The supernova of the MAGIC gamma-ray burst GRB190114C

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The supernova of the MAGIC gamma-ray burst GRB190114C. / Melandri, A.; Izzo, L.; Pian, E.; Malesani, D. B.; Della Valle, M.; Rossi, A.; D'Avanzo, 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.; Covino, S.; D'Elia, Valerio; de Ugarte Postigo, A.; De Pasquale, M.; Filippenko, A.; Fruchter, A. S.; Fynbo, J. P. U.; Giunta, A.; Hartmann, D. H.; Jakobsson, P.; Japelj, J.; Jonker, P. G.; Kann, D. A.; Lamb, G. P.; Levan, A. J.; Martin-Carrillo, A.; Moller, P.; Piranomonte, S.; Pugliese, G.; Salvaterra, R.; Schulze, S.; Starling, R. L. C.; Stella, L.; Tagliaferri, G.; Tanvir, N.; Watson, D.

In: Astronomy & Astrophysics, Vol. 659, 39, 01.03.2022.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Melandri, A, Izzo, L, Pian, E, Malesani, DB, Della Valle, M, Rossi, A, D'Avanzo, 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, D'Elia, V, de Ugarte Postigo, A, De Pasquale, M, Filippenko, A, Fruchter, AS, Fynbo, JPU, Giunta, A, Hartmann, DH, Jakobsson, P, Japelj, J, Jonker, PG, Kann, DA, Lamb, GP, Levan, AJ, Martin-Carrillo, A, Moller, 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 GRB190114C', Astronomy & Astrophysics, vol. 659, 39. https://doi.org/10.1051/0004-6361/202141788

APA

Melandri, A., Izzo, L., Pian, E., Malesani, D. B., Della Valle, M., Rossi, A., D'Avanzo, 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 GRB190114C. Astronomy & Astrophysics, 659, [39]. https://doi.org/10.1051/0004-6361/202141788

Vancouver

Melandri A, Izzo L, Pian E, Malesani DB, Della Valle M, Rossi A et al. The supernova of the MAGIC gamma-ray burst GRB190114C. Astronomy & Astrophysics. 2022 Mar 1;659. 39. https://doi.org/10.1051/0004-6361/202141788

Author

Melandri, A. ; Izzo, L. ; Pian, E. ; Malesani, D. B. ; Della Valle, M. ; Rossi, A. ; D'Avanzo, 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. ; Covino, S. ; D'Elia, Valerio ; de Ugarte Postigo, A. ; De Pasquale, M. ; Filippenko, A. ; Fruchter, A. S. ; Fynbo, J. P. U. ; Giunta, A. ; Hartmann, D. H. ; Jakobsson, P. ; Japelj, J. ; Jonker, P. G. ; Kann, D. A. ; Lamb, G. P. ; Levan, A. J. ; Martin-Carrillo, A. ; Moller, P. ; Piranomonte, S. ; Pugliese, G. ; Salvaterra, R. ; Schulze, S. ; Starling, R. L. C. ; Stella, L. ; Tagliaferri, G. ; Tanvir, N. ; Watson, D. / The supernova of the MAGIC gamma-ray burst GRB190114C. In: Astronomy & Astrophysics. 2022 ; Vol. 659.

Bibtex

@article{b481e3f0ae6b41fa97d89719b3b62bf1,

title = "The supernova of the MAGIC gamma-ray burst GRB190114C",

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, GRB, LIGHT, FERMI, TELESCOPE, DIVERSITY, SPECTRUM, STAR, JET",

author = "A. Melandri and L. Izzo and E. Pian and Malesani, {D. B.} and {Della Valle}, M. and A. Rossi and P. D'Avanzo 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 Valerio D'Elia and {de Ugarte Postigo}, A. and {De Pasquale}, M. and A. Filippenko 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. Moller 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",

year = "2022",

month = mar,

day = "1",

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

language = "English",

volume = "659",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - The supernova of the MAGIC gamma-ray burst GRB190114C

AU - Melandri, A.

AU - Izzo, L.

AU - Pian, E.

AU - Malesani, D. B.

AU - Della Valle, M.

AU - Rossi, A.

AU - D'Avanzo, 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 - D'Elia, Valerio

AU - de Ugarte Postigo, A.

AU - De Pasquale, M.

AU - Filippenko, A.

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 - Moller, 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.

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

KW - GRB

KW - LIGHT

KW - FERMI

KW - TELESCOPE

KW - DIVERSITY

KW - SPECTRUM

KW - STAR

KW - JET

U2 - 10.1051/0004-6361/202141788

DO - 10.1051/0004-6361/202141788

M3 - Journal article

VL - 659

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - 39

ER -

ID: 302553735