Euclid on Sky
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Fig. 8

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Projected distribution and density map of GC candidates (white points) brighter than IE = 23.5 (left panel) versus the diffuse light in IE (background image in the right panel) in the ERO-F field of view in the Fornax cluster. In the left panel, the size of the white points (GC candidates) corresponds to the total magnitude of GC candidates (brighter GCs appear larger). In the right panel, the smoothed version of the ERO-F data made from four exposures is shown. This is a different stack than the stacked frame used for the GC selection (which is made from two exposures with the best PSF). The black lines within the image are regions without any available data.

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