The core collapse supernova rate from the SDSS-II supernova survey

Matt Taylor; David Cinabro; Ben Dilday; Lluis Galbany; Ravi R. Gupta; R. Kessler; John Marriner; Robert C. Nichol; Michael Richmond; Donald P. Schneider; Jesper Sollerman

doi:10.1088/0004-637X/792/2/135

The core collapse supernova rate from the SDSS-II supernova survey

Matt Taylor
, David Cinabro
, Ben Dilday
, Lluis Galbany
, Ravi R. Gupta
, R. Kessler
, John Marriner
, Robert C. Nichol
, Michael Richmond
, Donald P. Schneider
, Jesper Sollerman

Research output: Contribution to journal › Article › peer-review

78 Scopus citations

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)
Article number	135
Journal	Astrophysical Journal
Volume	792
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/792/2/135
State	Published - Sep 10 2014

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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title = "The core collapse supernova rate from the SDSS-II supernova survey",

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.",

author = "Matt Taylor and David Cinabro and Ben Dilday and Lluis Galbany and Gupta, \{Ravi R.\} and R. Kessler and John Marriner and Nichol, \{Robert C.\} and Michael Richmond and Schneider, \{Donald P.\} and Jesper Sollerman",

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doi = "10.1088/0004-637X/792/2/135",

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T1 - The core collapse supernova rate from the SDSS-II supernova survey

AU - Taylor, Matt

AU - Cinabro, David

AU - Dilday, Ben

AU - Galbany, Lluis

AU - Gupta, Ravi R.

AU - Kessler, R.

AU - Marriner, John

AU - Nichol, Robert C.

AU - Richmond, Michael

AU - Schneider, Donald P.

AU - Sollerman, Jesper

PY - 2014/9/10

Y1 - 2014/9/10

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/84906731907

UR - https://www.scopus.com/pages/publications/84906731907#tab=citedBy

U2 - 10.1088/0004-637X/792/2/135

DO - 10.1088/0004-637X/792/2/135

M3 - Article

AN - SCOPUS:84906731907

SN - 0004-637X

VL - 792

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 135

ER -

The core collapse supernova rate from the SDSS-II supernova survey

Abstract

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