HUBER , D.

Context. Surface brightness–colour relations (SBCRs) are used to derive the stellar angular diameters from photometric observations. They have various astrophysical applications, such as the distance determination of eclipsing binaries or the determination of exoplanet parameters. However, strong discrepancies between the SBCRs still exist in...

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Photometric and interferometric parameters of 534 late-type stars and the associated references. The stars are separated into four tables, according to their spectral type and luminosity class, leading to F5/K7-II/III, F5/K7-IV/V, M-II/III and M-IV/V samples. Interferometric measurements are taken from the JMMC Measured Diameters Catalog (JMDC,...

We obtained high-resolution spectra of HD 221416 using several facilities within the TESS Follow-up Observation Program (TFOP), including HIRES (Vogt et al. 1994SPIE.2198..362V) on the 10 m telescope at Keck Observatory (Maunakea, Hawai'i); the Hertzsprung SONG Telescope at Teide Observatory (Tenerife; Grundahl et al. 2017ApJ...836..142G);...

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