Planetary radius measurements in literature have uncertainties about 40% larger than we measure in this work.

John Southworth, a co-author of this paper, used the revised stellar parameters, and in some cases did new fitting of #TESS lightcurves, and found that our measurements were more precise than those found in the literature.

The attached plot shows the revised #exoplanet radius and mass, along with the difference between ours and those in #TEPCat (https://www.astro.keele.ac.uk/jkt/tepcat/).