Multi-band analyses of the bright GRB 230812B and the associated SN2023pel

T. Hussenot-Desenonges; T. Wouters; N. Guessoum; I. Abdi; A. Abulwfa; C. Adami; J. F. Agüí Fernández; T. Ahumada; V. Aivazyan; D. Akl; S. Anand; C. M. Andrade; S. Antier; S. A. Ata; P. D'Avanzo; Y. A. Azzam; A. Baransky; S. Basa; M. Blazek; P. Bendjoya; S. Beradze; P. Boumis; M. Bremer; R. Brivio; V. Buat; M. Bulla; O. Burkhonov; E. Burns; S. B. Cenko; W. Corradi; M. W. Coughlin; F. Daigne; T. Dietrich; D. Dornic; J. -G. Ducoin; P. -A. Duverne; E. G. Elhosseiny; F. I. Elnagahy; M. A. El-Sadek; M. Ferro; E. Le Floc'h; M. Freeberg; J. P. U. Fynbo; D. Götz; E. Gurbanov; G. M. Hamed; E. Hasanov; B. F. Healy; K. E. Heintz; P. Hello; R. Inasaridze; A. Iskandar; N. Ismailov; L. Izzo; S. Jhawar; T. Jegou du Laz; T. M. Kamel; S. Karpov; A. Klotz; E. Koulouridis; N. P. Kuin; N. Kochiashvili; S. Leonini; K. -X. Lu; D. B. Malesani; M. Masek; J. Mao; A. Melandri; B. M. Mihov; R. Natsvlishvili; F. Navarete; V. Nedora; J. Nicolas; M. Odeh; J. Palmerio; P. T. H. Pang; M. De Pasquale; H. W. Peng; S. Pormente; J. Peloton; T. Pradier; O. Pyshna; Y. Rajabov; N. A. Rakotondrainibe; J. -P. Rivet; L. Rousselot; A. Saccardi; N. Sasaki; B. Schneider; M. Serrau; A. Shokry; L. Slavcheva-Mihova; A. Simon; O. Sokoliuk; G. Srinivasaragavan; R. Strausbaugh; N. R. Tanvir; A. Takey; C. C. Thöne; Y. Tillayev; I. Tosta e Melo; D. Turpin; A. de Ugarte Postigo; V. Vasylenko; S. D. Vergani; Z. Vidadi; D. Xu; L. T. Wang; X. F. Wang; J. M. Winters; X -L. Zhang; Z. Zhu

Multi-band analyses of the bright GRB 230812B and the associated SN2023pel

T. Hussenot-Desenonges, T. Wouters, N. Guessoum, I. Abdi, A. Abulwfa, C. Adami, J. F. Agüí Fernández, T. Ahumada, V. Aivazyan, D. Akl, S. Anand, C. M. Andrade, S. Antier, S. A. Ata, P. D'Avanzo, Y. A. Azzam, A. Baransky, S. Basa, M. Blazek, P. BendjoyaS. Beradze, P. Boumis, M. Bremer, R. Brivio, V. Buat, M. Bulla, O. Burkhonov, E. Burns, S. B. Cenko, W. Corradi, M. W. Coughlin, F. Daigne, T. Dietrich, D. Dornic, J. -G. Ducoin, P. -A. Duverne, E. G. Elhosseiny, F. I. Elnagahy, M. A. El-Sadek, M. Ferro, E. Le Floc'h, M. Freeberg, J. P. U. Fynbo, D. Götz, E. Gurbanov, G. M. Hamed, E. Hasanov, B. F. Healy, K. E. Heintz, P. Hello, R. Inasaridze, A. Iskandar, N. Ismailov, L. Izzo, S. Jhawar, T. Jegou du Laz, T. M. Kamel, S. Karpov, A. Klotz, E. Koulouridis, N. P. Kuin, N. Kochiashvili, S. Leonini, K. -X. Lu, D. B. Malesani, M. Masek, J. Mao, A. Melandri, B. M. Mihov, R. Natsvlishvili, F. Navarete, V. Nedora, J. Nicolas, M. Odeh, J. Palmerio, P. T. H. Pang, M. De Pasquale, H. W. Peng, S. Pormente, J. Peloton, T. Pradier, O. Pyshna, Y. Rajabov, N. A. Rakotondrainibe, J. -P. Rivet, L. Rousselot, A. Saccardi, N. Sasaki, B. Schneider, M. Serrau, A. Shokry, L. Slavcheva-Mihova, A. Simon, O. Sokoliuk, G. Srinivasaragavan, R. Strausbaugh, N. R. Tanvir, A. Takey, C. C. Thöne, Y. Tillayev, I. Tosta e Melo, D. Turpin, A. de Ugarte Postigo, V. Vasylenko, S. D. Vergani, Z. Vidadi, D. Xu, L. T. Wang, X. F. Wang, J. M. Winters, X -L. Zhang, Z. Zhu

Physics

Research output: Working paper › Preprint

Abstract

GRB~230812B is a bright and relatively nearby ($z =0.36$) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray, ultraviolet, optical, infrared, and sub-millimeter bands from the GRANDMA (Global Rapid Advanced Network for Multi-messenger Addicts) network of observatories and from observational partners. Adding complementary data from the literature, we then derive essential physical parameters associated with the ejecta and external properties (i.e. the geometry and environment) of the GRB and compare with other analyses of this event. We spectroscopically confirm the presence of an associated supernova, SN2023pel, and we derive a photospheric expansion velocity of v $\sim$ 17$\times10^3$ km s$^{-1}$. We analyze the photometric data first using empirical fits of the flux and then with full Bayesian Inference. We again strongly establish the presence of a supernova in the data, with a maximum (pseudo-)bolometric luminosity of $5.75 \times 10^{42}$ erg/s, at $15.76^{+0.81}_{-1.21}$ days (in the observer frame) after the trigger, with a half-max time width of 22.0 days. We compare these values with those of SN1998bw, SN2006aj, and SN2013dx. Our best-fit model favours a very low density environment ($\log_{10}({n_{\rm ISM}/{\rm cm}^{-3}}) = -2.38^{+1.45}_{-1.60}$) and small values for the jet's core angle $\theta_{\rm core} = 1.54^{+1.02}_{-0.81} \ \rm{deg}$ and viewing angle $\theta_{\rm obs} = 0.76^{+1.29}_{-0.76} \ \rm{deg}$. GRB 230812B is thus one of the best observed afterglows with a distinctive supernova bump.

Original language	Undefined/Unknown
State	Published - Oct 22 2023

Keywords

astro-ph.HE

Access to Document

2310.14310v2

Cite this

Hussenot-Desenonges, T, Wouters, T, Guessoum, N, Abdi, I, Abulwfa, A, Adami, C, Fernández, JFA, Ahumada, T, Aivazyan, V, Akl, D, Anand, S, Andrade, CM, Antier, S, Ata, SA, D'Avanzo, P, Azzam, YA, Baransky, A, Basa, S, Blazek, M, Bendjoya, P, Beradze, S, Boumis, P, Bremer, M, Brivio, R, Buat, V, Bulla, M, Burkhonov, O, Burns, E, Cenko, SB, Corradi, W, Coughlin, MW, Daigne, F, Dietrich, T, Dornic, D, Ducoin, J-G, Duverne, P-A, Elhosseiny, EG, Elnagahy, FI, El-Sadek, MA, Ferro, M, Floc'h, EL, Freeberg, M, Fynbo, JPU, Götz, D, Gurbanov, E, Hamed, GM, Hasanov, E, Healy, BF, Heintz, KE, Hello, P, Inasaridze, R, Iskandar, A, Ismailov, N, Izzo, L, Jhawar, S, Laz, TJD, Kamel, TM, Karpov, S, Klotz, A, Koulouridis, E, Kuin, NP, Kochiashvili, N, Leonini, S, Lu, K-X, Malesani, DB, Masek, M, Mao, J, Melandri, A, Mihov, BM, Natsvlishvili, R, Navarete, F, Nedora, V, Nicolas, J, Odeh, M, Palmerio, J, Pang, PTH, Pasquale, MD, Peng, HW, Pormente, S, Peloton, J, Pradier, T, Pyshna, O, Rajabov, Y, Rakotondrainibe, NA, Rivet, J-P, Rousselot, L, Saccardi, A, Sasaki, N, Schneider, B, Serrau, M, Shokry, A, Slavcheva-Mihova, L, Simon, A, Sokoliuk, O, Srinivasaragavan, G, Strausbaugh, R, Tanvir, NR, Takey, A, Thöne, CC, Tillayev, Y, Melo, ITE, Turpin, D, Postigo, ADU, Vasylenko, V, Vergani, SD, Vidadi, Z, Xu, D, Wang, LT, Wang, XF, Winters, JM, Zhang, X-L & Zhu, Z 2023 'Multi-band analyses of the bright GRB 230812B and the associated SN2023pel'.

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title = "Multi-band analyses of the bright GRB 230812B and the associated SN2023pel",

abstract = "GRB~230812B is a bright and relatively nearby ($z =0.36$) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray, ultraviolet, optical, infrared, and sub-millimeter bands from the GRANDMA (Global Rapid Advanced Network for Multi-messenger Addicts) network of observatories and from observational partners. Adding complementary data from the literature, we then derive essential physical parameters associated with the ejecta and external properties (i.e. the geometry and environment) of the GRB and compare with other analyses of this event. We spectroscopically confirm the presence of an associated supernova, SN2023pel, and we derive a photospheric expansion velocity of v $\sim$ 17$\times10^3$ km s$^{-1}$. We analyze the photometric data first using empirical fits of the flux and then with full Bayesian Inference. We again strongly establish the presence of a supernova in the data, with a maximum (pseudo-)bolometric luminosity of $5.75 \times 10^{42}$ erg/s, at $15.76^{+0.81}_{-1.21}$ days (in the observer frame) after the trigger, with a half-max time width of 22.0 days. We compare these values with those of SN1998bw, SN2006aj, and SN2013dx. Our best-fit model favours a very low density environment ($\log_{10}({n_{\rm ISM}/{\rm cm}^{-3}}) = -2.38^{+1.45}_{-1.60}$) and small values for the jet's core angle $\theta_{\rm core} = 1.54^{+1.02}_{-0.81} \ \rm{deg}$ and viewing angle $\theta_{\rm obs} = 0.76^{+1.29}_{-0.76} \ \rm{deg}$. GRB 230812B is thus one of the best observed afterglows with a distinctive supernova bump.",

keywords = "astro-ph.HE",

author = "T. Hussenot-Desenonges and T. Wouters and N. Guessoum and I. Abdi and A. Abulwfa and C. Adami and Fern{\'a}ndez, {J. F. Ag{\"u}{\'i}} and T. Ahumada and V. Aivazyan and D. Akl and S. Anand and Andrade, {C. M.} and S. Antier and Ata, {S. A.} and P. D'Avanzo and Azzam, {Y. A.} and A. Baransky and S. Basa and M. Blazek and P. Bendjoya and S. Beradze and P. Boumis and M. Bremer and R. Brivio and V. Buat and M. Bulla and O. Burkhonov and E. Burns and Cenko, {S. B.} and W. Corradi and Coughlin, {M. W.} and F. Daigne and T. Dietrich and D. Dornic and Ducoin, {J. -G.} and Duverne, {P. -A.} and Elhosseiny, {E. G.} and Elnagahy, {F. I.} and El-Sadek, {M. A.} and M. Ferro and Floc'h, {E. Le} and M. Freeberg and Fynbo, {J. P. U.} and D. G{\"o}tz and E. Gurbanov and Hamed, {G. M.} and E. Hasanov and Healy, {B. F.} and Heintz, {K. E.} and P. Hello and R. Inasaridze and A. Iskandar and N. Ismailov and L. Izzo and S. Jhawar and Laz, {T. Jegou du} and Kamel, {T. M.} and S. Karpov and A. Klotz and E. Koulouridis and Kuin, {N. P.} and N. Kochiashvili and S. Leonini and Lu, {K. -X.} and Malesani, {D. B.} and M. Masek and J. Mao and A. Melandri and Mihov, {B. M.} and R. Natsvlishvili and F. Navarete and V. Nedora and J. Nicolas and M. Odeh and J. Palmerio and Pang, {P. T. H.} and Pasquale, {M. De} and Peng, {H. W.} and S. Pormente and J. Peloton and T. Pradier and O. Pyshna and Y. Rajabov and Rakotondrainibe, {N. A.} and Rivet, {J. -P.} and L. Rousselot and A. Saccardi and N. Sasaki and B. Schneider and M. Serrau and A. Shokry and L. Slavcheva-Mihova and A. Simon and O. Sokoliuk and G. Srinivasaragavan and R. Strausbaugh and Tanvir, {N. R.} and A. Takey and Th{\"o}ne, {C. C.} and Y. Tillayev and Melo, {I. Tosta e} and D. Turpin and Postigo, {A. de Ugarte} and V. Vasylenko and Vergani, {S. D.} and Z. Vidadi and D. Xu and Wang, {L. T.} and Wang, {X. F.} and Winters, {J. M.} and Zhang, {X -L.} and Z. Zhu",

year = "2023",

month = oct,

day = "22",

language = "Undefined/Unknown",

type = "WorkingPaper",

}

TY - UNPB

T1 - Multi-band analyses of the bright GRB 230812B and the associated SN2023pel

AU - Hussenot-Desenonges, T.

AU - Wouters, T.

AU - Guessoum, N.

AU - Abdi, I.

AU - Abulwfa, A.

AU - Adami, C.

AU - Fernández, J. F. Agüí

AU - Ahumada, T.

AU - Aivazyan, V.

AU - Akl, D.

AU - Anand, S.

AU - Andrade, C. M.

AU - Antier, S.

AU - Ata, S. A.

AU - D'Avanzo, P.

AU - Azzam, Y. A.

AU - Baransky, A.

AU - Basa, S.

AU - Blazek, M.

AU - Bendjoya, P.

AU - Beradze, S.

AU - Boumis, P.

AU - Bremer, M.

AU - Brivio, R.

AU - Buat, V.

AU - Bulla, M.

AU - Burkhonov, O.

AU - Burns, E.

AU - Cenko, S. B.

AU - Corradi, W.

AU - Coughlin, M. W.

AU - Daigne, F.

AU - Dietrich, T.

AU - Dornic, D.

AU - Ducoin, J. -G.

AU - Duverne, P. -A.

AU - Elhosseiny, E. G.

AU - Elnagahy, F. I.

AU - El-Sadek, M. A.

AU - Ferro, M.

AU - Floc'h, E. Le

AU - Freeberg, M.

AU - Fynbo, J. P. U.

AU - Götz, D.

AU - Gurbanov, E.

AU - Hamed, G. M.

AU - Hasanov, E.

AU - Healy, B. F.

AU - Heintz, K. E.

AU - Hello, P.

AU - Inasaridze, R.

AU - Iskandar, A.

AU - Ismailov, N.

AU - Izzo, L.

AU - Jhawar, S.

AU - Laz, T. Jegou du

AU - Kamel, T. M.

AU - Karpov, S.

AU - Klotz, A.

AU - Koulouridis, E.

AU - Kuin, N. P.

AU - Kochiashvili, N.

AU - Leonini, S.

AU - Lu, K. -X.

AU - Malesani, D. B.

AU - Masek, M.

AU - Mao, J.

AU - Melandri, A.

AU - Mihov, B. M.

AU - Natsvlishvili, R.

AU - Navarete, F.

AU - Nedora, V.

AU - Nicolas, J.

AU - Odeh, M.

AU - Palmerio, J.

AU - Pang, P. T. H.

AU - Pasquale, M. De

AU - Peng, H. W.

AU - Pormente, S.

AU - Peloton, J.

AU - Pradier, T.

AU - Pyshna, O.

AU - Rajabov, Y.

AU - Rakotondrainibe, N. A.

AU - Rivet, J. -P.

AU - Rousselot, L.

AU - Saccardi, A.

AU - Sasaki, N.

AU - Schneider, B.

AU - Serrau, M.

AU - Shokry, A.

AU - Slavcheva-Mihova, L.

AU - Simon, A.

AU - Sokoliuk, O.

AU - Srinivasaragavan, G.

AU - Strausbaugh, R.

AU - Tanvir, N. R.

AU - Takey, A.

AU - Thöne, C. C.

AU - Tillayev, Y.

AU - Melo, I. Tosta e

AU - Turpin, D.

AU - Postigo, A. de Ugarte

AU - Vasylenko, V.

AU - Vergani, S. D.

AU - Vidadi, Z.

AU - Xu, D.

AU - Wang, L. T.

AU - Wang, X. F.

AU - Winters, J. M.

AU - Zhang, X -L.

AU - Zhu, Z.

PY - 2023/10/22

Y1 - 2023/10/22

N2 - GRB~230812B is a bright and relatively nearby ($z =0.36$) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray, ultraviolet, optical, infrared, and sub-millimeter bands from the GRANDMA (Global Rapid Advanced Network for Multi-messenger Addicts) network of observatories and from observational partners. Adding complementary data from the literature, we then derive essential physical parameters associated with the ejecta and external properties (i.e. the geometry and environment) of the GRB and compare with other analyses of this event. We spectroscopically confirm the presence of an associated supernova, SN2023pel, and we derive a photospheric expansion velocity of v $\sim$ 17$\times10^3$ km s$^{-1}$. We analyze the photometric data first using empirical fits of the flux and then with full Bayesian Inference. We again strongly establish the presence of a supernova in the data, with a maximum (pseudo-)bolometric luminosity of $5.75 \times 10^{42}$ erg/s, at $15.76^{+0.81}_{-1.21}$ days (in the observer frame) after the trigger, with a half-max time width of 22.0 days. We compare these values with those of SN1998bw, SN2006aj, and SN2013dx. Our best-fit model favours a very low density environment ($\log_{10}({n_{\rm ISM}/{\rm cm}^{-3}}) = -2.38^{+1.45}_{-1.60}$) and small values for the jet's core angle $\theta_{\rm core} = 1.54^{+1.02}_{-0.81} \ \rm{deg}$ and viewing angle $\theta_{\rm obs} = 0.76^{+1.29}_{-0.76} \ \rm{deg}$. GRB 230812B is thus one of the best observed afterglows with a distinctive supernova bump.

AB - GRB~230812B is a bright and relatively nearby ($z =0.36$) long gamma-ray burst (GRB) that has generated significant interest in the community and has thus been observed over the entire electromagnetic spectrum. We report over 80 observations in X-ray, ultraviolet, optical, infrared, and sub-millimeter bands from the GRANDMA (Global Rapid Advanced Network for Multi-messenger Addicts) network of observatories and from observational partners. Adding complementary data from the literature, we then derive essential physical parameters associated with the ejecta and external properties (i.e. the geometry and environment) of the GRB and compare with other analyses of this event. We spectroscopically confirm the presence of an associated supernova, SN2023pel, and we derive a photospheric expansion velocity of v $\sim$ 17$\times10^3$ km s$^{-1}$. We analyze the photometric data first using empirical fits of the flux and then with full Bayesian Inference. We again strongly establish the presence of a supernova in the data, with a maximum (pseudo-)bolometric luminosity of $5.75 \times 10^{42}$ erg/s, at $15.76^{+0.81}_{-1.21}$ days (in the observer frame) after the trigger, with a half-max time width of 22.0 days. We compare these values with those of SN1998bw, SN2006aj, and SN2013dx. Our best-fit model favours a very low density environment ($\log_{10}({n_{\rm ISM}/{\rm cm}^{-3}}) = -2.38^{+1.45}_{-1.60}$) and small values for the jet's core angle $\theta_{\rm core} = 1.54^{+1.02}_{-0.81} \ \rm{deg}$ and viewing angle $\theta_{\rm obs} = 0.76^{+1.29}_{-0.76} \ \rm{deg}$. GRB 230812B is thus one of the best observed afterglows with a distinctive supernova bump.

KW - astro-ph.HE

M3 - Preprint

BT - Multi-band analyses of the bright GRB 230812B and the associated SN2023pel

ER -