作者: D. J. Armstrong , Y. Gómez Maqueo Chew , F. Faedi , D. Pollacco
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摘要: We have combined the Kepler Eclipsing Binary Catalogue with information from HES, KIS and 2MASS photometric surveys to produce spectral energy distribution fits over 2600 eclipsing binaries in catalogue a wavelength range of 0.36–2.16 A. present primary (T1) secondary (T2) stellar temperatures, plus on radii system distance ratios. The derived temperatures are average accurate 370 K T1 620 K T2. Our results improve similarly physical parameters Input through consideration both stars binary rather than single star model, inclusion additional U-band photometry. expect these aid future uses data, target selection inform users extremely high-precision light curves available. do not include surface gravities or metallicities, as were found an insignificant effect observed bands.