Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared

Details Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared Type Ia Supernova Light Curve Inference: Hierarchical Models in the Optical and Near Infrared

2010-11-26

arxiv.org/abs/1011.5910v3

Astrophys.J.731:120,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

trivial edits to match published version

Scientific paper

10.1088/0004-637X/731/2/120

We have constructed a comprehensive statistical model for Type Ia supernova (SN Ia) light curves spanning optical through near infrared (NIR) data. A hierarchical framework coherently models multiple random and uncertain effects, including intrinsic supernova light curve covariances, dust extinction and reddening, and distances. An improved BayeSN MCMC code computes probabilistic inferences for the hierarchical model by sampling the global probability density of parameters describing individual supernovae and the population. We have applied this hierarchical model to optical and NIR data of 127 SN Ia from PAIRITEL, CfA3, CSP, and the literature. We find an apparent population correlation between the host galaxy extinction A_V and the the ratio of total-to-selective dust absorption R_V. For SN with low dust extinction, A_V < 0.4, we find R_V = 2.5 - 2.9, while at high extinctions, A_V > 1, low values of R_V < 2 are favored. The NIR luminosities are excellent standard candles and are less sensitive to dust extinction. They exhibit low correlation with optical peak luminosities, and thus provide independent information on distances. The combination of NIR and optical data constrains the dust extinction and improves the predictive precision of individual SN Ia distances by about 60%. Using cross-validation, we estimate an rms distance modulus prediction error of 0.11 mag for SN with optical and NIR data versus 0.15 mag for SN with optical data alone. Continued study of SN Ia in the NIR is important for improving their utility as precise and accurate cosmological distance indicators.

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