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.