Notes. Description of the columns: (1) and (2) source coordinates (J2000) extracted from FIRST; (3) redshift as measured from the SDSS; (4) FIRST peak flux density; (5) uncertainty of the FIRST peak flux; (6) FIRST observation time; (7) NVSS integrated flux density; (8) uncertainty of the NVSS integrated flux density; (9) NVSS observation time; (10) “traditional” balnicity index selection flag, “1” means BI > 0 (Gibson et al. 2009); (11) modified balnicity index selection flag, “1” means the value is larger than 0 (Gibson et al. 2009); (12) radio-loudness, the radio-to-optical (i-band) ratio of the quasar core (Kimball et al. 2011b), which were calculated from z, S_{1.4 GHz}, M_i taken from Schneider et al. (2007), and the assumption of a radio core spectral index of 0 and an optical spectral index of −0.5; (13) lower limit of the brightness temperature calculated using Eq. (A.7); (14) minimum Doppler factor calculated using the equipartition brightness temperature value of 10¹¹ K; (15) maximum viewing angles estimated as described in the Appendix using the value of δ₁; (16) minimum Doppler factor calculated using the inverse Compton brightness temperature value of 10¹² K; (17) maximum viewing angles estimated as described in the Appendix using the value of δ₂.