Fig. 10
Normalized histograms of output quantities from MAGPHYS, all derived using the HDF-S and 3D-HST photometry. The values for C III] emitters shown in pink and for the full photometric sample in the redshift range shown in blue. Each value shown is the median of the probability distributions produced by MAGPHYS when marginalizing over all other parameters. Star formation rates and specific star formation rates are averaged over the past 0.1 Gyr.
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