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Fig. 5.

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STARLIGHT fits (shown by blue lines) are applied to the MUSE spectra (represented in black, with yellow lines indicating masked data) along with S-PLUS photometry fits (depicted with black and red circles, depending on whether they were used in the fit, with red points marking the masked data, and cyan points for the S-PLUS photometric data fitted by STARLIGHT). Vertical dashed lines indicate the position of the stellar features labeled in the top panels.

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