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Fig. 3.

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SFR (mean of Hα and UV-based values) as a function of the stellar mass for galaxies in the RPS sample (orange diamonds), galaxies in the Virgo cluster region (within 10° from M 87, green circles) and galaxies outside of the cluster (blue circles). For comparison, we show the star-forming main sequence for Virgo cluster galaxies with normal H I content (Boselli et al. 2023b, gray line).

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