Image Details

Choose export citation format:

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 11.

Retrieved cloud fraction, ﹩{\bar{\phi }}_{\mathrm{clouds}}﹩, trends with retrieved water abundance (left) and planetary equilibrium temperature (right). Dashed and dotted lines represent the solar abundance values for temperatures < 1200 K and > 1200 K calculated by Madhusudhan (2012), respectively. The planets are colored by equilibrium temperature from the hottest (WASP-12b) in yellow to the coldest (HAT-P-11b) in purple.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse