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To ensure robust constraints are placed on exoplanet atmospheric transmissionspectra, future observations need to obtain high signal-to-noise ratio (SNR)measurements assuming smaller amplitude molecular signatures than those ofclear solar metallicity atmospheres. Analyzing 37 exoplanet transmissionspectra we find clear solar molecular features are measured in <7% of cases.

Exoplanet Atmosphere Forecast: Observers Should Expect Spectroscopic Transmission Features to be Muted to 33%