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Atmospheric Reconnaissance of TRAPPIST-1 f with JWST NIRISS SOSS: No Evidence for the Transit Light Source Effect

  • Authors: Olivia Lim, René Doyon, Ryan J. MacDonald, Étienne Artigau, Michael Radica, Mykhaylo Plotnykov, Alexandrine L'Heureux, Caroline Piaulet-Ghorayeb, Louis-Philippe Coulombe, David Lafrenière, Thomas J. Fauchez, Martin Turbet, Diana Valencia, Loïc Albert, Laura Flagg, Björn Benneke, Neil J. Cook, Pierre-Alexis Roy, Lisa Kaltenegger, Charles Cadieux, Nicolas B. Cowan, Michaël Gillon, Romain Allart, Lisa Dang, Doug Johnstone, Stefan Pelletier, Jared Splinter, Jake Taylor

Olivia Lim et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure B6.

Systematics-corrected, spectroscopic light curves (left of each pair of panels) and residuals from the best-fitting transit and systematics model (right of each pair of panels). Panels are displayed from left to right and from top to bottom in chronological order of observation. White spaces represent data that were masked during the light-curve fit. Shaded regions in Visit 1 indicate the wavelengths that the asteroid crossed on the spectral trace.

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