  We present bolometric and broadband light curves and spectra for a suite of
core-collapse supernova models exploded self-consistently in spherical symmetry
within the PUSH framework. We analyze broad trends in these light curves and
categorize them based on morphology. We find these morphological categories
relate simply to the progenitor radius and the mass of the hydrogen envelope.
We present a proof-of-concept sensitive-variable analysis, indicating that an
important determining factor in the properties of a light curve within a given
category is $^{56}$Ni mass. We follow spectra from the photospheric to the
nebular phase. These spectra show characteristic iron-line blanketing at short
wavelengths and Doppler-shifted Fe II and Ti II absorption lines. To enable
this analysis, we develop a first-of-its-kind pipeline from a massive
progenitor model, through a self-consistent explosion in spherical symmetry, to
electromagnetic counterparts. This opens the door to more detailed analyses of
the collective properties of these observables. We provide a machine readable
database of our light curves and spectra online at go.ncsu.edu/astrodata.
