An optimization technique for the Fourier analysis of the light curves of totally-eclipsing systems of Algol-type

Details An optimization technique for the Fourier analysis of the light curves of totally-eclipsing systems of Algol-type An optimization technique for the Fourier analysis of the light curves of totally-eclipsing systems of Algol-type

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.172..249n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 172, no. 2, Oct. 1990, p. 249-253.

Statistics

Computation

Eclipsing Binary Stars, Fourier Analysis, Light Curve, Optimization, Computational Astrophysics, Stellar Luminosity, Stellar Spectrophotometry, Variable Stars

Scientific paper

A fully automatized technique for the evaluation of geometric and photometric elements of Algol-type systems exhibiting total eclipses is presented. The method requires observations in at least two wavelengths and enables us to choose the most probable solution from a grid of solutions performed with various possible phase angles of the first contact of the eclipse

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