Casagrande, Luca; Portinari, Laura; Glass, I; Laney, D.; Silva Aguirre, V; Datson, J.; Andersen, J; Nordstrom, B; Holmberg, Johan; Flynn, C.; Asplund, Martin
The apparent size of stars is a crucial benchmark for fundamental stellar properties such as effective temperatures, radii and surface gravities. While interferometric measurements of stellar angular diameters are the most direct method to gauge these, they are still limited to relatively nearby and bright stars, which are saturated in most of the modern photometric surveys. This dichotomy prevents us from safely extending well-calibrated relations to the faint stars targeted in large...[Show more]
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