EvapMass: Minimum mass of planets predictor
Abstract: EvapMass predicts the minimum masses of planets in multi-planet systems using the photoevaporation-driven evolution model. The planetary system requires both a planet above and below the radius gap to be useful for this test. EvapMass includes an example Jupyter notebook for the Kepler-36 system. EvalMass can be used to identify TESS systems that warrant radial-velocity follow-up to further test the photoevaporation model.
Credit: Owen, James E.; Campos Estrada, Beatriz
Site: https://github.com/jo276/EvapMass
https://ui.adsabs.harvard.edu/abs/2020MNRAS.491.5287O
Bibcode: 2020ascl.soft11015O
ID: ascl:2011.015