A Reverse Shock in GRB 181201A

Tanmoy Laskar, Hendrik Jan van Eerten, Patricia Schady, C. G. Mundell, Kate D. Alexander, Rodolfo Barniol Duran, Edo Berger, J. Bolmer, Ryan Chornock, Deanne L. Coppejans, Wen Fai Fong, Andreja Gomboc, Núria Jordana-Mitjans, Shiho Kobayashi, Raffaella Margutti, Karl M. Menten, Re'Em Sari, Ryo Yamazaki, V. M. Lipunov, E. Gorbovskoy & 9 others V. G. Kornilov, N. Tyurina, D. Zimnukhov, R. Podesta, H. Levato, D. A.H. Buckley, A. Tlatov, R. Rebolo, M. Serra-Ricart

Research output: Contribution to journalArticle

Abstract

We present comprehensive multiwavelength radio to X-ray observations of GRB 181201A spanning from ≈150 s to ≈163 days after the burst, comprising the first joint ALMA-VLA-GMRT observations of a gamma-ray burst (GRB) afterglow. The radio and millimeter-band data reveal a distinct signature at ≈3.9 days, which we interpret as reverse-shock (RS) emission. Our observations present the first time that a single radio-frequency spectral energy distribution can be decomposed directly into RS and forward shock (FS) components. We perform detailed modeling of the full multiwavelength data set, using Markov Chain Monte Carlo sampling to construct the joint posterior density function of the underlying physical parameters describing the RS and FS synchrotron emission. We uncover and account for all discovered degeneracies in the model parameters. The joint RS-FS modeling reveals a weakly magnetized (σ ≈ 3 × 10-3), mildly relativistic RS, from which we derive an initial bulk Lorentz factor of Γ0 ≈ 103 for the GRB jet. Our results support the hypothesis that low-density environments are conducive to the observability of RS emission. We compare our observations to other events with strong RS detections and find a likely observational bias selecting for longer lasting, nonrelativistic RSs. We present and begin to address new challenges in modeling posed by the present generation of comprehensive, multifrequency data sets.

Original languageEnglish
Article number121
JournalAstrophysical Journal
Volume884
Issue number2
DOIs
Publication statusPublished - 17 Oct 2019

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

A Reverse Shock in GRB 181201A. / Laskar, Tanmoy; van Eerten, Hendrik Jan; Schady, Patricia; Mundell, C. G.; Alexander, Kate D.; Duran, Rodolfo Barniol; Berger, Edo; Bolmer, J.; Chornock, Ryan; Coppejans, Deanne L.; Fong, Wen Fai; Gomboc, Andreja; Jordana-Mitjans, Núria; Kobayashi, Shiho; Margutti, Raffaella; Menten, Karl M.; Sari, Re'Em; Yamazaki, Ryo; Lipunov, V. M.; Gorbovskoy, E.; Kornilov, V. G.; Tyurina, N.; Zimnukhov, D.; Podesta, R.; Levato, H.; Buckley, D. A.H.; Tlatov, A.; Rebolo, R.; Serra-Ricart, M.

In: Astrophysical Journal, Vol. 884, No. 2, 121, 17.10.2019.

Research output: Contribution to journalArticle

Laskar, T, van Eerten, HJ, Schady, P, Mundell, CG, Alexander, KD, Duran, RB, Berger, E, Bolmer, J, Chornock, R, Coppejans, DL, Fong, WF, Gomboc, A, Jordana-Mitjans, N, Kobayashi, S, Margutti, R, Menten, KM, Sari, RE, Yamazaki, R, Lipunov, VM, Gorbovskoy, E, Kornilov, VG, Tyurina, N, Zimnukhov, D, Podesta, R, Levato, H, Buckley, DAH, Tlatov, A, Rebolo, R & Serra-Ricart, M 2019, 'A Reverse Shock in GRB 181201A', Astrophysical Journal, vol. 884, no. 2, 121. https://doi.org/10.3847/1538-4357/ab40ce
Laskar, Tanmoy ; van Eerten, Hendrik Jan ; Schady, Patricia ; Mundell, C. G. ; Alexander, Kate D. ; Duran, Rodolfo Barniol ; Berger, Edo ; Bolmer, J. ; Chornock, Ryan ; Coppejans, Deanne L. ; Fong, Wen Fai ; Gomboc, Andreja ; Jordana-Mitjans, Núria ; Kobayashi, Shiho ; Margutti, Raffaella ; Menten, Karl M. ; Sari, Re'Em ; Yamazaki, Ryo ; Lipunov, V. M. ; Gorbovskoy, E. ; Kornilov, V. G. ; Tyurina, N. ; Zimnukhov, D. ; Podesta, R. ; Levato, H. ; Buckley, D. A.H. ; Tlatov, A. ; Rebolo, R. ; Serra-Ricart, M. / A Reverse Shock in GRB 181201A. In: Astrophysical Journal. 2019 ; Vol. 884, No. 2.
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AU - Laskar, Tanmoy

AU - van Eerten, Hendrik Jan

AU - Schady, Patricia

AU - Mundell, C. G.

AU - Alexander, Kate D.

AU - Duran, Rodolfo Barniol

AU - Berger, Edo

AU - Bolmer, J.

AU - Chornock, Ryan

AU - Coppejans, Deanne L.

AU - Fong, Wen Fai

AU - Gomboc, Andreja

AU - Jordana-Mitjans, Núria

AU - Kobayashi, Shiho

AU - Margutti, Raffaella

AU - Menten, Karl M.

AU - Sari, Re'Em

AU - Yamazaki, Ryo

AU - Lipunov, V. M.

AU - Gorbovskoy, E.

AU - Kornilov, V. G.

AU - Tyurina, N.

AU - Zimnukhov, D.

AU - Podesta, R.

AU - Levato, H.

AU - Buckley, D. A.H.

AU - Tlatov, A.

AU - Rebolo, R.

AU - Serra-Ricart, M.

PY - 2019/10/17

Y1 - 2019/10/17

N2 - We present comprehensive multiwavelength radio to X-ray observations of GRB 181201A spanning from ≈150 s to ≈163 days after the burst, comprising the first joint ALMA-VLA-GMRT observations of a gamma-ray burst (GRB) afterglow. The radio and millimeter-band data reveal a distinct signature at ≈3.9 days, which we interpret as reverse-shock (RS) emission. Our observations present the first time that a single radio-frequency spectral energy distribution can be decomposed directly into RS and forward shock (FS) components. We perform detailed modeling of the full multiwavelength data set, using Markov Chain Monte Carlo sampling to construct the joint posterior density function of the underlying physical parameters describing the RS and FS synchrotron emission. We uncover and account for all discovered degeneracies in the model parameters. The joint RS-FS modeling reveals a weakly magnetized (σ ≈ 3 × 10-3), mildly relativistic RS, from which we derive an initial bulk Lorentz factor of Γ0 ≈ 103 for the GRB jet. Our results support the hypothesis that low-density environments are conducive to the observability of RS emission. We compare our observations to other events with strong RS detections and find a likely observational bias selecting for longer lasting, nonrelativistic RSs. We present and begin to address new challenges in modeling posed by the present generation of comprehensive, multifrequency data sets.

AB - We present comprehensive multiwavelength radio to X-ray observations of GRB 181201A spanning from ≈150 s to ≈163 days after the burst, comprising the first joint ALMA-VLA-GMRT observations of a gamma-ray burst (GRB) afterglow. The radio and millimeter-band data reveal a distinct signature at ≈3.9 days, which we interpret as reverse-shock (RS) emission. Our observations present the first time that a single radio-frequency spectral energy distribution can be decomposed directly into RS and forward shock (FS) components. We perform detailed modeling of the full multiwavelength data set, using Markov Chain Monte Carlo sampling to construct the joint posterior density function of the underlying physical parameters describing the RS and FS synchrotron emission. We uncover and account for all discovered degeneracies in the model parameters. The joint RS-FS modeling reveals a weakly magnetized (σ ≈ 3 × 10-3), mildly relativistic RS, from which we derive an initial bulk Lorentz factor of Γ0 ≈ 103 for the GRB jet. Our results support the hypothesis that low-density environments are conducive to the observability of RS emission. We compare our observations to other events with strong RS detections and find a likely observational bias selecting for longer lasting, nonrelativistic RSs. We present and begin to address new challenges in modeling posed by the present generation of comprehensive, multifrequency data sets.

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