NASA NTRS · 19730050976
Correlations among the parameters of the spherical model for eclipsing binaries.
Abstract
Correlation coefficients have been computed to investigate the parameters used to describe the spherical model of an eclipsing binary system. Regions in parameter hyperspace have been identified where strong correlations exist and, by implication, the solution determinacy is low. The results are presented in tabular form for a large number of system configurations.
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Sobieski, S., White, J.. 1973-03-01. Correlations among the parameters of the spherical model for eclipsing binaries.. https://ntrs.nasa.gov/citations/19730050976
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