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Fig. 1

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Pixel light curves centred on the PSF for the second eclipse, excluding the first 45 minutes dominated by settling and binned for clarity. A sharp persistence effect from a cosmic ray is highlighted with orange dashed boxes (see Appendix A for details). Pixels highlighted with green boundaries were fit using the pixel-fitting method except where specified we excluded the pixels containing the highlighted flux jump. Significant systematics are visible in the central light curves which may be flux-conserved between pixels or be independent for each pixel.

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