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New Light Curve Analysis for Large Numbers of Eclipsing Binaries III. SMC and Galactic Center

Published online by Cambridge University Press:  23 April 2012

Young-Woon Kang ,
Keong Soo Hong  and
Pakakaew Rittipruk
Young-Woon Kang
Affiliation:
Sejong University, Seoul, 143-747, Korea email: kangye@sejong.ac.kr
Keong Soo Hong
Affiliation:
Sejong University, Seoul, 143-747, Korea email: kangye@sejong.ac.kr
Pakakaew Rittipruk
Affiliation:
Sejong University, Seoul, 143-747, Korea email: kangye@sejong.ac.kr
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Abstract

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We 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.

Keywords

starseclipsing binariesdata analysisfundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S282: From Interacting Binaries to Exoplanets: Essential Modeling Tools , July 2011 , pp. 329 - 330
Copyright
Copyright © International Astronomical Union 2012

References

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