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[ascl:2011.015] EvapMass: Minimum mass of planets predictor

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.

Code site:
https://github.com/jo276/EvapMass
Described in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.491.5287O
Bibcode:
2020ascl.soft11015O

Views: 736

ascl:2011.015
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