Image Details
Caption: Figure 1.
Data products at several stages of the reduction process for the NIRISS/SOSS eclipse observation of WASP-80 b. (a) Last group of the 113th integration, after superbias subtraction. (b) 1/f noise in frame (a). (c) Integration 113 after ramp fitting and flat field correction. (d) Final calibrated frame after background subtraction and bad pixels interpolation. The full and dashed lines represent the center and edges, respectively, of the aperture boxes used to extract the first (red) and second (blue) orders. The top trace is a contaminant from another star.
© 2025. The Author(s). Published by the American Astronomical Society.