Fig. 3.
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Observed-frame optical spectra obtained with Subaru/FOCAS, HET/LRS2, and Keck/LRIS of the newly confirmed quasars sorted on spectroscopic redshift. The total flux measurements at 144 MHz are also indicated on the left hand side of each spectrum. The detected emission lines are indicated by the grey dashed lines, which are Lyα+N V emission lines unless indicated otherwise.
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