Published January 1, 2019
| Version v1
Journal article
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A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015
Creators
- Pandey, S. B.1
- Hu, Y.2
- Castro-Tirado, Ao J.
- Pozanenko, A. S.
- Sanchez-Ramirez, R.
- Gorosabel, J.
- Guziy, S.
- Jelinek, M.
- Tello, J. C.2
- Jeong, S.
- Oates, S. R.
- Zhang, B. -B.
- Mazaeva, E. D.3
- Volnova, A. A.3
- Minaev, P. Yu.3
- van Eerten, H. J.4
- Caballero-Garcia, M. D.
- Perez-Ramirez, D.5
- Bremer, M.6
- Winters, J. -M.6
- Winters, J. -M.6
- 1. Aryabhatta Res Inst Observat Sci, Naini Tal 263002, India
- 2. CSIC, IAA, Glorieta Astron S-N, E-18008 Granada, Spain
- 3. Space Res Inst, Moscow, Russia
- 4. Univ Bath, Dept Phys, Claverton Down, Bath BA2 7AY, Avon, England
- 5. Univ Jaen, Campus Las Lagunillas S-N, E-23071 Jaen, Spain
- 6. Inst Radioastron Millimetr IRAM, 300 Rue Piscine, F-38406 St Martin Dheres, France
Description
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 10.4m 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 sGRB130603B, the afterglowlight curve, containing both our new and previously published photometric data is broadly consistent with the ISMafterglowmodel. 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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