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Cited article:

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The Astrophysical Journal 872 (1) 85 (2019)
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The Surface Brightness-color Relations Based on Eclipsing Binary Stars: Toward Precision Better than 1% in Angular Diameter Predictions

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The Astrophysical Journal 837 (1) 7 (2017)
https://doi.org/10.3847/1538-4357/aa5d56

Asiago eclipsing binaries program IV. SZ Camelopardalis, aβ Cephei pulsator in a quadruple, eclipsing system

E. Tamajo, U. Munari, A. Siviero, L. Tomasella and S. Dallaporta
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A CLASSICAL CEPHEID IN A LARGE MAGELLANIC CLOUD ECLIPSING BINARY: EVIDENCE OF SHORTCOMINGS IN CURRENT STELLAR EVOLUTIONARY MODELS?

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Accurate masses and radii of normal stars: modern results and applications

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ORBIT DETERMINATION OF DOUBLE-LINED SPECTROSCOPIC BINARIES BY FITTING THE REVISEDHIPPARCOSINTERMEDIATE ASTROMETRIC DATA

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The Astronomical Journal 139 (5) 1975 (2010)
https://doi.org/10.1088/0004-6256/139/5/1975