The SDSS-II Supernova survey: Parameterizing the type ia supernova rate as a function of host galaxy properties

Mathew Smith, Robert C. Nichol, Benjamin Dilday, John Marriner, Richard Kessler, Bruce Bassett, David Cinabro, Joshua Frieman, Peter Garnavich, Saurabh W. Jha, Hubert Lampeitl, Masao Sako, Donald P. Schneider, Jesper Sollerman

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Abstract

Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 < z < 0.25 is constructed. Using broadband photometry and redshifts, we use the PÉGASE.2 spectral energy distributions to estimate host galaxy stellar masses and recent star formation rates (SFRs). We find that the rate of SNe Ia per unit stellar mass is significantly higher (by a factor of 30) in highly star-forming galaxies compared to passive galaxies. When parameterizing the SN Ia rate (SNRIa) based on host galaxy properties, we find that the rate of SNe Ia in passive galaxies is not linearly proportional to the stellar mass; instead an SNRIaM 0.68 is favored. However, such a parameterization does not describe the observed SNRIa in star-forming galaxies. The SNRIa in star-forming galaxies is well fitted by SNRIa = (0.41 ± 0.15) × 10-10 M 0.72 ± 0.15 + (0.65 ± 0.25) × 10 -3SFR1.01 ± 0.22 (statistical errors only), where M is the host galaxy stellar mass (in M ) and SFR is the SFR (in M yr-1). We show that our results, for SNe Ia in passive galaxies, are consistent with those at higher redshifts (favoring SNRIaM) when accounting for the difference in the ages of our galaxies. This suggests that the rate of SNe Ia is correlated with the age of the stellar population. The MLCS extinction parameter, AV , is similar in passive and moderately star-forming galaxies, but we find indications that it is smaller, on average, in highly star-forming galaxies. This result appears to be driven by a deficit of the reddest (AV > 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.

Original languageEnglish (US)
Article number61
JournalAstrophysical Journal
Volume755
Issue number1
DOIs
StatePublished - Aug 10 2012

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supernovae
galaxies
sky
dust
stars
rate

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Smith, M., Nichol, R. C., Dilday, B., Marriner, J., Kessler, R., Bassett, B., ... Sollerman, J. (2012). The SDSS-II Supernova survey: Parameterizing the type ia supernova rate as a function of host galaxy properties. Astrophysical Journal, 755(1), [61]. https://doi.org/10.1088/0004-637X/755/1/61
Smith, Mathew ; Nichol, Robert C. ; Dilday, Benjamin ; Marriner, John ; Kessler, Richard ; Bassett, Bruce ; Cinabro, David ; Frieman, Joshua ; Garnavich, Peter ; Jha, Saurabh W. ; Lampeitl, Hubert ; Sako, Masao ; Schneider, Donald P. ; Sollerman, Jesper. / The SDSS-II Supernova survey : Parameterizing the type ia supernova rate as a function of host galaxy properties. In: Astrophysical Journal. 2012 ; Vol. 755, No. 1.
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abstract = "Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 < z < 0.25 is constructed. Using broadband photometry and redshifts, we use the P{\'E}GASE.2 spectral energy distributions to estimate host galaxy stellar masses and recent star formation rates (SFRs). We find that the rate of SNe Ia per unit stellar mass is significantly higher (by a factor of 30) in highly star-forming galaxies compared to passive galaxies. When parameterizing the SN Ia rate (SNRIa) based on host galaxy properties, we find that the rate of SNe Ia in passive galaxies is not linearly proportional to the stellar mass; instead an SNRIaM 0.68 is favored. However, such a parameterization does not describe the observed SNRIa in star-forming galaxies. The SNRIa in star-forming galaxies is well fitted by SNRIa = (0.41 ± 0.15) × 10-10 M 0.72 ± 0.15 + (0.65 ± 0.25) × 10 -3SFR1.01 ± 0.22 (statistical errors only), where M is the host galaxy stellar mass (in M ⊙) and SFR is the SFR (in M ⊙ yr-1). We show that our results, for SNe Ia in passive galaxies, are consistent with those at higher redshifts (favoring SNRIaM) when accounting for the difference in the ages of our galaxies. This suggests that the rate of SNe Ia is correlated with the age of the stellar population. The MLCS extinction parameter, AV , is similar in passive and moderately star-forming galaxies, but we find indications that it is smaller, on average, in highly star-forming galaxies. This result appears to be driven by a deficit of the reddest (AV > 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.",
author = "Mathew Smith and Nichol, {Robert C.} and Benjamin Dilday and John Marriner and Richard Kessler and Bruce Bassett and David Cinabro and Joshua Frieman and Peter Garnavich and Jha, {Saurabh W.} and Hubert Lampeitl and Masao Sako and Schneider, {Donald P.} and Jesper Sollerman",
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Smith, M, Nichol, RC, Dilday, B, Marriner, J, Kessler, R, Bassett, B, Cinabro, D, Frieman, J, Garnavich, P, Jha, SW, Lampeitl, H, Sako, M, Schneider, DP & Sollerman, J 2012, 'The SDSS-II Supernova survey: Parameterizing the type ia supernova rate as a function of host galaxy properties', Astrophysical Journal, vol. 755, no. 1, 61. https://doi.org/10.1088/0004-637X/755/1/61

The SDSS-II Supernova survey : Parameterizing the type ia supernova rate as a function of host galaxy properties. / Smith, Mathew; Nichol, Robert C.; Dilday, Benjamin; Marriner, John; Kessler, Richard; Bassett, Bruce; Cinabro, David; Frieman, Joshua; Garnavich, Peter; Jha, Saurabh W.; Lampeitl, Hubert; Sako, Masao; Schneider, Donald P.; Sollerman, Jesper.

In: Astrophysical Journal, Vol. 755, No. 1, 61, 10.08.2012.

Research output: Contribution to journalArticle

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T2 - Parameterizing the type ia supernova rate as a function of host galaxy properties

AU - Smith, Mathew

AU - Nichol, Robert C.

AU - Dilday, Benjamin

AU - Marriner, John

AU - Kessler, Richard

AU - Bassett, Bruce

AU - Cinabro, David

AU - Frieman, Joshua

AU - Garnavich, Peter

AU - Jha, Saurabh W.

AU - Lampeitl, Hubert

AU - Sako, Masao

AU - Schneider, Donald P.

AU - Sollerman, Jesper

PY - 2012/8/10

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N2 - Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 < z < 0.25 is constructed. Using broadband photometry and redshifts, we use the PÉGASE.2 spectral energy distributions to estimate host galaxy stellar masses and recent star formation rates (SFRs). We find that the rate of SNe Ia per unit stellar mass is significantly higher (by a factor of 30) in highly star-forming galaxies compared to passive galaxies. When parameterizing the SN Ia rate (SNRIa) based on host galaxy properties, we find that the rate of SNe Ia in passive galaxies is not linearly proportional to the stellar mass; instead an SNRIaM 0.68 is favored. However, such a parameterization does not describe the observed SNRIa in star-forming galaxies. The SNRIa in star-forming galaxies is well fitted by SNRIa = (0.41 ± 0.15) × 10-10 M 0.72 ± 0.15 + (0.65 ± 0.25) × 10 -3SFR1.01 ± 0.22 (statistical errors only), where M is the host galaxy stellar mass (in M ⊙) and SFR is the SFR (in M ⊙ yr-1). We show that our results, for SNe Ia in passive galaxies, are consistent with those at higher redshifts (favoring SNRIaM) when accounting for the difference in the ages of our galaxies. This suggests that the rate of SNe Ia is correlated with the age of the stellar population. The MLCS extinction parameter, AV , is similar in passive and moderately star-forming galaxies, but we find indications that it is smaller, on average, in highly star-forming galaxies. This result appears to be driven by a deficit of the reddest (AV > 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.

AB - Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 < z < 0.25 is constructed. Using broadband photometry and redshifts, we use the PÉGASE.2 spectral energy distributions to estimate host galaxy stellar masses and recent star formation rates (SFRs). We find that the rate of SNe Ia per unit stellar mass is significantly higher (by a factor of 30) in highly star-forming galaxies compared to passive galaxies. When parameterizing the SN Ia rate (SNRIa) based on host galaxy properties, we find that the rate of SNe Ia in passive galaxies is not linearly proportional to the stellar mass; instead an SNRIaM 0.68 is favored. However, such a parameterization does not describe the observed SNRIa in star-forming galaxies. The SNRIa in star-forming galaxies is well fitted by SNRIa = (0.41 ± 0.15) × 10-10 M 0.72 ± 0.15 + (0.65 ± 0.25) × 10 -3SFR1.01 ± 0.22 (statistical errors only), where M is the host galaxy stellar mass (in M ⊙) and SFR is the SFR (in M ⊙ yr-1). We show that our results, for SNe Ia in passive galaxies, are consistent with those at higher redshifts (favoring SNRIaM) when accounting for the difference in the ages of our galaxies. This suggests that the rate of SNe Ia is correlated with the age of the stellar population. The MLCS extinction parameter, AV , is similar in passive and moderately star-forming galaxies, but we find indications that it is smaller, on average, in highly star-forming galaxies. This result appears to be driven by a deficit of the reddest (AV > 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.

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