Fig. 1
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Footprint of the VIS image of the Perseus galaxy cluster covering 0.°84 × 0.°84 and overplotted on the PanSTARRS DR1 g + r + i colour image with FoV ~ 1.°17 × 1.°17; north is up and east left. The green circles show the location of the dwarf galaxy candidates identified in the ERO data, while the grey patches represent the footprint of HST/ACS observations (F850LP/SDSSz, F814w, F791w, F785LP, F775w, F625w, F622w filters). The green circles that fall just outside of the Euclid footprint were identified in an earlier data product with a slightly larger FoV.
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