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Fig. 6


Evolution of the physical properties of the BJGKn< 6 samples. The panels show the median of the probability distribution of (top to bottom and left to right) the specific star formation rate, star formation rate, age, B-band luminosity, K-band luminosity, and stellar mass. Red squares show the evolution of BJGKn< 6 galaxies brighter than K = −21.2. The colored areas represent the dispersion of each sample. The error bars correspond to the median error of the physical properties determined by the iSEDfit. Dashed lines show the fit to the CANDELS analysis taken from van Dokkum et al. (2013) for galaxies of stellar masses similar to the Milky Way.

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