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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 1.

The top panel of each subplot shows the broadband light curve (black and gray points) and the best-fit transit and systematics model (blue curve) for the five transits of TRAPPIST-1 f. Gray points are integrations that were masked in the light-curve fit. The in-transit, masked integrations in Visit 4 correspond to a possible spot-crossing event. All other masked integrations are masked due to stellar activity. The middle panels show the residuals from the best-fit model, while the bottom panels show the integrated flux of the Hα stellar line. Gray points correspond to the light-curve points that were masked in the fit. All error bars are 1σ uncertainties.

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