Image Details
Caption: Figure 7.
Top panel: comparison of the limb-darkened angular diameters measured here vs. diameters from JSDC (Bourgés et al. 2014). The linear fit is f(x) = 0.969x + 0.088. Bottom panel: the same, but from Gaia (Gaia Collaboration et al. 2018; Cruzalèbes et al. 2019), with a linear fit of f(x) = 0.996x + 0.246. Note that no errors were indicated for the Gaia diameters, so the residuals are simply θ NPOI − θ GAIA.
© 2023. The Author(s). Published by the American Astronomical Society.