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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 B5.

Gallery of light-curve residuals from our fits to the JWST/NIRSpec G395H spectroscopic light curves, with NRS1 data on the left and NRS2 on the right. 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, and note the different offsets in each panel. The vertical blue lines demarcate the approximate four transit contacts to indicate ingress and egress.

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