Details

Autor(en) / Beteiligte

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

Titel

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

Ist Teil von

• The Astrophysical journal, 2023-05, Vol.948 (1), p.52

Ort / Verlag

Philadelphia: The American Astronomical Society

Erscheinungsjahr

2023

Quelle

Electronic Journals Library

Beschreibungen/Notizen

• Abstract 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.