ZTF Early Observations of Type Ia Supernovae I: Properties of the 2018 Sample
Yuhan Yao, Adam A. Miller, S. R. Kulkarni, Mattia Bulla, Frank J., Masci, Daniel A. Goldstein, Ariel Goobar, Peter Nugent, Alison Dugas, Nadia, Blagorodnova, James D. Neill, Michael Rigault, Jesper Sollerman, J. Nordin,, Eric C. Bellm, S. Bradley Cenko, Kishalay De

TL;DR
This paper presents high-quality early light curves of 127 Type Ia supernovae discovered by ZTF in 2018, enabling detailed studies of their progenitor properties and early evolution.
Contribution
It introduces a method for forced PSF photometry applicable to extragalactic transients and provides the largest sample of young SNe Ia with early detections, including peculiar events.
Findings
Detected all SNe in both bands more than 10 days before maximum light.
Largest sample of young SNe Ia with early observations to date.
Identified peculiar supernovae, including super-Chandrasekhar candidates.
Abstract
Early-time observations of Type Ia supernovae (SNe Ia) are essential to constrain their progenitor properties. In this paper, we present high-quality light curves of 127 SNe Ia discovered by the Zwicky Transient Facility (ZTF) in 2018. We describe our method to perform forced point spread function (PSF) photometry, which can be applied to other types of extragalactic transients. With a planned cadence of six observations per night (), all of the 127 SNe Ia are detected in both and band more than 10\,d (in the rest frame) prior to the epoch of -band maximum light. The redshifts of these objects range from to 0.165; the median redshift is 0.074. Among the 127 SNe, 50 are detected at least 14\,d prior to maximum light (in the rest frame), with a subset of 9 objects being detected more than 17\,d before -band peak. This is the largest sample of young SNe Ia…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Methane Hydrates and Related Phenomena · Astronomy and Astrophysical Research
