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A Panchromatic Characterization of the Evening and Morning Atmosphere of WASP-107 b: Composition and Cloud Variations, and Insight into the Effect of Stellar Contamination

  • Authors: Matthew M. Murphy, Thomas G. Beatty, Everett Schlawin, Taylor J. Bell, Michael Radica, Thomas D. Kennedy, Nishil Mehta, Luis Welbanks, Michael R. Line, Vivien Parmentier, Thomas P. Greene, Sagnick Mukherjee, Jonathan J. Fortney, Kazumasa Ohno, Lindsey Wiser, Kenneth Arnold, Emily Rauscher, Isaac R. Edelman, Marcia J. Rieke

Matthew M. Murphy et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 11.

Comparing the relative limb transit depths of WASP-107 b to WASP-39 b (N. Espinoza et al. 2024). Panel (A) shows the evening-limb spectra for each planet, relative to the depth at 4.15 μm and scaled to each planet’s scale height. Panel (B) shows the same for the morning-limb spectra, and panel (C) shows the relative evening- and morning-limb spectra just for WASP-107 b.

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