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The Importance of Optical Wavelength Data on Atmospheric Retrievals of Exoplanet Transmission Spectra

  • Authors: Charlotte Fairman, Hannah R. Wakeford, Ryan J. MacDonald

Charlotte Fairman et al 2024 The Astronomical Journal 167 .

  • Provider: AAS Journals

Caption: Figure 9.

IC (measured in nats) broken down by parameter group for ﹩{\lambda }_{\min }﹩ = 1.1–0.3 μm. Top: breakdown of parameters by R P,ref, T, alkali species, H2O, carbon species, cloud parameters, high-temperature species (TiO/VO), and stellar parameters. Bottom: breakdown of IC change per cloud parameter. Planets are ordered from highest to lowest (left to right) retrieved Rayleigh enhancement factor, ﹩\mathrm{log}a﹩.

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