FUZZY SUPERNOVA TEMPLATES. II. PARAMETER ESTIMATION
FUZZY SUPERNOVA TEMPLATES. II. PARAMETER ESTIMATION
Wide field surveys will soon be discovering Type Ia supernovae (SNe) at rates of several thousand per year. Spectroscopic follow-up can only scratch the surface for such enormous samples, so these extensive data sets will only be useful to the extent that they can be characterized by the survey photometry …