  The SuperNovae Analysis aPplication (SNAP) is a new tool for the analysis of
SN observations and validation of SN models. SNAP consists of an open source
relational database with (a) observational light curve, (b) theoretical light
curve, and (c) correlation table sets, statistical comparison software, and a
web interface available to the community. The theoretical models are intended
to span a gridded range of parameter space. The goal is to have users to upload
new SN models or new SN observations and run the comparison software to
determine correlations via the web site. There are looming problems on the
horizon that SNAP begins to solve. Namely, large surveys will discover
thousands of SNe annually. Frequently, the parameter space of a new SN event is
unbounded. SNAP will be a resource to constrain parameters and determine if an
event needs follow-up without spending resources to create new light curve
models from scratch. Secondly, there is not a rapidly available, systematic way
to determine degeneracies between parameters or even what physics is needed to
model a realistic SNe. The correlations made within the SNAP system begin to
solve these problems.
