Near-Infrared Properties of Type Ia Supernovae
M. M. Phillips
+ Author Affiliations
- Author Affiliations
Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena, Chile. Email: mmp@lco.cl
Publications of the Astronomical Society of Australia 29(4) 434-446 https://doi.org/10.1071/AS11056
Submitted: 30 September 2011 Accepted: 15 November 2012 Published: 28 February 2012
Journal Compilation © Astronomical Society of Australia 2012
Abstract
The photometric properties of Type Ia supernovae (SNe Ia) in the near-infrared as garnered from observations made over the last 30 years are reviewed. During this period, light curves for more than 120 nearby SNe Ia have been published, revealing considerable homogeneity but also some fascinating differences. These data have confirmed that, for all but the fastest declining objects, SNe Ia are essentially perfect standard candles in the near-infrared, displaying only a slight dependence of peak luminosity on decline rate and color.
Keywords: supernovae: general — cosmology: observations
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