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

Institute of Cosmology & Gravitation

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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
Journal	The Astrophysical Journal
Volume	792
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/792/2/135
Publication status	Published - 26 Aug 2014

Keywords

astro-ph.SR
astro-ph.CO

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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.",

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note = "Minor corrections to references and affiliations to conform with published version",

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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

N1 - Minor corrections to references and affiliations to conform with published version

PY - 2014/8/26

Y1 - 2014/8/26

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.

KW - astro-ph.SR

KW - astro-ph.CO

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

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

M3 - Article

SN - 0004-637X

VL - 792

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 2

ER -

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

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Keywords

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