Fig. 8.
LIR, SF vs. LX[2−10 keV] of the XQSOs separated in four redshift bins, color-coded by their median 1.4 GHz radio luminosity. The upper and lower panels show XQSOs from the COSMOS and XXL-S fields, respectively. Lines show the mean value of LIR, SF in different redshift bins, as indicated in legend. We note that the two color-coded bars correspond to very different ranges in L1.4 GHz in COSMOS and XXL-S.
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