ZTF early observations of Type Ia supernovae. II. First light, the initial rise, and time to reach maximum brightness. (2020)
Keywords :
Type Ia supernovae ; Surveys ; Catalogs ; Observational astronomy ; Supernovae
Abstract:While it is clear that Type Ia supernovae (SNe) are the result of thermonuclear explosions in C/O white dwarfs (WDs), a great deal remains uncertain about the binary companion that facilitates the explosive disruption of the WD. Here, we present a comprehensive analysis of a large, unique data set of 127 SNe Ia with exquisite coverage by the Zwicky Transient Facility (ZTF). High-cadence (six observations per night) ZTF observations allow us to measure the SN rise time and examine its initial evolution. We develop a Bayesian framework to model the early rise as a power law in time, which enables the inclusion of priors in our model. For a volume-limited subset of normal SNe Ia, we find that the mean power-law index is
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In this paper, we have presented an analysis of the initial evolution
and rise times of 127 ZTF-discovered SNe Ia with early observations;
see Paper I (Yao+ 2019, J/ApJ/886/152) for details on how the sample
was selected. These SNe were observed as part of the ZTF high-cadence
extragalactic experiment, which obtained three g_ZTF_ and three r_ZTF_
observations every night the telescope was open.
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