Acta Astronomica

dc.creatorGraczyk, D.
dc.date2019-12-18T18:14:55Z
dc.date2022-07-07T22:05:54Z
dc.date2019-12-18T18:14:55Z
dc.date2022-07-07T22:05:54Z
dc.date2010
dc.date.accessioned2023-08-22T09:11:19Z
dc.date.available2023-08-22T09:11:19Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/237171
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8335590
dc.descriptionA semi-automatic method of identifying eclipsing binaries in large photometric surveys, based on the analysis of the light curve statistical moments, is presented. This method was tested on the OGLE-II database of variable stars in the Large Magellanic Cloud. As a result 99.0% of eclipsing binaries in Wyrzykowski et al. (2003) catalog and 100% of eclipsing binaries in Groenewegen (2005) catalog were recovered. Additionally we identified 752 new eclipsing binaries in the LMC that were not presented in earlier catalogs thereby increasing detection rates by about 25%. The method is more focusing on detached and semi-detached eclipsing binaries. We conclude that this method is well suited for use in eclipsing binary searches of large surveys such as OGLE-III.
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.relationinfo:eu-repo/grantAgreement/Fondap/15010003
dc.relationhttps://www.researchgate.net/publication/234542708_The_Light_Curve_Statistical_Moments_Analysis_The_Identification_of_Eclipsing_Binaries
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleThe Light Curve Statistical Moments Analysis: The Identification of Eclipsing Binaries
dc.titleActa Astronomica
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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