Benchmarking a Light-Curve Model at Low-z

Details Benchmarking a Light-Curve Model at Low-z Benchmarking a Light-Curve Model at Low-z

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.294..241m&link_type=abstract

Astrophysics and Space Science, Volume 294, Issue 3-4, pp. 241-253

Astronomy and Astrophysics

Astrophysics

Type Ia Supernovae, Light-Curves

Scientific paper

A set of well-measured, {low-z}, type Ia supernovae from the Calán/Tololo SNe data sets is used to determine benchmark parameters in our hydrodynamics-based, light-curve model. The light-curve data fit fairly well in B, V, and R passbands but not as well in the I passband. The fitting procedure, extracted best-fit model parameters, and their connection to type Ia SN parameters are presented. Our benchmarked light-curve model represents an alternative to empirical template methods for the analysis of light-curve data.

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