Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University
Mon. Not. R. Astron. Soc. 477, 3145-3163 (2018)
The All-Sky Automated Survey for Supernovae (ASAS-SN) is the first optical survey to routinely monitor the whole sky with a cadence of ∼2–3 d down to V 17 mag. ASAS-SN has monitored the whole sky since 2014, collecting ∼100–500 epochs of observations per field. The V-band light curves for candidate variables identified during the search for supernovae are
classified using a random forest classifier and visually verified.We present a catalogue of 66 179
bright, new variable stars discovered during our search for supernovae, including 27 479 periodic variables and 38 700 irregular variables. V-band light curves for the ASAS-SN variables
are available through the ASAS-SN variable stars data base (https://asas-sn.osu.edu/variables).
The data base will begin to include the light curves of known variable stars in the near future
along with the results for a systematic, all-sky variability survey.
@article{UTF692,
author = {Jayasinghe, T. and Kochanek, C. S. and Stanek, K. Z. and Shappee, B. J. and Holoien, T. W. -S. and Thompson, Todd A. and Prieto, J. L. and Dong, Subo and Pawlak, M. and Shields, J. V. and Pojmanski, G. and Otero, S. and Britt, C. A. and Will, D.},
title = {{The ASAS-SN catalogue of variable stars I: The Serendipitous Survey}},
journal = {Mon. Not. R. Astron. Soc.},
volume = {477},
pages = {3145-3163},
year = {2018},
doi = {10.1093/mnras/sty838},
}