Fitting starspot-crossing events recovers transit depths better than masking in high-SNR, high-contamination cases; small/faint spots can overcorrect, and SCEs inflate depth uncertainties at JWST precision.
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Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves
Fitting starspot-crossing events recovers transit depths better than masking in high-SNR, high-contamination cases; small/faint spots can overcorrect, and SCEs inflate depth uncertainties at JWST precision.