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Table 3

Physical quantities associated to the source quasar.

Object Pair Line FWHM (Å) log (MBH/M) L/LEdd RBLR/RE

(a) HE 0047-1756 A-B Mg II 46.3 46.3 4145  ±  365 8.86  ±  0.23 0.23  ±  0.13 17.74  ±  0.54 9.53
(b) Q0142-100 A-B C IV 47.4 47.4 (4750  ±  220) (9.51  ±  0.3)3 0.58  ±  0.45 18.28  ±  0.76 35.85
(c) SDSS J0246-0825 A-B Mg II 46.0 45.8 3700  ±  670 8.59  ±  0.36 0.17  ±  0.15 17.57  ±  0.85 9.00
(d) HE 0435-1223 B-D Mg II 45.7 46.0 4930  ±  195 8.76  ±  0.44 0.11  ±  0.11 17.50  ±  1.00 5.67
(e) SDSS J0806+2006 A-B Mg II 45.8 46.0 3370  ±  430 8.53  ±  0.35 0.20  ±  0.17 17.59  ±  0.81 8.34
(f) FBQ 0951+2635 A-B Mg II 46.5 46.6 5850  ±  133 9.21  ±  0.26 0.18  ±  0.11 17.80  ±  0.59 9.04
(g) BRI 0952-0115 A-B C IV 46.2 46.5 (5210  ±  1300) (9.14  ±  0.40) 0.14  ±  0.13 17.83  ±  0.95 16.07
(h) SDSS J1138+0314 B-C C IV 45.5 45.3 (1990  ±  180) (7.69  ±  0.33) 0.43  ±  0.36 17.22  ±  0.77 2.92
(i) J1226-0006 A-B Mg II 45.8 45.5 7840  ±  550 8.96  ±  0.43 0.04  ±  0.04 17.30  ±  0.99 4.54
(j) SDSS J1335+0118 A-B Mg II 46.4 46.5 6110  ±  205 9.19  ±  0.26 0.15  ±  0.10 17.74  ±  0.61 9.92
(k) Q1355-2257 A-B Mg II 46.5 46.3 5035  ±  140 9.04  ±  0.34 0.19  ±  0.16 17.76  ±  0.79 14.89
(l) WFI 2033-4723 B-C Mg II 46.0 45.8 3960  ±  465 8.63  ±  0.35 0.15  ±  0.13 17.56  ±  0.81 8.25
(m) HE 2149-2745 A-B C IV 46.0 46.0 (7470  ±  1865) (9.82  ±  0.40) 0.01  ±  0.01 18.20  ±  0.95 32.47

(n) J0924+0219 A Mg II 44.7 - 3660  ±  310 7.93  ±  0.34 0.04  ±  0.03 16.93  ±  0.78 1.45
(o) J1131-1231 B Mg II 45.0 - 5630  ±  165 8.32  ±  0.62 0.03  ±  0.04 16.94  ±  1.42 1.89
B H β 45.0 - 4545  ±  255 7.90  ±  0.60 0.07  ±  0.10 16.71  ±  1.37 1.12
(p) H1413+117 AB H β 46.7 - 5170  ±  250 9.12  ±  0.01 0.28  ±  0.06 17.82  ±  0.05 17.76
(q) Q2237+0305 D Mg II 46.5 - 2900  ±  565 8.68  ±  0.36 0.44  ±  0.39 17.88  ±  0.86 4.06
C-D C IV 46.1 - (3780  ±  120) (8.63  ±  0.32) 0.25  ±  0.19 17.60  ±  0.74 2.13

Notes. Values in parentheses are from Peng et al. (2006b) and Assef et al. (2011). The last four systems under the horizontal line are part of the extended sample which gather data from literature (Sect. 2.3).

(†)

Lower limit, see Appendix A of Assef et al. (2011);

(‡)

the redshift of this object is unsecure (Kneib et al. 1998; Goicoechea & Shalyapin 2010) and we used zl = 1.0.

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