A more general model for the intrinsic scatter in type Ia supernova distance moduli

John Marriner, J. P. Bernstein, Richard Kessler, Hubert Lampeitl, Ramon Miquel, Jennifer Mosher, Robert C. Nichol, Masao Sako, Donald P. Schneider, Mathew Smith

Research output: Contribution to journalArticle

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Abstract

We describe a new formalism to fit the parameters α and β that are used in the SALT2 model to determine the standard magnitudes of Type Ia supernovae (SNe Ia). The new formalism describes the intrinsic scatter in SNe Ia by a covariance matrix in place of the single parameter normally used. We have applied this formalism to the Sloan Digital Sky Survey Supernova Survey (SDSS-II) data and conclude that the data are best described by α = 0.135+.033 -.017 and β = 3.19+0.14 - 0.24, where the error is dominated by the uncertainty in the form of the intrinsic scatter matrix. Our result depends on the introduction of a more general form for the intrinsic scatter of the distance moduli of SNe Ia than is conventional, resulting in a larger value of β and a larger uncertainty than the conventional approach. Although this analysis results in a larger value of β and a larger error, the SDSS data differ (at a 98% confidence level) from β = 4.1, the value expected for extinction by the type of dust found in the Milky Way. We have modeled the distribution of SNe Ia in terms of their color and conclude that there is strong evidence that variation in color is a significant contributor to the scatter of SNe Ia around their standard candle magnitude.

Original languageEnglish (US)
Article number72
JournalAstrophysical Journal
Volume740
Issue number2
DOIs
StatePublished - Oct 20 2011

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supernovae
formalism
color
matrix
confidence
extinction
dust
matrices
parameter
distribution
analysis

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Marriner, J., Bernstein, J. P., Kessler, R., Lampeitl, H., Miquel, R., Mosher, J., ... Smith, M. (2011). A more general model for the intrinsic scatter in type Ia supernova distance moduli. Astrophysical Journal, 740(2), [72]. https://doi.org/10.1088/0004-637X/740/2/72
Marriner, John ; Bernstein, J. P. ; Kessler, Richard ; Lampeitl, Hubert ; Miquel, Ramon ; Mosher, Jennifer ; Nichol, Robert C. ; Sako, Masao ; Schneider, Donald P. ; Smith, Mathew. / A more general model for the intrinsic scatter in type Ia supernova distance moduli. In: Astrophysical Journal. 2011 ; Vol. 740, No. 2.
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Marriner, J, Bernstein, JP, Kessler, R, Lampeitl, H, Miquel, R, Mosher, J, Nichol, RC, Sako, M, Schneider, DP & Smith, M 2011, 'A more general model for the intrinsic scatter in type Ia supernova distance moduli', Astrophysical Journal, vol. 740, no. 2, 72. https://doi.org/10.1088/0004-637X/740/2/72

A more general model for the intrinsic scatter in type Ia supernova distance moduli. / Marriner, John; Bernstein, J. P.; Kessler, Richard; Lampeitl, Hubert; Miquel, Ramon; Mosher, Jennifer; Nichol, Robert C.; Sako, Masao; Schneider, Donald P.; Smith, Mathew.

In: Astrophysical Journal, Vol. 740, No. 2, 72, 20.10.2011.

Research output: Contribution to journalArticle

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AU - Mosher, Jennifer

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AU - Sako, Masao

AU - Schneider, Donald P.

AU - Smith, Mathew

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AB - We describe a new formalism to fit the parameters α and β that are used in the SALT2 model to determine the standard magnitudes of Type Ia supernovae (SNe Ia). The new formalism describes the intrinsic scatter in SNe Ia by a covariance matrix in place of the single parameter normally used. We have applied this formalism to the Sloan Digital Sky Survey Supernova Survey (SDSS-II) data and conclude that the data are best described by α = 0.135+.033 -.017 and β = 3.19+0.14 - 0.24, where the error is dominated by the uncertainty in the form of the intrinsic scatter matrix. Our result depends on the introduction of a more general form for the intrinsic scatter of the distance moduli of SNe Ia than is conventional, resulting in a larger value of β and a larger uncertainty than the conventional approach. Although this analysis results in a larger value of β and a larger error, the SDSS data differ (at a 98% confidence level) from β = 4.1, the value expected for extinction by the type of dust found in the Milky Way. We have modeled the distribution of SNe Ia in terms of their color and conclude that there is strong evidence that variation in color is a significant contributor to the scatter of SNe Ia around their standard candle magnitude.

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Marriner J, Bernstein JP, Kessler R, Lampeitl H, Miquel R, Mosher J et al. A more general model for the intrinsic scatter in type Ia supernova distance moduli. Astrophysical Journal. 2011 Oct 20;740(2). 72. https://doi.org/10.1088/0004-637X/740/2/72