THE DETECTION RATE of EARLY UV EMISSION from SUPERNOVAE: A DEDICATED GALEX/PTF SURVEY and CALIBRATED THEORETICAL ESTIMATES

Autor: S. Ben-Ami, Joshua S. Bloom, Udi Nakar, D. Christopher Martin, Noam Ganot, Peter Nugent, Dovi Poznanski, Iair Arcavi, Tom A. Barlow, Doron Chelouche, Suvi Gezari, Shrinivas R. Kulkarni, Avishay Gal-Yam, Stephen E. Rafter, Mansi M. Kasliwal, Ari Laor, Ehud Behar, James D. Neill, Benny Trakhtenbrot, Ilan Sagiv, Eran O. Ofek, Mark Sullivan, Dan Maoz, Ofer Lapid, Eli Waxman

Publikováno v: Ganot, N; Gal-Yam, A; Ofek, EO; Sagiv, I; Waxman, E; Lapid, O; et al.(2016). THE DETECTION RATE of EARLY UV EMISSION from SUPERNOVAE: A DEDICATED GALEX/PTF SURVEY and CALIBRATED THEORETICAL ESTIMATES. Astrophysical Journal, 820(1). doi: 10.3847/0004-637X/820/1/57. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/2z42g1xw
Astrophysical Journal, vol 820, iss 1
The Astrophysical Journal, vol 820, iss 1

The radius and surface composition of an exploding massive star,as well as the explosion energy per unit mass, can be measured using early UV observations of core collapse supernovae (SNe). We present the first results from a simultaneous GALEX/PTF s

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http://www.escholarship.org/uc/item/2z42g1xw