New Light Curve Analysis for Large Numbers of Eclipsing Binaries III. SMC and Galactic Center
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Published:2011-07
Issue:S282
Volume:7
Page:329-330
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ISSN:1743-9213
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Container-title:Proceedings of the International Astronomical Union
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language:en
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Short-container-title:Proc. IAU
Author:
Kang Young-Woon,Hong Keong Soo,Rittipruk Pakakaew
Abstract
AbstractWe improved the method of light curve analysis for large numbers of eclipsing binaries. Current methods require a week to analyze the light curves of an eclipsing binary for its physical and orbital parameters. Therefore, we developed a new method to treat large numbers of light curves of eclipsing binaries. We tested the new method by analyzing more than 14 hundred light curves and 9 hundred light curves discovered by OGLE in the Small Magellanic Cloud and Galactic center, respectively.
Publisher
Cambridge University Press (CUP)
Subject
Astronomy and Astrophysics,Space and Planetary Science
Cited by
2 articles.
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