Fig. 2.
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Zoomed view of the dwarf galaxy in Fig. 1 as seen by Euclid/VIS in IEand HST/ACS in F814W (PIPER survey, Harris et al. 2020). The total integration times for these images are 8960 s and 2100 s respectively. The depths of both datasets are comparable, while HST/ACS provides a higher spatial resolution with a better sampled PSF than Euclid/VIS.
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