Fourier analysis of the light curves of eclipsing variables. XXVI - Comparison with Kitamura's method

Details Fourier analysis of the light curves of eclipsing variables. XXVI - Comparison with Kitamura's method Fourier analysis of the light curves of eclipsing variables. XXVI - Comparison with Kitamura's method

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72....3k&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 3-14. Research supported by the British Council.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Fourier Analysis, Light Curve, Computer Techniques, Fourier Transformation, Limb Darkening

Scientific paper

Analytic expressions are constructed for incomplete Fourier transforms underlying Kitamura's method (1965) for the analysis of the light curves of eclipsing binaries. Expansion established for Kitamura's coefficients cn and sn are used as the basis for checking the numerical accuracy of these coefficients tabulated by Kitamura (1967); the result points to the high quality of Kitamura's tables constructed by numerical quadratures.

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