A major goal of ASAS-SN is to make a complete census of bright supernovae, so from the beginning our strategy has been to observe the sky in a ``galaxy-unbiased way''. We want to find all SNe above a certain brightness, whether they happen in a well-monitored, nearby Messier galaxy or a tiny, uncatalogued, dwarf galaxy.

Here we show archival SDSS images of host galaxies for eight of the Type Ia SNe discovered in 2013 by ASAS-SN. The images are sorted by the luminosity of the host galaxy (from less to more luminous) and are centered on the supernova position. Even this initial, small sample of Type I discovered by ASAS-SN shows a significant diversity of host galaxy luminosity and type, and also supernova location within the host. Obtaining a galaxy-unbiased sample of nearby supernovae with ASAS-SN, both core-collapse and Type Ia, is particularly valuable because we can easily obtain the photometric and spectroscopic data needed to study the properties of these host galaxies both globally and local to the SN site.