhui WangYunnan National Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, 650011 Kunming, Yunnan, ChinaYu XinYunnan National Astronomical Observatory, Chinese Academy of Sciences, Phoenix Hill, 650011 Kunming, Yunnan, ChinaCh. CuiBeijing National Astronomical Observatory, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, ChinaN. TungalagCenter of Astronomy and Geophysics Mongolian Academy of Sciences, Ulaanbaatar, MongoliaZ-K PengSchool of Astronomy and Space Science, Nanjing University, 210093, Nanjing, ChinaAmit KumarAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263 002, IndiaRahul GuptaAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263 002, IndiaAmar AryanAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263 002, IndiaBrajesh KumarAryabhatta Research Institute of Observational Sciences, Manora Peak, Nainital 263 002, IndiaL. N. VolvachRadio Astronomy Laboratory of the Crimean Astrophysical Observatory, Katsiveli, CrimeaGavin P. LambUniversity of Leicester, Department of Physics & Astronomy and Leicester Institute of Space & Earth Observation, University Road, Leicester LE1 7RH, UKA. F. ValeevSpecial Astrophysical Observatory, Nizhniy Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Respublic, 369167, Russia
ABI
Abstract
Abstract 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.
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