# The ASAS-SN Bright Supernova Catalog I: 2013-2014

Holoien, TW-S and Stanek, KZ and Kochanek, CS and Shappee, BJ and Prieto, JL and Brimacombe, J and Bersier, D and Bishop, DW and Dong, S and Brown, JS and Danilet, AB and Simonian, GV and Basu, U and Beacom, JF and Falco, E and Pojmanski, G and Skowron, DM and Wozniak, PR and Avila, CG and Conseil, E and Contreras, C and Cruz, I and Fernandez, JM and Koff, RA and Guo, Z and Herczeg, GJ and Hissong, J and Hsiao, EY and Jose, J and Kiyota, S and Long, F and Monard, LAG and Nicholls, B and Nicolas, J and Wiethoff, WS (2016) The ASAS-SN Bright Supernova Catalog I: 2013-2014. Monthly Notices of the Royal Astronomical Society, 464 (3). pp. 2672-2686. ISSN 0035-8711

We present basic statistics for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during its first year-and-a-half of operations, spanning 2013 and 2014. We also present the same information for all other bright ($m_V\leq17$), spectroscopically confirmed supernovae discovered from 2014 May 1 through the end of 2014, providing a comparison to the ASAS-SN sample starting from the point where ASAS-SN became operational in both hemispheres. In addition, we present collected redshifts and near-UV through IR magnitudes, where available, for all host galaxies of the bright supernovae in both samples. This work represents a comprehensive catalog of bright supernovae and their hosts from multiple professional and amateur sources, allowing for population studies that were not previously possible because the all-sky emphasis of ASAS-SN redresses most previously existing biases. In particular, ASAS-SN systematically finds supernovae closer to the centers of host galaxies than either other professional surveys or amateurs, a remarkable result given ASAS-SN's poorer angular resolution. This is the first of a series of yearly papers on bright supernovae and their hosts that will be released by the ASAS-SN team.