Our stellar radii have uncertainties of about 2%, and we measure stellar temperatures to around 50K.
We validated our parameters, via synthetic #Gaia #DR3 G-band photometry, we find that our parameters show a factor of 10 reduction in RMS residual and nearly a 40% improvement in mean uncertainty, when compared to the literature. The attached plot shows this comparison, with data derived from literature parameters shown in blue, and our parameters shown in red.








