I will present the results of applying a panchromatic SED-fitting
technique to a sample of 1404 local galaxies selected at 250um in data
from the Herschel ATLAS project. I will discuss our results, including
the determination of dust luminosities and masses, star formation
rates, and a variety of other physical parameters. I will also present
the results obtained by using our large sample to create a new set of
empirical template SEDs for these galaxies, binned according to their
physical properties, and show their differences from other
currently-available panchromatic SED template libraries.