English

The ASAS-SN Bright Supernova Catalog -- IV. 2017

High Energy Astrophysical Phenomena 2019-10-14 v2

Abstract

In this catalog we compile information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) as well as all other bright (mpeak17m_{peak}\leq17), spectroscopically confirmed supernovae found in 2017, totaling 308 supernovae. We also present UV through near-IR magnitudes gathered from public databases of all host galaxies for the supernovae in the sample. We perform statistical analyses of our full bright supernova sample, which now contains 949 supernovae discovered since 2014 May 1, including supernovae from our previous catalogs. This is the fourth of a series of yearly papers on bright supernovae and their hosts from the ASAS-SN team, and this work presents updated data and measurements, including light curves, redshifts, classifications, and host galaxy identifications, that supersede information contained in any previous publications.

Keywords

Cite

@article{arxiv.1811.08904,
  title  = {The ASAS-SN Bright Supernova Catalog -- IV. 2017},
  author = {T. W. -S. Holoien and J. S. Brown and P. J. Vallely and K. Z. Stanek and C. S. Kochanek and B. J. Shappee and J. L. Prieto and Subo Dong and J. Brimacombe and D. W. Bishop and S. Bose and J. F. Beacom and D. Bersier and Ping Chen and L. Chomiuk and E. Falco and S. Holmbo and T. Jayasinghe and N. Morrell and G. Pojmanski and J. V. Shields and J. Strader and M. D. Stritzinger and Todd A. Thompson and P. R. Wozniak and G. Bock and P. Cacella and J. G. Carballo and E. Conseil and I. Cruz and R. G. Farfan and J. M. Fernandez and S. Kiyota and R. A. Koff and G. Krannich and P. Marples and G. Masi and L. A. G. Monard and J. A. Munoz and B. Nicholls and R. S. Post and G. Stone and D. L. Trappett and W. S. Wiethoff},
  journal= {arXiv preprint arXiv:1811.08904},
  year   = {2019}
}

Comments

14 pages, 6 figures, 4 tables. Updated to reflect changes made in the published version. Tables containing the catalog data presented in this submission are included in machine-readable format as ancillary files

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