A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015
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...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2019-06, Vol.485 (4), p.5294-5318 |
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| creator | Pandey, S B Hu, Y Castro-Tirado, Ao J Pozanenko, A S Sánchez-Ramírez, R Gorosabel, J Guziy, S Jelinek, M Tello, J C Jeong, S Oates, S R Zhang, B-B Mazaeva, E D Volnova, A A Minaev, P Yu van Eerten, H J Caballero-García, M D Pérez-Ramírez, D Bremer, M Winters, J-M Park, I H Guelbenzu, A Nicuesa Klose, S Moskvitin, A Sokolov, V V Sonbas, E Ayala, A Cepa, J Butler, N Troja, E Chernenko, A M Molkov, S V Volvach, A E Inasaridze, R Ya Egamberdiyev, Sh A Burkhonov, O Reva, I V Polyakov, K A Matkin, A A Ivanov, A L Molotov, I Guver, T Watson, A M Kutyrev, A Lee, W H Fox, O Littlejohns, O Cucchiara, A Gonzalez, J Richer, M G Román-Zúñiga, C G Tanvir, N R Bloom, J S Prochaska, J X Gehrels, N Moseley, H de Diego, J A Ramírez-Ruiz, E Klunko, E V Fan, Y Zhao, X Bai, J Wang, Ch Xin, Y Cui, Ch Tungalag, N Peng, Z-K Kumar, Amit Gupta, Rahul Aryan, Amar Kumar, Brajesh Volvach, L N Lamb, G P Valeev, A F |
| description | 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. |
| doi_str_mv | 10.1093/mnras/stz530 |
| format | Article |
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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.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stz530</identifier><language>eng</language><publisher>United States: Oxford University Press</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; Astrophysics ; gamma-rays: general ; NUCLEAR PHYSICS AND RADIATION PHYSICS ; Physics ; radiation mechanims : non-thermalonova ; techniques: photometric ; X-ray: bursts</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2019-06, Vol.485 (4), p.5294-5318</ispartof><rights>2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society 2019</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c432t-34c3666a9c7e9b6f756cf0e82332463eadbb7ffb49d08e2a6f30782bdd2eaaa53</citedby><cites>FETCH-LOGICAL-c432t-34c3666a9c7e9b6f756cf0e82332463eadbb7ffb49d08e2a6f30782bdd2eaaa53</cites><orcidid>0000-0002-7158-5099 ; 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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.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Astrophysics</subject><subject>gamma-rays: general</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>Physics</subject><subject>radiation mechanims : non-thermalonova</subject><subject>techniques: photometric</subject><subject>X-ray: 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PHYSICS</topic><topic>Physics</topic><topic>radiation mechanims : non-thermalonova</topic><topic>techniques: photometric</topic><topic>X-ray: bursts</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pandey, S B</creatorcontrib><creatorcontrib>Hu, Y</creatorcontrib><creatorcontrib>Castro-Tirado, Ao J</creatorcontrib><creatorcontrib>Pozanenko, A S</creatorcontrib><creatorcontrib>Sánchez-Ramírez, R</creatorcontrib><creatorcontrib>Gorosabel, J</creatorcontrib><creatorcontrib>Guziy, S</creatorcontrib><creatorcontrib>Jelinek, M</creatorcontrib><creatorcontrib>Tello, J C</creatorcontrib><creatorcontrib>Jeong, S</creatorcontrib><creatorcontrib>Oates, S R</creatorcontrib><creatorcontrib>Zhang, B-B</creatorcontrib><creatorcontrib>Mazaeva, E D</creatorcontrib><creatorcontrib>Volnova, A A</creatorcontrib><creatorcontrib>Minaev, P Yu</creatorcontrib><creatorcontrib>van Eerten, H J</creatorcontrib><creatorcontrib>Caballero-García, M D</creatorcontrib><creatorcontrib>Pérez-Ramírez, D</creatorcontrib><creatorcontrib>Bremer, M</creatorcontrib><creatorcontrib>Winters, J-M</creatorcontrib><creatorcontrib>Park, I H</creatorcontrib><creatorcontrib>Guelbenzu, A Nicuesa</creatorcontrib><creatorcontrib>Klose, S</creatorcontrib><creatorcontrib>Moskvitin, A</creatorcontrib><creatorcontrib>Sokolov, V V</creatorcontrib><creatorcontrib>Sonbas, E</creatorcontrib><creatorcontrib>Ayala, A</creatorcontrib><creatorcontrib>Cepa, J</creatorcontrib><creatorcontrib>Butler, N</creatorcontrib><creatorcontrib>Troja, E</creatorcontrib><creatorcontrib>Chernenko, A M</creatorcontrib><creatorcontrib>Molkov, S V</creatorcontrib><creatorcontrib>Volvach, A E</creatorcontrib><creatorcontrib>Inasaridze, R Ya</creatorcontrib><creatorcontrib>Egamberdiyev, Sh A</creatorcontrib><creatorcontrib>Burkhonov, O</creatorcontrib><creatorcontrib>Reva, I V</creatorcontrib><creatorcontrib>Polyakov, K A</creatorcontrib><creatorcontrib>Matkin, A A</creatorcontrib><creatorcontrib>Ivanov, A L</creatorcontrib><creatorcontrib>Molotov, I</creatorcontrib><creatorcontrib>Guver, T</creatorcontrib><creatorcontrib>Watson, A M</creatorcontrib><creatorcontrib>Kutyrev, A</creatorcontrib><creatorcontrib>Lee, W H</creatorcontrib><creatorcontrib>Fox, O</creatorcontrib><creatorcontrib>Littlejohns, O</creatorcontrib><creatorcontrib>Cucchiara, A</creatorcontrib><creatorcontrib>Gonzalez, J</creatorcontrib><creatorcontrib>Richer, M G</creatorcontrib><creatorcontrib>Román-Zúñiga, C G</creatorcontrib><creatorcontrib>Tanvir, N R</creatorcontrib><creatorcontrib>Bloom, J S</creatorcontrib><creatorcontrib>Prochaska, J X</creatorcontrib><creatorcontrib>Gehrels, N</creatorcontrib><creatorcontrib>Moseley, H</creatorcontrib><creatorcontrib>de Diego, J A</creatorcontrib><creatorcontrib>Ramírez-Ruiz, E</creatorcontrib><creatorcontrib>Klunko, E V</creatorcontrib><creatorcontrib>Fan, Y</creatorcontrib><creatorcontrib>Zhao, X</creatorcontrib><creatorcontrib>Bai, J</creatorcontrib><creatorcontrib>Wang, Ch</creatorcontrib><creatorcontrib>Xin, Y</creatorcontrib><creatorcontrib>Cui, Ch</creatorcontrib><creatorcontrib>Tungalag, N</creatorcontrib><creatorcontrib>Peng, Z-K</creatorcontrib><creatorcontrib>Kumar, Amit</creatorcontrib><creatorcontrib>Gupta, Rahul</creatorcontrib><creatorcontrib>Aryan, Amar</creatorcontrib><creatorcontrib>Kumar, Brajesh</creatorcontrib><creatorcontrib>Volvach, L N</creatorcontrib><creatorcontrib>Lamb, G P</creatorcontrib><creatorcontrib>Valeev, A F</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Pandey, S B</au><au>Hu, Y</au><au>Castro-Tirado, Ao J</au><au>Pozanenko, A S</au><au>Sánchez-Ramírez, R</au><au>Gorosabel, J</au><au>Guziy, S</au><au>Jelinek, M</au><au>Tello, J C</au><au>Jeong, S</au><au>Oates, S R</au><au>Zhang, B-B</au><au>Mazaeva, E D</au><au>Volnova, A A</au><au>Minaev, P Yu</au><au>van Eerten, H J</au><au>Caballero-García, M D</au><au>Pérez-Ramírez, D</au><au>Bremer, M</au><au>Winters, J-M</au><au>Park, I H</au><au>Guelbenzu, A Nicuesa</au><au>Klose, S</au><au>Moskvitin, A</au><au>Sokolov, V V</au><au>Sonbas, E</au><au>Ayala, A</au><au>Cepa, J</au><au>Butler, N</au><au>Troja, E</au><au>Chernenko, A M</au><au>Molkov, S V</au><au>Volvach, A E</au><au>Inasaridze, R Ya</au><au>Egamberdiyev, Sh A</au><au>Burkhonov, O</au><au>Reva, I V</au><au>Polyakov, K A</au><au>Matkin, A A</au><au>Ivanov, A L</au><au>Molotov, I</au><au>Guver, T</au><au>Watson, A M</au><au>Kutyrev, A</au><au>Lee, W H</au><au>Fox, O</au><au>Littlejohns, O</au><au>Cucchiara, A</au><au>Gonzalez, J</au><au>Richer, M G</au><au>Román-Zúñiga, C G</au><au>Tanvir, N R</au><au>Bloom, J S</au><au>Prochaska, J X</au><au>Gehrels, N</au><au>Moseley, H</au><au>de Diego, J A</au><au>Ramírez-Ruiz, E</au><au>Klunko, E V</au><au>Fan, Y</au><au>Zhao, X</au><au>Bai, J</au><au>Wang, Ch</au><au>Xin, Y</au><au>Cui, Ch</au><au>Tungalag, N</au><au>Peng, Z-K</au><au>Kumar, Amit</au><au>Gupta, Rahul</au><au>Aryan, Amar</au><au>Kumar, Brajesh</au><au>Volvach, L N</au><au>Lamb, G P</au><au>Valeev, A F</au><aucorp>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2019-06-01</date><risdate>2019</risdate><volume>485</volume><issue>4</issue><spage>5294</spage><epage>5318</epage><pages>5294-5318</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><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.</abstract><cop>United States</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/stz530</doi><tpages>25</tpages><orcidid>https://orcid.org/0000-0002-7158-5099</orcidid><orcidid>https://orcid.org/0000-0002-9008-592X</orcidid><orcidid>https://orcid.org/0000000271585099</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0035-8711 |
| ispartof | Monthly notices of the Royal Astronomical Society, 2019-06, Vol.485 (4), p.5294-5318 |
| issn | 0035-8711 1365-2966 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1572823 |
| source | Oxford Journals Open Access Collection |
| subjects | ASTRONOMY AND ASTROPHYSICS Astrophysics gamma-rays: general NUCLEAR PHYSICS AND RADIATION PHYSICS Physics radiation mechanims : non-thermalonova techniques: photometric X-ray: bursts |
| title | A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015 |
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