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Fig. 5.


SFR estimates from SED fitting and from [OII] (derived from Eq. (4) of Kewley et al. 2004) of the galaxies in our spectroscopic sample at 0.8 <  z <  0.9. Red circles show the dust uncorrected Hα derived star formation rates for the galaxies in our sample and that were measured by Sobral et al. (2011). The subscript corr denotes the dust-corrected SFRs derived from each estimate using the optical depth derived through SED fitting (see Sect. 3.2).

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