Fig. 17
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Left: level 2a flux image from the ERO program of the lensed cluster observations of SMACS0723 (PID 2736). Slew persistence that resembles a check mark can be seen in the image taken 5 h after the bright star that was the origin of the slew persistence. Right: image taken 12 h later in program PID 1124. The slew persistence can just be made out in this image.
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