ASASSN-V J104422.03-620547.7 , the SIMBAD biblio

2018MNRAS.477.3145J - Mon. Not. R. Astron. Soc., 477, 3145-3163 (2018/July-1)

The ASAS-SN catalogue of variable stars I: The Serendipitous Survey.

JAYASINGHE T., KOCHANEK C.S., STANEK K.Z., SHAPPEE B.J., HOLOIEN T.W.-S., THOMPSON T.A., PRIETO J.L., DONG S., PAWLAK M., SHIELDS J.V., POJMANSKI G., OTERO S., BRITT C.A. and WILL D.

Abstract (from CDS):

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.

Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): catalogues - surveys - binaries: eclipsing - stars: variables: general

VizieR on-line data: <CDS Catalogue: II/366> : gather 2018MNRAS.477.3145J (N=65270), 2019MNRAS.486.1907J (N=350445), 2019MNRAS.485..961J (N=8848), 2019MNRAS.487.5932P (N=1924), 2020MNRAS.491...13J (N=122648), and 2020MNRAS.493.4186J (N=117367)

Nomenclature: ASASSN-V JHHMMSS.ss+DDMMSS.s N=66179.

Status at CDS : All or part of tables of objects could be ingested in SIMBAD; there are some issues with cross-identifications or classifications.

CDS comments: The resolution of the ASAS-SN survey is 15''. As a consequence the astrometry is poor, usually within 5'', but it can be more than 1 pixel. Status of the catalogue II/366 in SIMBAD : Classical Cepheids (Type = DCEP or DCEPS, N=2183), and Mira Variables (Type = M, N=10230), have been enterely ingested; other LPVs are being processed. Objects with an undefined variability type (Type = VAR, N=62577) will not be ingested.

Simbad objects: 1902

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