Abstract
We use the Sloan Digital Sky Survey II Supernova Survey (SDSS-II SNS) data to measure the volumetric core collapse supernova (CCSN) rate in the redshift range (0.03 < z < 0.09). Using a sample of 89 CCSN, we find a volume-averaged rate of 1.06 ± 0.19 × 10-4((h/0.7) 3/(yr Mpc3)) at a mean redshift of 0.072 ± 0.009. We measure the CCSN luminosity function from the data and consider the implications on the star formation history.
Original language | English (US) |
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Article number | 135 |
Journal | Astrophysical Journal |
Volume | 792 |
Issue number | 2 |
DOIs | |
State | Published - Sep 10 2014 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science