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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 C1.

Relative changes in the best-fit evening- (top panel) and morning-limb (bottom panel) transmission spectra when unfixing certain orbital parameters during the fit. The effects of unfixing the period are shown as circles, semimajor axis as squares, inclination as triangles, and eccentricity as stars. We compare these changes to the relative 1σ uncertainty obtained on the limb depths, shown by the black dashed lines.

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