Constraining Type Ia supernova explosions and early flux excesses with the Zwicky Transient Factory

Constraining Type Ia supernova explosions and early flux excesses with the Zwicky Transient Factory

In the new era of time-domain surveys, Type Ia supernovae are being caught sooner after explosion, which has exposed significant variation in their early light curves. Two driving factors for early-time evolution are the distribution of 56Ni in the ejecta and the presence of flux excesses of various...

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Bibliographic Details
Main Authors: Bellm, E.C (Author), Coughlin, M. (Author), Deckers, M. (Author), Dimitriadis, G. (Author), Goobar, A. (Author), Graham, M. (Author), Kasliwal, M. (Author), Laher, R.R (Author), Magee, M.R (Author), Maguire, K. (Author), Miller, A.A (Author), Nordin, J. (Author), Rigault, M. (Author), Sainz De Murieta, A. (Author), Shupe, D.L (Author), Smith, M. (Author), Walters, R. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Curve fitting
Detection efficiency
Driving factors
Efficiency
Explosion energy
Explosion models
Explosions
Intrinsic rates
Light curves
Supernovae
Supernovae explosions
supernovae: general
Supernovae: general
surveys
Surveys
Time domain
Time evolutions
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