Galaxy evolution and star formation efficiency at 0.2 < z < 0.6

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Fig. 10

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The star formation rate (SFR) obtained from the far infrared luminosity, versus the stellar mass of galaxies in our sample (full black circles), compared to the sample of Da Cunha et al. (2010, full red squares) and Fiolet et al. (2009, full green triangles).

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