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New Light Curve Analysis for Large Numbers of Eclipsing Binaries III. SMC and Galactic Center
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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.
Cambridge University Press (CUP)
Title: New Light Curve Analysis for Large Numbers of Eclipsing Binaries III. SMC and Galactic Center
Description:
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.
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