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Fig. 12

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Flagging status at the frame level for the first five integrations (y-axis) of the L168-9b data after applying the cosmic-ray detection step (also known as the jump detection step) using version 1.8.5 of the pipeline. The flagging status is shown for all pixels located in the brightest Col. 36 (x-axis). The colour code shows the status of each frame. Frames in blue are valid and therefore kept in the dataset for the ramp adjustment step. Frames in grey are rejected from the dataset by the last frame-effect detection step. Frames in yellow are rejected by the jump detection step and are mostly between number 1 and 5. They are located at short wavelengths (rows of pixels ranging from ~340 to 390, mainly focused on pixels with high fluxes).

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