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Fig. 1.
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Spatial distribution and photometric properties of target stars. Left panel: map of the analysed MUSE field. Sources with extracted spectra are marked by red dots. Middle and right panels: (F439W–F569W, F569W) (middle) and (F170W–F569W, F170W) CMDs of NGC 1850 (grey points). Target stars are marked by red dots.
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