Image Details
Caption: Figure B2.
Top: raw NIRISS/SOSS order 1 (0.85–2.83 μm) white-light curves with 1σ error bars for the supreme-SPOON reduction (red) and the additional one (blue) with their temporally binned points. Bottom: difference between the white-light curve from the additional reduction and the one from supreme-SPOON. The error bars on the residuals represent the maximum ones between the two reductions. In general, both white-light curves follow the same trends.
© 2025. The Author(s). Published by the American Astronomical Society.