The Astrophysical Journal (Jan 2023)

A Systematic Study of Ia-CSM Supernovae from the ZTF Bright Transient Survey

  • Yashvi Sharma,
  • Jesper Sollerman,
  • Christoffer Fremling,
  • Shrinivas R. Kulkarni,
  • Kishalay De,
  • Ido Irani,
  • Steve Schulze,
  • Nora Linn Strotjohann,
  • Avishay Gal-Yam,
  • Kate Maguire,
  • Daniel A. Perley,
  • Eric C. Bellm,
  • Erik C. Kool,
  • Thomas G. Brink,
  • Rachel Bruch,
  • Maxime Deckers,
  • Richard Dekany,
  • Alison Dugas,
  • Alexei V. Filippenko,
  • Samantha Goldwasser,
  • Matthew J. Graham,
  • Melissa L. Graham,
  • Steven L. Groom,
  • Matt Hankins,
  • Jacob Jencson,
  • Joel P. Johansson,
  • Viraj Karambelkar,
  • Mansi M. Kasliwal,
  • Frank J. Masci,
  • Michael S. Medford,
  • James D. Neill,
  • Guy Nir,
  • Reed L. Riddle,
  • Mickael Rigault,
  • Tassilo Schweyer,
  • Jacco H. Terwel,
  • Lin Yan,
  • Yi Yang,
  • Yuhan Yao

DOI
https://doi.org/10.3847/1538-4357/acbc16
Journal volume & issue
Vol. 948, no. 1
p. 52

Abstract

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Among the supernovae (SNe) that show strong interaction with a circumstellar medium (CSM), there is a rare subclass of Type Ia supernovae, SNe Ia-CSM, which show strong narrow hydrogen emission lines much like SNe IIn but on top of a diluted Type Ia spectrum. The only previous systematic study of this class identified 16 SNe Ia-CSM, eight historic and eight from the Palomar Transient Factory (PTF). Now using the successor survey to PTF, the Zwicky Transient Facility (ZTF), we have classified 12 additional SNe Ia-CSM through the systematic Bright Transient Survey (BTS). Consistent with previous studies, we find these SNe to have slowly evolving optical light curves with peak absolute magnitudes between −19.1 and −21, spectra having weak H β and large Balmer decrements of ∼7. Out of the 10 SNe from our sample observed by NEOWISE, nine have 3 σ detections, with some SNe showing a reduction in the red wing of H α , indicative of newly formed dust. We do not find our SN Ia-CSM sample to have a significantly different distribution of equivalent widths of He i λ 5876 than SNe IIn as observed in Silverman et al. The hosts tend to be late-type galaxies with recent star formation. We derive a rate estimate of ${29}_{-21}^{+27}$ Gpc ^−3 yr ^−1 for SNe Ia-CSM, which is ∼0.02%–0.2% of the SN Ia rate. We also identify six ambiguous SNe IIn/Ia-CSM in the BTS sample and including them gives an upper limit rate of 0.07%–0.8%. This work nearly doubles the sample of well-studied Ia-CSM objects in Silverman et al., increasing the total number to 28.

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