Fig. 1

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White light curves created from the first two spectral orders of the NIRISS SOSS data and combined best-fit model. The top panels show the observed data and fitted model light curves, while the bottom panels show the standardized residuals. The standardized residuals are the residuals divided by the uncertainty σφ that combines the uncertainties in flux reported by the pipeline σt with the additional jitter term σω fitted by the juliet framework (
). The outer bottom panels compare the distribution of the standardized residuals to the shape expected for Gaussian noise. The shaded regions indicate the time intervals used for baseline normalization (gray) and a suspected spot crossing event (yellow).
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