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Table 2: Spearman rank correlation test results for the whole sample and AGN subclasses for the log $\nu _{\rm p} L_{\rm p}$ vs. log $\nu _{\rm p}$ -correlation. On the left side is the z-corrected correlation, and on the right side the D-corrected one. Galaxies (GAL) have been omitted due to small sample size.
Table 1: The sample and the observational synchrotron peak frequencies obtained in this work. The values of $\nu _{\rm p}$ listed here have been determined directly from the SEDs and are not corrected for redshift nor for Doppler boosting.