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The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10405630" target="_blank" >RIV/00216208:11320/19:10405630 - isvavai.cz</a>

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=osl~YTW7mi" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=osl~YTW7mi</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/stz444" target="_blank" >10.1093/mnras/stz444</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone

  • Original language description

    The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long-baseline (similar to 4 yr) light curves for sources brighter than V less than or similar to 17 mag across the whole sky. The Transiting Exoplanet Survey Satellite (TESS) has started to produce high-quality light curves with a baseline of at least 27 d, eventually for most of the sky. The combination of ASAS-SN and TESS light curves probes both long-and short-term variability in great detail, especially towards the TESS continuous viewing zones (CVZ) at the ecliptic poles. We have produced similar to 1.3 million V-band light curves covering a total of similar to 1000 deg(2) towards the southern TESS CVZ and have systematically searched these sources for variability. We have identified similar to 11 700 variables, including similar to 7 000 new discoveries. The light curves and characteristics of the variables are all available through the ASAS-SN variable stars data base (https://asas-sn.osu.edu/variables). We also introduce an online resource to obtain pre-computed ASAS-SN V-band light curves (https://asas-sn.osu.edu/photometry) starting with the light curves of the similar to 1.3 million sources studied in this work. This effort will be extended to provide ASAS-SN light curves for similar to 50 million sources over the entire sky.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

  • Volume of the periodical

    485

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    11

  • Pages from-to

    961-971

  • UT code for WoS article

    000466786400066

  • EID of the result in the Scopus database

    2-s2.0-85067213090