A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015

S.B. Pandey, Y. Hu, A.J. Castro-Tirado, A.S. Pozanenko, R. Sanchez-Ramirez, J. Gorosabel, S. Guziy, M. Jelinek, S. Jeong, S.R. Oates, Bin-Bin Zhang, E.D. Mazaeva, A.A. Volnova, P.Yu. Minaev, Hendrik Van Eerten, M.D. Caballero-Garcia, D. Perez-Ramirez, M. Bremer, J.-M. Winters, I.H. Park & 53 others A. Nicuesa Guelbenzu, S. Klose, A. Moskvitin, V.V. Sokolov, E. Sonbas, A. Ayala, J. Cepa, N. Butler, Eleanora Troja, A.M. Chernenko, S.V. Molkov, A.E. Volvach, R.Ya. Inasaridze, Sh.A. Egamberdiyev, O. Burkhonov, I.V. Reva, K.A. Polyakov, A.A. Matkin, A.L. Ivanov, I. Molotov, T. Guver, A.M. Watson, A. Kutyrev, W.H. Lee, O. Fox, O. Littlejohns, A. Cucchiara, J. Gonzalez, M.G. Richer, C.G. Roman-Zuniga, N.R. Tanvir, J.S. Bloom, J.X. Prochaska, N. Gehrels, H. Moseley, J.A. de Diego, E. Ramirez-Ruiz, E.V. Klunko, Y. Fan, X. Zhao, J. Bai, Ch. Wang, Y. Xin, Ch. Cui, N. Tungalag, Z.-K. Peng, Amit Kumar, Rahul Gupta, Amar Aryan, Brajesh Kumar, L.N. Volvach, G.P. Lamb, A.F. Valeev

Research output: Contribution to journalArticle

2 Citations (Scopus)

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 languageEnglish
Pages (from-to)5294-5318
Number of pages25
JournalMonthly Notices of the Royal Astronomical Society
Volume485
Issue number4
Early online date25 Feb 2019
DOIs
Publication statusPublished - 1 Jun 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

Cite this

Pandey, S. B., Hu, Y., Castro-Tirado, A. J., Pozanenko, A. S., Sanchez-Ramirez, R., Gorosabel, J., ... 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. https://doi.org/10.1093/mnras/stz530

A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015. / Pandey, S.B.; Hu, Y.; Castro-Tirado, A.J.; Pozanenko, A.S.; Sanchez-Ramirez, R.; Gorosabel, J.; Guziy, S.; Jelinek, M.; Jeong, S.; Oates, S.R.; Zhang, Bin-Bin; Mazaeva, E.D.; Volnova, A.A.; Minaev, P.Yu.; Van Eerten, Hendrik; Caballero-Garcia, M.D.; Perez-Ramirez, 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, Eleanora; 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.; Roman-Zuniga, C.G.; Tanvir, N.R.; Bloom, J.S.; Prochaska, J.X.; Gehrels, N.; Moseley, H.; de Diego, J.A.; Ramirez-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, 01.06.2019, p. 5294-5318.

Research output: Contribution to journalArticle

Pandey, SB, Hu, Y, Castro-Tirado, AJ, Pozanenko, AS, Sanchez-Ramirez, R, Gorosabel, J, Guziy, S, Jelinek, M, Jeong, S, Oates, SR, Zhang, B-B, Mazaeva, ED, Volnova, AA, Minaev, PY, Van Eerten, H, Caballero-Garcia, MD, Perez-Ramirez, D, Bremer, M, Winters, J-M, Park, IH, Nicuesa Guelbenzu, A, Klose, S, Moskvitin, A, Sokolov, VV, Sonbas, E, Ayala, A, Cepa, J, Butler, N, Troja, E, Chernenko, AM, Molkov, SV, Volvach, AE, Inasaridze, RY, Egamberdiyev, SA, Burkhonov, O, Reva, IV, Polyakov, KA, Matkin, AA, Ivanov, AL, Molotov, I, Guver, T, Watson, AM, Kutyrev, A, Lee, WH, Fox, O, Littlejohns, O, Cucchiara, A, Gonzalez, J, Richer, MG, Roman-Zuniga, CG, Tanvir, NR, Bloom, JS, Prochaska, JX, Gehrels, N, Moseley, H, de Diego, JA, Ramirez-Ruiz, E, Klunko, EV, Fan, Y, Zhao, X, Bai, J, Wang, C, Xin, Y, Cui, C, Tungalag, N, Peng, Z-K, Kumar, A, Gupta, R, Aryan, A, Kumar, B, Volvach, LN, Lamb, GP & Valeev, AF 2019, 'A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015', Monthly Notices of the Royal Astronomical Society, vol. 485, no. 4, pp. 5294-5318. https://doi.org/10.1093/mnras/stz530
Pandey, S.B. ; Hu, Y. ; Castro-Tirado, A.J. ; Pozanenko, A.S. ; Sanchez-Ramirez, R. ; Gorosabel, J. ; Guziy, S. ; Jelinek, M. ; Jeong, S. ; Oates, S.R. ; Zhang, Bin-Bin ; Mazaeva, E.D. ; Volnova, A.A. ; Minaev, P.Yu. ; Van Eerten, Hendrik ; Caballero-Garcia, M.D. ; Perez-Ramirez, 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, Eleanora ; 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. ; Roman-Zuniga, C.G. ; Tanvir, N.R. ; Bloom, J.S. ; Prochaska, J.X. ; Gehrels, N. ; Moseley, H. ; de Diego, J.A. ; Ramirez-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. / A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 485, No. 4. pp. 5294-5318.
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title = "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 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.",
keywords = "Gamma-rays: general, Radiation mechanims: non-thermalonova, Techniques: photometric, X-ray: bursts",
author = "S.B. Pandey and Y. Hu and A.J. Castro-Tirado and A.S. Pozanenko and R. Sanchez-Ramirez and J. Gorosabel and S. Guziy and M. Jelinek and S. Jeong and S.R. Oates and Bin-Bin Zhang and E.D. Mazaeva and A.A. Volnova and P.Yu. Minaev and {Van Eerten}, Hendrik and M.D. Caballero-Garcia and D. Perez-Ramirez and M. Bremer and J.-M. Winters and I.H. Park and {Nicuesa Guelbenzu}, A. and S. Klose and A. Moskvitin and V.V. Sokolov and E. Sonbas and A. Ayala and J. Cepa and N. Butler and Eleanora Troja and A.M. Chernenko and S.V. Molkov and A.E. Volvach and R.Ya. Inasaridze and Sh.A. Egamberdiyev and O. Burkhonov and I.V. Reva and K.A. Polyakov and A.A. Matkin and A.L. Ivanov and I. Molotov and T. Guver and A.M. Watson and A. Kutyrev and W.H. Lee and O. Fox and O. Littlejohns and A. Cucchiara and J. Gonzalez and M.G. Richer and C.G. Roman-Zuniga and N.R. Tanvir and J.S. Bloom and J.X. Prochaska and N. Gehrels and H. Moseley and {de Diego}, J.A. and E. Ramirez-Ruiz and E.V. Klunko and Y. Fan and X. Zhao and J. Bai and Ch. Wang and Y. Xin and Ch. Cui and N. Tungalag and Z.-K. Peng and Amit Kumar and Rahul Gupta and Amar Aryan and Brajesh Kumar and L.N. Volvach and G.P. Lamb and A.F. Valeev",
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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, A.J.

AU - Pozanenko, A.S.

AU - Sanchez-Ramirez, R.

AU - Gorosabel, J.

AU - Guziy, S.

AU - Jelinek, M.

AU - Jeong, S.

AU - Oates, S.R.

AU - Zhang, Bin-Bin

AU - Mazaeva, E.D.

AU - Volnova, A.A.

AU - Minaev, P.Yu.

AU - Van Eerten, Hendrik

AU - Caballero-Garcia, M.D.

AU - Perez-Ramirez, 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, Eleanora

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 - Roman-Zuniga, 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 - Ramirez-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.

PY - 2019/6/1

Y1 - 2019/6/1

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

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U2 - 10.1093/mnras/stz530

DO - 10.1093/mnras/stz530

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SP - 5294

EP - 5318

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

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ER -