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Asteroseismology of Eclipsing Binary Stars in the Kepler Era [PDF]

open access: yes, 2014
Eclipsing binary stars have long served as benchmark systems to measure fundamental stellar properties. In the past few decades, asteroseismology - the study of stellar pulsations - has emerged as a new powerful tool to study the structure and evolution ...
A. Derekas   +107 more
core   +4 more sources

ELLC - a fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets [PDF]

open access: yesAstronomy and Astrophysics, 2016
Very high quality light curves are now available for thousands of detached eclipsing binary stars and transiting exoplanet systems as a result of surveys for transiting exoplanets and other large-scale photometric surveys.
Maxted, P. F. L.
core   +7 more sources

Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2 and 3 [PDF]

open access: yesAstronomy & Astrophysics, 2018
The Kepler K2 mission now makes it possible to find and study a wider variety of eclipsing binary stars than has been possible to-date, particularly long-period systems with narrow eclipses.
Hutcheon, RJ, Maxted, PFL
core   +4 more sources

Automatic classification of eclipsing binary stars using deep learning methods [PDF]

open access: yesAstronomy and Computing, 2021
In the last couple of decades, tremendous progress has been achieved in developing robotic telescopes and, as a result, sky surveys (both terrestrial and space) have become the source of a substantial amount of new observational data.
M. Cokina   +3 more
semanticscholar   +3 more sources

Eclipsing binary stars in the era of massive surveys First results and future prospects [PDF]

open access: yesEPJ Web of Conferences, 2017
Our thinking about eclipsing binary stars has undergone a tremendous change in the last decade. Eclipsing binary stars are one of nature’s best laboratories for determining the fundamental physical properties of stars and thus for testing the predictions
Papageorgiou Athanasios   +3 more
doaj   +2 more sources

TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26 [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2021
In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary candidates, detection of hitherto unknown eclipsing systems ...
A. Prša   +46 more
semanticscholar   +7 more sources

The TESS Ten Thousand Catalog: 10,001 Uniformly Vetted and Validated Eclipsing Binary Stars Detected in Full-frame Image Data by Machine Learning and Analyzed by Citizen Scientists

open access: yesThe Astrophysical Journal Supplement Series
The Transiting Exoplanet Survey Satellite (TESS) has surveyed nearly the entire sky in full-frame image mode with a time resolution of 200 s to 30 minutes and a temporal baseline of at least 27 days.
Veselin B. Kostov   +38 more
doaj   +2 more sources

Kepler Eclipsing Binary Stars. V. Identification of 31 Eclipsing Binaries in the K2 Engineering Data-set [PDF]

open access: yes, 2014
Over 2500 eclipsing binaries were identified and characterized from the ultra-precise photometric data provided by the Kepler space telescope. Kepler is now beginning its second mission, K2, which is proving to again provide ultra-precise photometry for ...
Abdul-Masih, Michael   +10 more
core   +5 more sources

Expected Large Synoptic Survey Telescope (LSST) Yield of Eclipsing Binary Stars [PDF]

open access: yes, 2011
In this paper we estimate the Large Synoptic Survey Telescope (LSST) yield of eclipsing binary stars, which will survey ~20,000 square degrees of the southern sky during the period of 10 years in 6 photometric passbands to r ~ 24.5.
Abazajian   +21 more
core   +2 more sources

The surface brightness–colour relations based on eclipsing binary stars and calibrated with Gaia EDR3 [PDF]

open access: yesAstronomy & Astrophysics, 2021
Aims. The surface brightness–colour relation (SBCR) is a basic tool for establishing precise and accurate distances within the Local Group. Detached eclipsing binary stars with accurately determined radii and trigonometric parallaxes allow calibration of
D. Graczyk   +25 more
semanticscholar   +1 more source

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