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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 5294-5318 |
| Number of pages | 25 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 485 |
| Issue number | 4 |
| DOIs | |
| State | Published - Mar 13 2019 |
Keywords
- Gamma-rays: general
- Radiation mechanims: non-thermalonova
- Techniques: photometric
- X-ray: bursts
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015. / 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.; Nicuesa Guelbenzu, A.; 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.
In: Monthly Notices of the Royal Astronomical Society, Vol. 485, No. 4, 13.03.2019, p. 5294-5318.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015
AU - Pandey, S. B.
AU - Hu, Y.
AU - Castro-Tirado, Ao J.
AU - Pozanenko, A. S.
AU - Sánchez-Ramírez, R.
AU - Gorosabel, J.
AU - Guziy, S.
AU - Jelinek, M.
AU - Tello, J. C.
AU - Jeong, S.
AU - Oates, S. R.
AU - Zhang, B. B.
AU - Mazaeva, E. D.
AU - Volnova, A. A.
AU - Minaev, P. Yu
AU - Van Eerten, H. J.
AU - Caballero-García, M. D.
AU - Pérez-Ramírez, D.
AU - Bremer, M.
AU - Winters, J. M.
AU - Park, I. H.
AU - Nicuesa Guelbenzu, A.
AU - Klose, S.
AU - Moskvitin, A.
AU - Sokolov, V. V.
AU - Sonbas, E.
AU - Ayala, A.
AU - Cepa, J.
AU - Butler, N.
AU - Troja, E.
AU - Chernenko, A. M.
AU - Molkov, S. V.
AU - Volvach, A. E.
AU - Inasaridze, R. Ya
AU - Egamberdiyev, Sh A.
AU - Burkhonov, O.
AU - Reva, I. V.
AU - Polyakov, K. A.
AU - Matkin, A. A.
AU - Ivanov, A. L.
AU - Molotov, I.
AU - Guver, T.
AU - Watson, A. M.
AU - Kutyrev, A.
AU - Lee, W. H.
AU - Fox, O.
AU - Littlejohns, O.
AU - Cucchiara, A.
AU - Gonzalez, J.
AU - Richer, M. G.
AU - Román-Zúñiga, C. G.
AU - Tanvir, N. R.
AU - Bloom, J. S.
AU - Prochaska, J. X.
AU - Gehrels, N.
AU - Moseley, H.
AU - De Diego, J. A.
AU - Ramírez-Ruiz, E.
AU - Klunko, E. V.
AU - Fan, Y.
AU - Zhao, X.
AU - Bai, J.
AU - Wang, Ch
AU - Xin, Y.
AU - Cui, Ch
AU - Tungalag, N.
AU - Peng, Z. K.
AU - Kumar, Amit
AU - Gupta, Rahul
AU - Aryan, Amar
AU - Kumar, Brajesh
AU - Volvach, L. N.
AU - Lamb, G. P.
AU - Valeev, A. F.
N1 - Funding Information: Swift data/science center is thankfully acknowledged for the publi-cally available data about GRBs. AJCT acknowledges support from the Junta de Andalucia (Project P07-TIC-03094) and support from the Spanish Ministry Projects AYA2012-39727-C03-01 and 2015-71718R. This work has been supported by the Spanish Science Ministry 'Centro de Excelencia Severo Ochoa' Program under grant SEV-2017-0709. The work is partly based on the observations made with the Gran Telescopio Canarias (GTC), installed in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, in the island of La Palma Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut for Astronomie and the Instituto de Astrofisica de Andalucia (CSIC). This research was also partially based on observations carried out at the OSN operated by CSIC. FEDER funds are acknowledged. This work is partly based on observations carried out under project numbers xa52, s14dd001, s14dd002, and s14dd006 with the IRAM NOEMA Interferometer (http://www.iram-institute.org/EN/conten t-page-188-7-55-188-0-0.html). S.B.P. acknowledge BRICS grant number 'DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017(G)' for this work. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). SRO gratefully acknowledges the support of the Leverhulme Trust Early Career Fellowship. SJ acknowledges support from Korean grants NRF-2014R1A6A3A03057484 and NRF-2015R1D1A4A01020961. E.S. acknowledges assistance from the Scientific and Technological Research Council of Turkey (TUBITAK) through project 112T224. We thank TUBITAK for a partial support in using T100 telescope with project number 10CT100-95. S.B.P. acknowledge discussions with Dr. Masaomi Tanaka on kilonovae and related science. A.S.P acknowledges partial support grants RFBR 17-02-01388, 17-51-44018, and 17-52-80139. E.D.M., A.A.V., and P.Yu.M. are grateful to RSCF grant 18-12-00522 for support. B.-B.Z. acknowledges support from National Thousand Young Talents program of China and National Key Research and Development Program of China (2018YFA0404204). R.Ya.I. is grateful for partial support by the grant RUSTAVELI/FR/379/6-300/14. We thank the RATIR project team and the staff of the Observatorio Astronómico Nacional on Sierra San Pedro Mártir. RATIR is a collaboration between the University of California, the Universidad Nacional Autonóma de México, NASA Goddard Space Flight Center, and Arizona State University, benefiting from the loan of an H2RG detector and hardware and software support from Teledyne Scientific and Imaging. RATIR, the automation of the Harold L. Johnson Telescope of the Observatorio Astronomico Nacional on Sierra San Pedro Martir, and the operation of both are funded through NASA grants NNX09AH71G, NNX09AT02G, NNX10AI27G, and NNX12AE66G, CONACyT grants INFR-2009-01-122785 and CB-2008-101958, UNAM PAPIIT grant IN113810, and UC MEXUS-CONACyT grant CN 09-283. R.S.R. acknowledges support from ASI (Italian Space Agency) through the Contract No. 2015-046-R.0 and from European Union Horizon 2020 Programme under the AHEAD project (grant agreement No. 654215). SJ acknowledges the support of the Korea Basic Science Research Program through NRF-2015R1D1A4A01020961. Mondy observations were performed with budgetary funding of Basic Research program II.16 and the data were obtained using the equipment of Center for Common Use 'Angara' (http://ckp-rf.ru/ckp/3056/). We are also thankful to I. Márquez for useful discussions. Funding Information: Swift data/science center is thankfully acknowledged for the publically available data about GRBs. AJCT acknowledges support from the Junta de Andalucia (Project P07-TIC-03094) and support from the Spanish Ministry Projects AYA2012-39727-C03-01 and 2015-71718R. This work has been supported by the Spanish Science Ministry ‘Centro de Excelencia Severo Ochoa’ Program under grant SEV-2017-0709. The work is partly based on the observations made with the Gran Telescopio Canarias (GTC), installed in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, in the island of La Palma Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut for Astronomie and the Instituto de Astrofisica de Andalucia (CSIC). This research was also partially based on observations carried out at the OSN operated by CSIC. FEDER funds are acknowledged. This work is partly based on observations carried out under project numbers xa52, s14dd001, s14dd002, and s14dd006 with the IRAM NOEMA Interferometer (http://www.iram-institute.org/EN/conten t-page-188-7-55-188-0-0.html). S.B.P. acknowledge BRICS grant number ‘DST/IMRCD/BRICS/PilotCall1/ProFCheap/2017(G)’ for this work. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). SRO gratefully acknowledges the support of the Leverhulme Trust Early Career Fellowship. SJ acknowledges support from Korean grants NRF-2014R1A6A3A03057484 and NRF-2015R1D1A4A01020961. E.S. acknowledges assistance from the Scientific and Technological Research Council of Turkey (TUBITAK) through project 112T224. We thank TUBITAK for a partial support in using T100 telescope with project number 10CT100-95. S.B.P. acknowledge discussions with Dr. Masaomi Tanaka on kilonovae and related science. A.S.P acknowledges partial support grants RFBR 17-02-01388, 17-51-44018, and 17-52-80139. E.D.M., A.A.V., and P.Yu.M. are grateful to RSCF grant 18-12-00522 for support. B.-B.Z. acknowledges support from National Thousand Young Talents program of China and National Key Research and Development Program of China (2018YFA0404204). R.Ya.I. is grateful for partial support by the grant RUSTAVELI/FR/379/6-300/14. We thank the RATIR project team and the staff of the Observatorio Astronómico Nacional on Sierra San Pedro Mártir. RATIR is a collaboration between the University of California, the Universidad Nacional Autonóma de México, NASA Goddard Space Flight Center, and Arizona State University, benefiting from the loan of an H2RG detector and hardware and software support from Teledyne Scientific and Imaging. RATIR, the automation of the Harold L. Johnson Telescope of the Observatorio Astronomico Nacional on Sierra San Pedro Martir, and the operation of both are funded through NASA grants NNX09AH71G, NNX09AT02G, NNX10AI27G, and NNX12AE66G, CONACyT grants INFR-2009-01-122785 and CB-2008-101958, UNAM PAPIIT grant IN113810, and UC MEXUS-CONACyT grant CN 09-283. R.S.R. acknowledges support from ASI (Italian Space Agency) through the Contract No. 2015-046-R.0 and from European Union Horizon 2020 Programme under the AHEAD project (grant agreement No. 654215). SJ acknowledges the support of the Korea Basic Science Research Program through NRF-2015R1D1A4A01020961. Mondy observations were performed with budgetary funding of Basic Research program II.16 and the data were obtained using the equipment of Center for Common Use ‘Angara’ (http://ckp-rf.ru/ckp/3056/). We are also thankful to I. Márquez for useful discussions. Publisher Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
PY - 2019/3/13
Y1 - 2019/3/13
N2 - 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.
AB - 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.
KW - Gamma-rays: general
KW - Radiation mechanims: non-thermalonova
KW - Techniques: photometric
KW - X-ray: bursts
UR - http://www.scopus.com/inward/record.url?scp=85067046867&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85067046867&partnerID=8YFLogxK
U2 - 10.1093/mnras/stz530
DO - 10.1093/mnras/stz530
M3 - Article
AN - SCOPUS:85067046867
VL - 485
SP - 5294
EP - 5318
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 4
ER -