Top: Hertzsprung-Russell diagram with the luminosity of the RG and MS from the eclipsing binary radius and the IRFM temperature (this work). The two isochrones shown were calculated from the MESA grid of stellar models used in this paper. We also include eclipsing binary measurements from Gaulme et al. (2016) and the asteroseismic inference of the RG from Montalbán et al. (2021). Bottom: Mass and radius of the same sources, along with the same isochrones. All markers have error bars in x and y, but in some cases, they are smaller than the marker.