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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 B3.

Gallery of light-curve residuals from our fits to the JWST/MIRI LRS spectroscopic light curves. Gray points are the light curve at native cadence, and black points are binned to ∼500 s cadence chosen to be consistent across all instruments (Figures B1–B5). Each channel’s residual time series is vertically offset for visual separation. Note that the left and middle panels share an offset, and the right panel has a different offset. The vertical blue lines demarcate the approximate four transit contacts to indicate ingress and egress.

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