Fig. 5.
Stellar mass (X-axis) vs. star formation rate tracer SFR2800 Å (Y-axis) defined by Madau et al. (1998, see Eq. (8)) of ALHAMBRA galaxies at redshift 0.3 ≤ z < 0.5 (left panel) and 0.5 ≤ z < 0.7 (right panel). High densities are presented in green, and lower densities in blue. The dashed and solid red lines show the fit to the quiescent sequence and the limiting SFR2800 Å values for star-forming galaxies, respectively. The yellow markers illustrate galaxies labelled as dusty star-forming galaxies by the rest-frame stellar mass–colour diagram corrected for extinction (MCDE).
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