2 code implementations • 29 May 2020 • Travis A. Berger, Daniel Huber, Eric Gaidos, Jennifer L. van Saders, Lauren M. Weiss
We measure the stellar mass dependence of the planet radius valley to be $d \log R_{\mathrm{p}}$/$d \log M_\star = 0. 26^{+0. 21}_{-0. 16}$, consistent with the slope predicted by a planet mass dependence on stellar mass ($0. 24-0. 35$) and core-powered mass-loss (0. 33).
Earth and Planetary Astrophysics Astrophysics of Galaxies Solar and Stellar Astrophysics