Euclid on Sky
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Fig. 6

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Top panel: histogram of all pixels across a 200 arcsec2 region from a VIS detrended image. The histogram shows regular spikes at the 1 ADU frequency, indicative of quantisation noise (this effect is also observed in the raw data). Bottom panel: same region after resampling the detrended image with SWarp using a Lanczos3 function. The histogram shows that the pixels have been correlated and the quantisation error has been smoothed out.

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