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Fig. 10.
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Distribution of the metallicity derived using the calibration of Curti et al. (2017) using the Hβ, [OIII], [NII], and Hα lines with an S/N > 5 from the MUSE data for the galaxies NGC 4469 (left) and NGC 4526 (right). The white cross shows the position of the photometric centre.
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