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Limit on Supernova Emission in the Brightest Gamma-Ray Burst, GRB 221009A

Title: Limit on Supernova Emission in the Brightest Gamma-Ray Burst, GRB 221009A
Authors: Shrestha, M; Sand, DJ; Alexander, KD; Bostroem, KA; Hosseinzadeh, G; Pearson, J; Aghakhanloo, M; Vinkó, J; Andrews, JE; Jencson, JE; Lundquist, MJ; Wyatt, S; Howell, DA; McCully, C; Gonzalez, EP; Pellegrino, C; Terreran, G; Hiramatsu, D; Newsome, M; Farah, J; Jha, SW; Smith, N; Wheeler, JC; Martínez-Vázquez, C; Carballo-Bello, JA; Drlica-Wagner, A; James, DJ; Mutlu-Pakdil, B; Stringfellow, GS; Sakowska, JD; Noël, NED; Bom, CR; Kuehn, K
Publisher Information: American Astronomical Society
Publication Year: 2023
Collection: Liverpool John Moores University: LJMU Research Online
Subject Terms: QB Astronomy; QC Physics
Description: We present photometric and spectroscopic observations of the extraordinary gamma-ray burst (GRB) 221009A in search of an associated supernova. Some past GRBs have shown bumps in the optical light curve that coincide with the emergence of supernova spectral features, but we do not detect any significant light-curve features in GRB 221009A, nor do we detect any clear sign of supernova spectral features. Using two well-studied GRB-associated supernovae (SN 2013dx, M r , max = − 19.54 ; SN 2016jca, M r , max = − 19.04 ) at a similar redshift as GRB 221009A (z = 0.151), we modeled how the emergence of a supernova would affect the light curve. If we assume the GRB afterglow to decay at the same rate as the X-ray data, the combination of afterglow and a supernova component is fainter than the observed GRB brightness. For the case where we assume the best-fit power law to the optical data as the GRB afterglow component, a supernova contribution should have created a clear bump in the light curve, assuming only extinction from the Milky Way. If we assume a higher extinction of E(B − V) = 1.74 mag (as has been suggested elsewhere), the supernova contribution would have been hard to detect, with a limit on the associated supernova of M r , max ≈ − 19.54. We do not observe any clear supernova features in our spectra, which were taken around the time of expected maximum light. The lack of a bright supernova associated with GRB 221009A may indicate that the energy from the explosion is mostly concentrated in the jet, leaving a lower energy budget available for the supernova.
Document Type: article in journal/newspaper
File Description: text
Language: English
ISSN: 2041-8205
Relation: https://researchonline.ljmu.ac.uk/id/eprint/19842/1/Limit%20on%20Supernova%20Emission%20in%20the%20Brightest%20Gamma-Ray%20Burst,%20GRB%20221009A.pdf; Shrestha, M ORCID logoorcid:0000-0002-4022-1874 , Sand, DJ ORCID logoorcid:0000-0003-4102-380X , Alexander, KD ORCID logoorcid:0000-0002-8297-2473 , Bostroem, KA ORCID logoorcid:0000-0002-4924-444X , Hosseinzadeh, G ORCID logoorcid:0000-0002-0832-2974 , Pearson, J ORCID logoorcid:0000-0002-0744-0047 , Aghakhanloo, M ORCID logoorcid:0000-0001-8341-3940 , Vinkó, J ORCID logoorcid:0000-0001-8764-7832 , Andrews, JE ORCID logoorcid:0000-0003-0123-0062 , Jencson, JE ORCID logoorcid:0000-0001-5754-4007 , Lundquist, MJ ORCID logoorcid:0000-0001-9589-3793 , Wyatt, S ORCID logoorcid:0000-0003-2732-4956 , Howell, DA ORCID logoorcid:0000-0003-4253-656X , McCully, C ORCID logoorcid:0000-0001-5807-7893 , Gonzalez, EP ORCID logoorcid:0000-0003-0209-9246 , Pellegrino, C ORCID logoorcid:0000-0002-7472-1279 , Terreran, G ORCID logoorcid:0000-0003-0794-5982 , Hiramatsu, D ORCID logoorcid:0000-0002-1125-9187 , Newsome, M, Farah, J ORCID logoorcid:0000-0003-4914-5625 , Jha, SW ORCID logoorcid:0000-0001-8738-6011 , Smith, N ORCID logoorcid:0000-0001-5510-2424 , Wheeler, JC ORCID logoorcid:0000-0003-1349-6538 , Martínez-Vázquez, C ORCID logoorcid:0000-0002-9144-7726 , Carballo-Bello, JA ORCID logoorcid:0000-0002-3690-105X , Drlica-Wagner, A ORCID logoorcid:0000-0001-8251-933X , James, DJ ORCID logoorcid:0000-0001-5160-4486 , Mutlu-Pakdil, B ORCID logoorcid:0000-0001-9649-4815 , Stringfellow, GS ORCID logoorcid:0000-0003-1479-3059 , Sakowska, JD ORCID logoorcid:0000-0002-1594-1466 , Noël, NED ORCID logoorcid:0000-0002-8282-469X , Bom, CR ORCID logoorcid:0000-0003-4383-2969 and Kuehn, K ORCID logoorcid:0000-0003-0120-0808 (2023) Limit on Supernova Emission in the Brightest Gamma-Ray Burst, GRB 221009A. Astrophysical Journal Letters, 946 (1). ISSN 2041-8205
DOI: 10.3847/2041-8213/acbd50
Availability: https://researchonline.ljmu.ac.uk/id/eprint/19842/; https://doi.org/10.3847/2041-8213/acbd50
Rights: cc_by
Accession Number: edsbas.BA9613B5
Database: BASE