The Young and Bright Type Ia Supernova ASASSN-14lp: Discovery, Early-Time Observations, First-Light Time, Distance to NGC 4666, and Progenitor Constraints
B. J. Shappee, A. L. Piro, T. W.-S. Holoien, J. L. Prieto, C., Contreras, K. Itagaki, C. R. Burns, C. S. Kochanek, K. Z. Stanek, E. Alper,, U. Basu, J. F. Beacom, D. Bersier, J. Brimacombe, E. Conseil, A. B. Danilet,, Subo Dong, E. Falco, D. Grupe, E. Y. Hsiao, S. Kiyota

TL;DR
This paper reports the discovery and detailed early observations of the bright Type Ia supernova ASASSN-14lp, providing insights into its light curve, distance, and progenitor system constraints.
Contribution
It presents the earliest detection of ASASSN-14lp, detailed multi-wavelength data, and progenitor constraints, enhancing understanding of Type Ia supernovae and their origins.
Findings
Early detection less than a day after first light
Distance to host galaxy NGC 4666 estimated at 14.7 Mpc
Progenitor constraints exclude red giant secondaries larger than 0.34 solar radii
Abstract
On 2014 Dec. 9.61, the All-Sky Automated Survey for SuperNovae (ASAS-SN or "Assassin") discovered ASASSN-14lp just days after first light using a global array of 14-cm diameter telescopes. ASASSN-14lp went on to become a bright supernova ( mag), second only to SN 2014J for the year. We present prediscovery photometry (with a detection less than a day after first light) and ultraviolet through near-infrared photometric and spectroscopic data covering the rise and fall of ASASSN-14lp for more than 100 days. We find that ASASSN-14lp had a broad light curve (), a -band maximum at , a rise time of days, and moderate host--galaxy extinction (). Using ASASSN-14lp we derive a distance modulus for NGC 4666 of corresponding to a…
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