The supernova of the MAGIC gamma-ray burst GRB 190114C

A. Melandri; L. Izzo; E. Pian; D. B. Malesani; M. Della Valle; A. Rossi; P. DAvanzo; D. Guetta; P. A. Mazzali; S. Benetti; N. Masetti; E. Palazzi; S. Savaglio; L. Amati; L. A. Antonelli; C. Ashall; M. G. Bernardini; S. Campana; R. Carini; S. Covino; V. DElia; A. De Ugarte Postigo; M. De Pasquale; A. V. Filippenko; A. S. Fruchter; J. P.U. Fynbo; A. Giunta; D. H. Hartmann; P. Jakobsson; J. Japelj; P. G. Jonker; D. A. Kann; G. P. Lamb; A. J. Levan; A. Martin-Carrillo; P. Møller; S. Piranomonte; G. Pugliese; R. Salvaterra; S. Schulze; R. L.C. Starling; L. Stella; G. Tagliaferri; N. Tanvir; D. Watson

doi:10.1051/0004-6361/202141788

The supernova of the MAGIC gamma-ray burst GRB 190114C

A. Melandri
, L. Izzo
, E. Pian
, D. B. Malesani
, M. Della Valle
, A. Rossi
, P. DAvanzo
, D. Guetta
, P. A. Mazzali
, S. Benetti
, N. Masetti
, E. Palazzi
, S. Savaglio
, L. Amati
, L. A. Antonelli
, C. Ashall
, M. G. Bernardini
, S. Campana
, R. Carini
, S. Covino

V. DElia, A. De Ugarte Postigo, M. De Pasquale, A. V. Filippenko, A. S. Fruchter, J. P.U. Fynbo, A. Giunta, D. H. Hartmann, P. Jakobsson, J. Japelj, P. G. Jonker, D. A. Kann, G. P. Lamb, A. J. Levan, A. Martin-Carrillo, P. Møller, S. Piranomonte, G. Pugliese, R. Salvaterra, S. Schulze, R. L.C. Starling, L. Stella, G. Tagliaferri, N. Tanvir, D. Watson

Faculty of Physical Sciences

University of Iceland

Research output: Contribution to journal › Article › peer-review

Abstract

We observed GRB 190114C (redshift z = 0.4245), the first gamma-ray burst (GRB) ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hubble Space Telescope, with the primary goal of studying its underlying supernova, SN 2019jrj. The monitoring spanned the time interval between 1.3 and 370 days after the burst, in the observer frame. We find that the afterglow emission can be modelled with a forward shock propagating in a uniform medium modified by time-variable extinction along the line of sight. A jet break could be present after 7 rest-frame days, and accordingly the maximum luminosity of the underlying supernova (SN) ranges between that of stripped-envelope core-collapse SNe of intermediate luminosity and that of the luminous GRB-associated SN 2013dx. The observed spectral absorption lines of SN 2019jrj are not as broad as in classical GRB SNe and are instead more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN 2004aw as an analogue, we tentatively derive the basic physical properties of SN 2019jrj. We discuss the possibility that a fraction of the TeV emission of this source might have had a hadronic origin and estimate the expected high-energy neutrino detection level with IceCube.

Original language	English
Article number	A39
Journal	Astronomy and Astrophysics
Volume	659
DOIs	https://doi.org/10.1051/0004-6361/202141788
Publication status	Published - 1 Mar 2022

Bibliographical note

Funding Information: Acknowledgements. We thank the anonymous referee for valuable comments and suggestions that improved the paper. A. M., M. G. B., P. D. A., S. C., and G. T. acknowledge support from ASI grant I/004/11/5. P. D. A., M. D. V., E. Pa., S. Sa., and S. P. acknowledge support from PRIN-MIUR 2017 (grant 20179ZF5KS). L. I. was supported by the VILLUM FONDEN (project numbers 16599 and 25501). D. B. M. acknowledges support from research grant 19054 from VILLUM FONDEN. A. V. F.’s research is supported by the Christopher R. Redlich Fund, the Miller Institute for Basic Research in Science (in which he is a Senior Miller Fellow), and many individual donors. D. A. K. acknowledges support from Spanish National Research Project RTI2018-098104-JI00 (GRBPhot). D. W. is supported by Independent Research Fund Denmark grant DFF–7014-00017. The Cosmic Dawn Center is supported by the Danish National Research Foundation under grant 140. A. R. acknowledges support from the project Supporto Arizona and Italia. The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are The University of Arizona on behalf of the Arizona Board of Regents; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsge-sellschaft, Germany, representing the Max-Planck Society, The Leibniz Institute for Astrophysics Potsdam, and Heidelberg University; The Ohio State University, representing OSU, University of Notre Dame, University of Minnesota, and University of Virginia. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. Publisher Copyright: ©

Other keywords

Gamma-ray burst: individual: GRB 190114C
Supernovae: individual: SN 2019jrj

Access to Document

10.1051/0004-6361/202141788

Cite this

Melandri, A., Izzo, L., Pian, E., Malesani, D. B., Della Valle, M., Rossi, A., DAvanzo, P., Guetta, D., Mazzali, P. A., Benetti, S., Masetti, N., Palazzi, E., Savaglio, S., Amati, L., Antonelli, L. A., Ashall, C., Bernardini, M. G., Campana, S., Carini, R., ... Watson, D. (2022). The supernova of the MAGIC gamma-ray burst GRB 190114C. Astronomy and Astrophysics, 659, Article A39. https://doi.org/10.1051/0004-6361/202141788

@article{0f9ee522a6644849b29ae76c32bf9e05,

title = "The supernova of the MAGIC gamma-ray burst GRB 190114C",

abstract = "We observed GRB 190114C (redshift z = 0.4245), the first gamma-ray burst (GRB) ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hubble Space Telescope, with the primary goal of studying its underlying supernova, SN 2019jrj. The monitoring spanned the time interval between 1.3 and 370 days after the burst, in the observer frame. We find that the afterglow emission can be modelled with a forward shock propagating in a uniform medium modified by time-variable extinction along the line of sight. A jet break could be present after 7 rest-frame days, and accordingly the maximum luminosity of the underlying supernova (SN) ranges between that of stripped-envelope core-collapse SNe of intermediate luminosity and that of the luminous GRB-associated SN 2013dx. The observed spectral absorption lines of SN 2019jrj are not as broad as in classical GRB SNe and are instead more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN 2004aw as an analogue, we tentatively derive the basic physical properties of SN 2019jrj. We discuss the possibility that a fraction of the TeV emission of this source might have had a hadronic origin and estimate the expected high-energy neutrino detection level with IceCube.",

keywords = "Gamma-ray burst: individual: GRB 190114C, Supernovae: individual: SN 2019jrj",

author = "A. Melandri and L. Izzo and E. Pian and Malesani, \{D. B.\} and \{Della Valle\}, M. and A. Rossi and P. DAvanzo and D. Guetta and Mazzali, \{P. A.\} and S. Benetti and N. Masetti and E. Palazzi and S. Savaglio and L. Amati and Antonelli, \{L. A.\} and C. Ashall and Bernardini, \{M. G.\} and S. Campana and R. Carini and S. Covino and V. DElia and \{De Ugarte Postigo\}, A. and \{De Pasquale\}, M. and Filippenko, \{A. V.\} and Fruchter, \{A. S.\} and Fynbo, \{J. P.U.\} and A. Giunta and Hartmann, \{D. H.\} and P. Jakobsson and J. Japelj and Jonker, \{P. G.\} and Kann, \{D. A.\} and Lamb, \{G. P.\} and Levan, \{A. J.\} and A. Martin-Carrillo and P. M{\o}ller and S. Piranomonte and G. Pugliese and R. Salvaterra and S. Schulze and Starling, \{R. L.C.\} and L. Stella and G. Tagliaferri and N. Tanvir and D. Watson",

note = "Funding Information: Acknowledgements. We thank the anonymous referee for valuable comments and suggestions that improved the paper. A. M., M. G. B., P. D. A., S. C., and G. T. acknowledge support from ASI grant I/004/11/5. P. D. A., M. D. V., E. Pa., S. Sa., and S. P. acknowledge support from PRIN-MIUR 2017 (grant 20179ZF5KS). L. I. was supported by the VILLUM FONDEN (project numbers 16599 and 25501). D. B. M. acknowledges support from research grant 19054 from VILLUM FONDEN. A. V. F.{\textquoteright}s research is supported by the Christopher R. Redlich Fund, the Miller Institute for Basic Research in Science (in which he is a Senior Miller Fellow), and many individual donors. D. A. K. acknowledges support from Spanish National Research Project RTI2018-098104-JI00 (GRBPhot). D. W. is supported by Independent Research Fund Denmark grant DFF–7014-00017. The Cosmic Dawn Center is supported by the Danish National Research Foundation under grant 140. A. R. acknowledges support from the project Supporto Arizona and Italia. The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are The University of Arizona on behalf of the Arizona Board of Regents; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsge-sellschaft, Germany, representing the Max-Planck Society, The Leibniz Institute for Astrophysics Potsdam, and Heidelberg University; The Ohio State University, representing OSU, University of Notre Dame, University of Minnesota, and University of Virginia. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. Publisher Copyright: {\textcopyright}",

year = "2022",

month = mar,

day = "1",

doi = "10.1051/0004-6361/202141788",

language = "English",

volume = "659",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Melandri, A, Izzo, L, Pian, E, Malesani, DB, Della Valle, M, Rossi, A, DAvanzo, P, Guetta, D, Mazzali, PA, Benetti, S, Masetti, N, Palazzi, E, Savaglio, S, Amati, L, Antonelli, LA, Ashall, C, Bernardini, MG, Campana, S, Carini, R, Covino, S, DElia, V, De Ugarte Postigo, A, De Pasquale, M, Filippenko, AV, Fruchter, AS, Fynbo, JPU, Giunta, A, Hartmann, DH, Jakobsson, P, Japelj, J, Jonker, PG, Kann, DA, Lamb, GP, Levan, AJ, Martin-Carrillo, A, Møller, P, Piranomonte, S, Pugliese, G, Salvaterra, R, Schulze, S, Starling, RLC, Stella, L, Tagliaferri, G, Tanvir, N & Watson, D 2022, 'The supernova of the MAGIC gamma-ray burst GRB 190114C', Astronomy and Astrophysics, vol. 659, A39. https://doi.org/10.1051/0004-6361/202141788

TY - JOUR

T1 - The supernova of the MAGIC gamma-ray burst GRB 190114C

AU - Melandri, A.

AU - Izzo, L.

AU - Pian, E.

AU - Malesani, D. B.

AU - Della Valle, M.

AU - Rossi, A.

AU - DAvanzo, P.

AU - Guetta, D.

AU - Mazzali, P. A.

AU - Benetti, S.

AU - Masetti, N.

AU - Palazzi, E.

AU - Savaglio, S.

AU - Amati, L.

AU - Antonelli, L. A.

AU - Ashall, C.

AU - Bernardini, M. G.

AU - Campana, S.

AU - Carini, R.

AU - Covino, S.

AU - DElia, V.

AU - De Ugarte Postigo, A.

AU - De Pasquale, M.

AU - Filippenko, A. V.

AU - Fruchter, A. S.

AU - Fynbo, J. P.U.

AU - Giunta, A.

AU - Hartmann, D. H.

AU - Jakobsson, P.

AU - Japelj, J.

AU - Jonker, P. G.

AU - Kann, D. A.

AU - Lamb, G. P.

AU - Levan, A. J.

AU - Martin-Carrillo, A.

AU - Møller, P.

AU - Piranomonte, S.

AU - Pugliese, G.

AU - Salvaterra, R.

AU - Schulze, S.

AU - Starling, R. L.C.

AU - Stella, L.

AU - Tagliaferri, G.

AU - Tanvir, N.

AU - Watson, D.

N1 - Funding Information: Acknowledgements. We thank the anonymous referee for valuable comments and suggestions that improved the paper. A. M., M. G. B., P. D. A., S. C., and G. T. acknowledge support from ASI grant I/004/11/5. P. D. A., M. D. V., E. Pa., S. Sa., and S. P. acknowledge support from PRIN-MIUR 2017 (grant 20179ZF5KS). L. I. was supported by the VILLUM FONDEN (project numbers 16599 and 25501). D. B. M. acknowledges support from research grant 19054 from VILLUM FONDEN. A. V. F.’s research is supported by the Christopher R. Redlich Fund, the Miller Institute for Basic Research in Science (in which he is a Senior Miller Fellow), and many individual donors. D. A. K. acknowledges support from Spanish National Research Project RTI2018-098104-JI00 (GRBPhot). D. W. is supported by Independent Research Fund Denmark grant DFF–7014-00017. The Cosmic Dawn Center is supported by the Danish National Research Foundation under grant 140. A. R. acknowledges support from the project Supporto Arizona and Italia. The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are The University of Arizona on behalf of the Arizona Board of Regents; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsge-sellschaft, Germany, representing the Max-Planck Society, The Leibniz Institute for Astrophysics Potsdam, and Heidelberg University; The Ohio State University, representing OSU, University of Notre Dame, University of Minnesota, and University of Virginia. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. Publisher Copyright: ©

PY - 2022/3/1

Y1 - 2022/3/1

N2 - We observed GRB 190114C (redshift z = 0.4245), the first gamma-ray burst (GRB) ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hubble Space Telescope, with the primary goal of studying its underlying supernova, SN 2019jrj. The monitoring spanned the time interval between 1.3 and 370 days after the burst, in the observer frame. We find that the afterglow emission can be modelled with a forward shock propagating in a uniform medium modified by time-variable extinction along the line of sight. A jet break could be present after 7 rest-frame days, and accordingly the maximum luminosity of the underlying supernova (SN) ranges between that of stripped-envelope core-collapse SNe of intermediate luminosity and that of the luminous GRB-associated SN 2013dx. The observed spectral absorption lines of SN 2019jrj are not as broad as in classical GRB SNe and are instead more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN 2004aw as an analogue, we tentatively derive the basic physical properties of SN 2019jrj. We discuss the possibility that a fraction of the TeV emission of this source might have had a hadronic origin and estimate the expected high-energy neutrino detection level with IceCube.

AB - We observed GRB 190114C (redshift z = 0.4245), the first gamma-ray burst (GRB) ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hubble Space Telescope, with the primary goal of studying its underlying supernova, SN 2019jrj. The monitoring spanned the time interval between 1.3 and 370 days after the burst, in the observer frame. We find that the afterglow emission can be modelled with a forward shock propagating in a uniform medium modified by time-variable extinction along the line of sight. A jet break could be present after 7 rest-frame days, and accordingly the maximum luminosity of the underlying supernova (SN) ranges between that of stripped-envelope core-collapse SNe of intermediate luminosity and that of the luminous GRB-associated SN 2013dx. The observed spectral absorption lines of SN 2019jrj are not as broad as in classical GRB SNe and are instead more similar to those of less-luminous core-collapse SNe. Taking the broad-lined stripped-envelope core-collapse SN 2004aw as an analogue, we tentatively derive the basic physical properties of SN 2019jrj. We discuss the possibility that a fraction of the TeV emission of this source might have had a hadronic origin and estimate the expected high-energy neutrino detection level with IceCube.

KW - Gamma-ray burst: individual: GRB 190114C

KW - Supernovae: individual: SN 2019jrj

UR - https://www.scopus.com/pages/publications/85126487171

U2 - 10.1051/0004-6361/202141788

DO - 10.1051/0004-6361/202141788

M3 - Article

SN - 0004-6361

VL - 659

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A39

ER -

The supernova of the MAGIC gamma-ray burst GRB 190114C

Abstract

Bibliographical note

Other keywords

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