The B3-VLA CSS sample - VIII. New optical identifications from the Sloan Digital Sky Survey The ultraviolet-optical spectral energy distribution of the young radio sources

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Fig. 3

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Comparison between photometric and spectroscopic redshifts. The two very discrepant large error objects are 0744+464 and 1314+453A. The central line is for z_ph2 = z_sp/1.23, (see text) the two others represent the data dispersion.

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