The Astrophysical Journal Letters (Jan 2024)

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

  • M. R. Siebert,
  • C. DeCoursey,
  • D. A. Coulter,
  • M. Engesser,
  • J. D. R. Pierel,
  • A. Rest,
  • E. Egami,
  • M. Shahbandeh,
  • W. Chen,
  • O. D. Fox,
  • Y. Zenati,
  • T. J. Moriya,
  • A. J. Bunker,
  • P. A. Cargile,
  • M. Curti,
  • D. J. Eisenstein,
  • S. Gezari,
  • S. Gomez,
  • M. Guolo,
  • B. D. Johnson,
  • B. A. Joshi,
  • M. Karmen,
  • R. Maiolino,
  • R. M. Quimby,
  • B. Robertson,
  • L. G. Strolger,
  • F. Sun,
  • Q. Wang,
  • T. Wevers

DOI
https://doi.org/10.3847/2041-8213/ad6c32
Journal volume & issue
Vol. 972, no. 1
p. L13

Abstract

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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 $Z={0.35}_{-0.08}^{+0.16}{Z}_{\odot }$ . 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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