tokens: RH thanks Avi Shporer for providing the program to compute ingress and egress shapes, Tiffany Kataria for making available preliminary 3D atmospheric circulation simulations, Edwin Kite for discussion on the molten lava planet, Feng Tian for discussion on the atmospheric escape of rocky planets, and Wesley Traub and Yuk L. Yung for helpful discussions. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. Support for RH’s work was provided in part by NASA through Hubble Fellowship grant #51332 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. Part of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. NKL’s work was performed in part under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute.
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