Welcome to the Documentation for FastSpecFit
Overview
FastSpecFit is a stellar continuum and emission-line modeling code which is
optimized for speed and simplicity; it uses physically motivated stellar
population synthesis and emission-line templates to jointly model UV/optical
spectrophotometry and ultraviolet through infrared broadband photometry
(fastspec). Alternatively, it can be used to model just the broadband
photometry (fastphot).
FastSpecFit currently only supports DESI
spectrophotometric data, although contributions to develop the software for
other instruments and surveys are more than welcome.
Contents
Value Added Catalogs (VACs)
DR2 (Loa)
DR1 (Iron)
DR1 Supplement (Guadalupe)
EDR (Fuji)