Fig. 4.
H2S broadened by H2 and He using different broadening parameters based on values for HCl and OCS. The cross sections in the top panel are computed at T = 1000 K and (P = 0.1 bar), which are typical values for a layer of atmosphere of a Hot Jupiter exoplanet observed in this wavelength region. The cross sections in the bottom panel are computed at T = 100 K and P = 1 × 10−5 bar.
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