Fig. 20

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H II regions LF for each galaxy in the PHANGS-MUSE sample. Only objects satisfying the selection described in Sect. 7.4 have been used to compute the LF. The black dashed lines represent the observed LF, the blue dotted lines represent the LF from S22, the red line is the fit obtained from our data, and finally, the black vertical line is the low luminosity cut (Lmin). Only regions with L>Lmin are considered when fitting the LF.
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