Intensity interferometry can measure Red Clump star angular diameters to <1% precision in short exposures, providing independent validation for surface-brightness-color relations in the distance ladder.
D., Davis, J., Bless, R
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Empirical zero-point constants for Gaia bolometric corrections are derived as weighted averages 0.8677, 1.0449, and 2.0510 mag for G, GBP, and GRP from 88 stars, yielding corresponding magnitude zero-points via IAU definitions.
citing papers explorer
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Validating the Angular Sizes of Red Clump Stars with Intensity Interferometry
Intensity interferometry can measure Red Clump star angular diameters to <1% precision in short exposures, providing independent validation for surface-brightness-color relations in the distance ladder.
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Spectroscopic Bolometric Corrections and Empirical Zero-point Constants of \textit{Gaia} Magnitudes, $G$, $G_{\rm BP}$, and $G_{\rm RP}$, from \textit{Gaia} XP Spectra
Empirical zero-point constants for Gaia bolometric corrections are derived as weighted averages 0.8677, 1.0449, and 2.0510 mag for G, GBP, and GRP from 88 stars, yielding corresponding magnitude zero-points via IAU definitions.