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Fig. 4.

image

Stellar masses and SFRs derived from SED fitting (see Sect. 3.2) in our spectroscopic sample at 0.8 <  z <  0.9. For comparison, we show the derived best-fit relation for star-forming galaxies computed at z = 0.84 using the equation derived by Whitaker et al. (2012) over a large average volume in the COSMOS field. The vertical dotted line shows the completeness limit of our survey. The dotted contours show the COSMOS2015 (Laigle et al. 2016) distribution of galaxies with 0.8 <  zphot <  0.9 and iAB <  23 from 10% to 95% of the sample in 5% steps. Empty circles highlight the photometric quiescent sample with log10(sSFR) <  − 11.

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