Optical and Infrared Photometry of the Nearby SN 2017cbv
arXiv:1806.08794 · doi:10.3847/1538-4357/aacd4e
Abstract
On 2017 March 11, the DLT40 Transient Discovery Survey discovered SN 2017cbv in NGC5643, a Type 2 Seyfert Galaxy in the Lupus Constellation. SN 2017cbv went on to become a bright Type Ia supernova, with a of 11.51 0.05 mag. We present early time optical and infrared photometry of SN 2017cbv covering the rise and fall of over 68 days. We find that SN 2017cbv has a broad light curve = 0.88 0.07, a -band maximum at 2457840.97 0.43, a negligible host galaxy reddening where 0, and a distance modulus of 30.49 0.32 to the SN, corresponding to a distance of Mpc. We also present the results of two different numerical models we used for analysis in this paper: SALT2, an empirical model for Type Ia supernova optical light curves that accounts for variability components; and SNooPy, the CSP-II light-curve model that covers both optical and near-infrared wavelengths and is used for distance estimates.
arXiv comment11 pages, 6 figures, 5 tables. Accepted to ApJ
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