Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST

Abstract We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at z = 2.83. This SN (named SN 2023adta) was identified in deep JWST/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Follow-up observations with JWST/NIRSpec provided a spectroscopic redshift of z = 2.83 and the classification as an SN Ic-BL. The light curve of SN 2023adta matches well with other stripped-envelope SNe, and we find a high peak luminosity, M V = −19.0 ± 0.2 mag, based on the distribution of best-fit SNe. The broad absorption features in its spectrum are consistent with other SNe Ic-BL 1–3 weeks after peak brightness. We measure a Ca ii near-IR triplet expansion velocity of 29,000 ± 2000 km s −1 . The host galaxy of SN 2023adta is irregular, and modeling of its spectral energy distribution indicates a metallicity of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>Z</mml:mi> <mml:mo>=</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>0.35</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.08</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.16</mml:mn> </mml:mrow> </mml:msubsup> <mml:msub> <mml:mrow> <mml:mi>Z</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> </mml:math> . This environment is consistent with the population of low- z SNe Ic-BL that prefer lower metallicities relative to other stripped-envelope SNe and track long-duration γ -ray burst environments. We do not identify any γ -ray bursts that are coincident with SN 2023adta. Given the rarity of SNe Ic-BL in the local Universe, the detection of an SN Ic-BL at z = 2.83 could indicate that their rates are enhanced at high redshift.

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Journal
The Astrophysical Journal Letters
Published
2024-08-26
DOI
https://doi.org/10.3847/2041-8213/ad6c32
Citations
10
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
3.32

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article

Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST

Qinan Wang, T. Wevers, Eiichi Egami, Bhavin Joshi et al.
10 citations
The Astrophysical Journal Letters
Gamma-ray bursts and supernovae
3.32
article

Discovery of a Relativistic Stripped-envelope Type Ic-BL Supernova at z = 2.83 with JWST

Qinan Wang, T. Wevers, Eiichi Egami, Bhavin Joshi, Muryel Guolo, Mitchell Karmen, Fengwu Sun, R. Maiolino, Benjamin D. Johnson, Takashi J. Moriya, A. Rest, Matthew R. Siebert, Michael Engesser, Louis-Gregory Strolger, Mirko Curti, Yossef Zenati, R. Quimby, Ori D. Fox, Christa DeCoursey, Daniel J. Eisenstein, D. A. Coulter, Andrew J. Bunker, Phillip A. Cargile, Melissa Shahbandeh, Brant E. Robertson, Sebastián Gómez, Suvi Gezari, Justin D. R. Pierel, Wenlei Chen
article en
10 citations

Abstract

Abstract We present James Webb Space Telescope (JWST) NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at z = 2.83. This SN (named SN 2023adta) was identified in deep JWST/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Follow-up observations with JWST/NIRSpec provided a spectroscopic redshift of z = 2.83 and the classification as an SN Ic-BL. The light curve of SN 2023adta matches well with other stripped-envelope SNe, and we find a high peak luminosity, M V = −19.0 ± 0.2 mag, based on the distribution of best-fit SNe. The broad absorption features in its spectrum are consistent with other SNe Ic-BL 1–3 weeks after peak brightness. We measure a Ca ii near-IR triplet expansion velocity of 29,000 ± 2000 km s −1 . The host galaxy of SN 2023adta is irregular, and modeling of its spectral energy distribution indicates a metallicity of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>Z</mml:mi> <mml:mo>=</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>0.35</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>0.08</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>0.16</mml:mn> </mml:mrow> </mml:msubsup> <mml:msub> <mml:mrow> <mml:mi>Z</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> </mml:math> . This environment is consistent with the population of low- z SNe Ic-BL that prefer lower metallicities relative to other stripped-envelope SNe and track long-duration γ -ray burst environments. We do not identify any γ -ray bursts that are coincident with SN 2023adta. Given the rarity of SNe Ic-BL in the local Universe, the detection of an SN Ic-BL at z = 2.83 could indicate that their rates are enhanced at high redshift.

The Astrophysical Journal LettersVol. 972(1)
Oklahoma State University (US), Space Telescope Science Institute (US), European Southern Observatory (DE), University of Arizona (US), Johns Hopkins University (US), Kavli Institute for the Physics and Mathematics of the Universe (JP), University of California, Santa Cruz (US), National Institutes of Natural Sciences (JP), The Graduate University for Advanced Studies, SOKENDAI (JP), University of Cambridge (GB), San Diego State University (US), University of Oxford (GB), Center for Astrophysics Harvard & Smithsonian (US), National Astronomical Observatory of Japan (JP), University College London (GB), Monash University (AU), The University of Tokyo (JP)
National Science Foundation, National Aeronautics and Space Administration, University of California, Santa Cruz, Space Telescope Science Institute, UK Research and Innovation, European Commission, Science and Technology Facilities Council
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Openalex Percentile: Top 8%
Gamma-ray bursts and supernovae
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