The attached plot shows the revised #exoplanet radius and mass, along with the difference between ours and those in #TEPCat (astro.keele.ac.uk/jkt/tepcat/).
The attached plot shows the revised #exoplanet radius and mass, along with the difference between ours and those in #TEPCat (astro.keele.ac.uk/jkt/tepcat/).
Using synthetic #Gaia #DR3 G-band photometry, our parameters show a factor of 10 reduction in RMS residual and nearly a 40% improvement in mean uncertainty, when compared to the literature.