A Comparison of Simulated JWST Observations Derived from Equilibrium and Non-equilibrium Chemistry Models of Giant Exoplanets

@article{Blumenthal2017ACO,
  title={A Comparison of Simulated JWST Observations Derived from Equilibrium and Non-equilibrium Chemistry Models of Giant Exoplanets},
  author={Sarah D. Blumenthal and Avi M. Mandell and Eric H'ebrard and Natasha E. Batalha and Patricio E. Cubillos and Sarah Rugheimer and Hannah R. Wakeford},
  journal={The Astrophysical Journal},
  year={2017},
  volume={853}
}
We aim to see if the difference between equilibrium and disequilibrium chemistry is observable in the atmospheres of transiting planets by the James Webb Space Telescope (JWST). We perform a case study comparing the dayside emission spectra of three planets like HD 189733b, WASP-80b, and GJ 436b, in and out of chemical equilibrium at two metallicities each. These three planets were chosen because they span a large range of planetary masses and equilibrium temperatures, from hot and Jupiter… 

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