Statistical Analysis of Hubble/WFC3 Transit Spectroscopy of Extrasolar Planets
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Abstract
Transmission spectroscopy provides a window to study exoplanetary
atmospheres, but that window is fogged by clouds and hazes. Clouds and haze
introduce a degeneracy between the strength of gaseous absorption features and
planetary physical parameters such as abundances. One way to break that
degeneracy is via statistical studies. We collect all published HST/WFC3
transit spectra for 1.1-1.65
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2041-8213