Euclid on Sky
Open Access

Fig. 3

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Left: ERO pipeline LSB stack preserving all scales across the image. The pipeline is optimised for the photometry of extended objects such as these Perseus cluster galaxies. Right: ERO pipeline for compact-sources removing most of the LSB signal. The stack with internal background subtraction suppresses much of the signal from the large galaxies. The field size is 3′ by 3′.

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