Fig. 3.
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Extinction-reddening corrected colour-magnitude diagrams from MUSE images of the three fields, moving from the centre towards the outer regions from left to right; the filled circles represent the sources for which spectra have been extracted and they are colour-coded by their S/N at the central wavelength. We note that the galaxy’s distance modulus is (m − M)0 = 24.4 (Bernard et al. 2010).
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