Image Details
Caption: Figure 4.
The observational H-R diagram—effective temperature vs. surface gravity—showing the UberMS fit to TOI-7019’s TRES spectrum and broadband photometry. Black contours delineate the 1σ–3σ statistical error regimes. The R. Andrae et al. (2023) measurement using low-resolution Gaia XP data is also shown. Gaia XP metallicities have a reported uncertainty of 0.1 dex (R. Andrae et al. 2023). MIST isochrones are overlaid for a range of stellar ages, with other parameters fixed to the adopted values for TOI-7019.
© 2026. The Author(s). Published by the American Astronomical Society.