Table A.2.
Sample of Type 1 AGNs used in this work.
| Source name | Log νp | Log νpLνp | Log MBH, fit | λEdd, FIT | σ | FWHM | τLT | Log VPσ | Log VPfwhm | L5100 Å | L1350 Å | Log MBH, Hβ | Log MBH, CIV |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [Hz] | [erg s−1] | [M⊙] | [km s−1] | [km s−1] | [lt. days] | [M⊙] | [M⊙] | [erg s−1] | [erg s−1] | [M⊙] | [M⊙] | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
| 3C 273 (a) | 15.42 | 46.39 | 9.175 ± 0.450 | 0.26 ± 0.12 | – | 2742 ± 58 |
 |
– |
 |
45.810 | – | 8.691 | – |
| (b) | 1777 ± 150 | 2598 ± 299 |
 |
 |
 |
45.960 | – | 8.719 | – | ||||
| Ark 120 (a) | 15.28 | 44.52 | 8.520 ± 0.450 | 0.016 ± 0.007 | – | 5850 ± 480 |
 |
– |
 |
44.140 | – | 8.514 | – |
| (b) | 1959 ± 109 | 5536 ± 297 |
 |
 |
 |
44.230 | – | 8.511 | – | ||||
| (b) | 1884 ± 48 | 5284 ± 203 |
 |
 |
 |
44.230 | – | 8.471 | – | ||||
| Fairall 9 (a) | 15.42 | 44.60 | 8.280 ± 0.450 | 0.033 ± 0.015 | – | 5900 ± 650 |
 |
– |
 |
44.140 | – | 8.522 | – |
| (b) | 3787 ± 197 | 6901 ± 707 |
 |
 |
 |
44.250 | – | 8.713 | – | ||||
| MRK 142 (d) | 15.40 | 43.92 | 7.980 ± 0.450 | 0.014 ± 0.006 | 859 ± 102 | 1368 ± 379 |
 |
 |
 |
43.540 | – | 6.952 | – |
| (e) | – | 1647 ± 69 |
 |
– |
 |
43.520 | – | 7.103 | – | ||||
| MRK 290 (g) | 15.41 | 43.95 | 7.975 ± 0.450 | 0.015 ± 0.007 | 1606 ± 47 | 4270 ± 157 |
 |
 |
 |
43.110 | – | 7.726 | – |
| MRK 335 (a) | 15.32 | 44.22 | 8.290 ± 0.450 | 0.014 ± 0.006 | – | 1260 ± 120 |
 |
– |
 |
43.790 | – | 7.006 | – |
| (b) | 917 ± 52 | 1629 ± 145 |
 |
 |
 |
43.860 | – | 7.264 | – | ||||
| (b) | 948 ± 113 | 1375 ± 357 |
 |
 |
 |
43.860 | – | 7.117 | – | ||||
| (c) | 1293 ± 64 | 1025 ± 35 |
 |
 |
 |
43.700 | – | 6.781 | – | ||||
| (e) | – | 1997 ± 265 |
 |
– |
 |
43.640 | – | 7.331 | – | ||||
| MRK 509 (a) | 15.35 | 44.68 | 8.460 ± 0.450 | 0.026 ± 0.012 | – | 2860 ± 120 |
 |
– |
 |
44.170 | – | 7.908 | – |
| (b) | 1276 ± 28 | 2715 ± 101 |
 |
 |
 |
44.280 | – | 7.918 | – | ||||
| MRK 590 (a) | 15.50 | 43.18 | 7.410 ± 0.450 | 0.009 ± 0.004 | – | 2170 ± 120 |
 |
– |
 |
43.710 | – | 7.438 | – |
| (b) | 789 ± 74 | 1675 ± 587 |
 |
 |
 |
43.810 | – | 7.263 | – | ||||
| (b) | 1935 ± 52 | 2566 ± 106 |
 |
 |
 |
43.810 | – | 7.634 | – | ||||
| (b) | 1251 ± 72 | 2115 ± 575 |
 |
 |
 |
43.810 | – | 7.466 | – | ||||
| (b) | 1201 ± 130 | 1979 ± 386 |
 |
 |
 |
43.810 | – | 7.408 | – | ||||
| MRK 877 (a) | 15.20 | 44.91 | 8.875 ± 0.450 | 0.017 ± 0.008 | – | 3880 ± 650 |
 |
– |
 |
44.370 | – | 8.273 | – |
| (b) | 2626 ± 211 | 4718 ± 991 |
 |
 |
 |
44.480 | – | 8.498 | – | ||||
| MRK 1044 (e) | 15.50 | 43.39 | 7.515 ± 0.450 | 0.012 ± 0.006 | – | 1211 ± 48 |
 |
– |
 |
43.050 | – | 6.601 | – |
| MRK 1383 (b) | 15.56 | 45.32 | 8.360 ± 0.450 | 0.145 ± 0.067 | 3442 ± 308 | 6323 ± 1295 |
 |
 |
 |
44.720 | – | 8.872 | – |
| MRK 1501 (c) | 15.34 | 44.69 | 8.485 ± 0.450 | 0.026 ± 0.012 | 3321 ± 107 | 5054 ± 145 |
 |
 |
 |
44.320 | – | 8.477 | – |
| NGC 3783 (a) | 15.40 | 43.64 | 7.840 ± 0.450 | 0.010 ± 0.005 | – | 4100 ± 1160 |
 |
– |
 |
43.250 | – | 7.761 | – |
| (b) | 1753 ± 141 | 3093 ± 529 |
 |
 |
 |
43.260 | – | 7.521 | – | ||||
| NGC 4151 (a) | 15.20 | 42.35 | 7.595 ± 0.450 | 0.001 ± 0.000 | – | 5230 ± 920 |
 |
– |
 |
42.860 | – | 7.777 | – |
| (b) | 1914 ± 42 | 4248 ± 516 |
 |
 |
 |
42.880 | – | 7.606 | – | ||||
| NGC 5548 (a) | 15.33 | 43.52 | 7.920 ± 0.450 | 0.006 ± 0.003 | – | 5500 ± 400 |
 |
– |
 |
43.430 | – | 8.106 | – |
| (b) | 1687 ± 56 | 4044 ± 199 |
 |
 |
 |
43.510 | – | 7.879 | – | ||||
| (b) | 2026 ± 68 | 5706 ± 357 |
 |
 |
 |
43.510 | – | 8.178 | – | ||||
| (d) | 4270 ± 292 | 11177 ± 2266 |
 |
 |
 |
42.620 | – | 8.317 | – | ||||
| (g) | 1822 ± 35 | 4849 ± 112 |
 |
 |
 |
42.660 | – | 7.611 | – | ||||
| NGC 7469 (a) | 15.40 | 43.69 | 7.865 ± 0.450 | 0.011 ± 0.005 | – | 3220 ± 1580 |
 |
– |
 |
43.740 | – | 7.796 | – |
| (b) | 1456 ± 207 | 2169 ± 459 |
 |
 |
 |
43.720 | – | 7.443 | – | ||||
| (e) | – | 1722 ± 30 |
 |
– |
 |
43.560 | – | 7.162 | – | ||||
| PG 0026+129 (a) | 15.47 | 45.31 | 8.535 ± 0.450 | 0.095 ± 0.044 | – | 1358 ± 91 |
 |
– |
 |
44.850 | – | 7.601 | – |
| (b) | 1773 ± 285 | 1719 ± 495 |
 |
 |
 |
45.020 | – | 7.891 | – | ||||
| (e) | – | 2544 ± 56 |
 |
– |
 |
44.840 | – | 8.141 | – | ||||
| PG 0052+251 (a) | 15.35 | 45.40 | 8.820 ± 0.450 | 0.060 ± 0.028 | – | 4550 ± 270 |
 |
– |
 |
44.810 | – | 8.631 | – |
| (b) | 1783 ± 86 | 4165 ± 381 |
 |
 |
 |
44.960 | – | 8.629 | – | ||||
| PG 0804+761 (a) | 15.40 | 45.34 | 8.690 ± 0.450 | 0.071 ± 0.033 | – | 2430 ± 42 |
 |
– |
 |
44.820 | – | 8.091 | – |
| (b) | 1971 ± 105 | 2012 ± 845 |
 |
 |
 |
44.940 | – | 7.987 | – | ||||
| PG 0844+349 (a) | 15.44 | 45.00 | 8.440 ± 0.450 | 0.058 ± 0.027 | – | 2830 ± 120 |
 |
– |
 |
44.240 | – | 7.934 | – |
| (b) | 1448 ± 79 | 2148 ± 612 |
 |
 |
 |
44.350 | – | 7.749 | – | ||||
| (e) | – | 2694 ± 58 |
 |
– |
 |
44.150 | – | 7.846 | – | ||||
| PG 0953+414 (a) | 15.45 | 45.88 | 8.860 ± 0.450 | 0.167 ± 0.077 | – | 2723 ± 62 |
 |
– |
 |
45.080 | – | 8.320 | – |
| (b) | 1306 ± 144 | 3002 ± 398 |
 |
 |
 |
45.220 | – | 8.475 | – | ||||
| PG 1211+143 (a) | 15.37 | 45.20 | 8.680 ± 0.450 | 0.053 ± 0.024 | – | 1479 ± 66 |
 |
– |
 |
44.690 | – | 7.595 | – |
| (b) | 1080 ± 102 | 1317 ± 138 |
 |
 |
 |
44.750 | – | 7.524 | – | ||||
| (e) | – | 2012 ± 37 |
 |
– |
 |
44.660 | – | 7.847 | – | ||||
| PG 1247+267 (h) | 15.39 | 47.58 | 9.830 ± 0.450 | 0.895 ± 0.414 | 2104 ± 540 | 4568 ± 1338 |
 |
 |
 |
– | 47.590 | – | 9.882 |
| PG 1307+085 (a) | 15.55 | 45.38 | 8.410 ± 0.450 | 0.148 ± 0.069 | – | 5260 ± 270 |
 |
– |
 |
44.720 | – | 8.712 | – |
| (b) | 1820 ± 122 | 5058 ± 524 |
 |
 |
 |
44.880 | – | 8.758 | – | ||||
| PG 1411+442 (a) | 15.24 | 44.90 | 8.790 ± 0.450 | 0.020 ± 0.009 | – | 2740 ± 110 |
 |
– |
 |
44.510 | – | 8.040 | – |
| (b) | 1607 ± 169 | 2398 ± 353 |
 |
 |
 |
44.630 | – | 7.985 | – | ||||
| PG 1700+518 (a) | 15.04 | 45.65 | 9.565 ± 0.450 | 0.019 ± 0.009 | – | 1970 ± 150 |
 |
– |
 |
45.430 | – | 8.214 | – |
| (b) | 1700 ± 123 | 1846 ± 682 |
 |
 |
 |
45.630 | – | 8.257 | – | ||||
| (e) | – | 2252 ± 85 |
 |
– |
 |
45.440 | – | 8.335 | – | ||||
| PG 2130+099 (a) | 15.39 | 44.70 | 8.390 ± 0.450 | 0.032 ± 0.015 | – | 3010 ± 180 |
 |
– |
 |
44.330 | – | 8.032 | – |
| (b) | 1623 ± 86 | 2912 ± 231 |
 |
 |
 |
44.460 | – | 8.068 | – | ||||
| (c) | 1825 ± 65 | 2097 ± 102 |
 |
 |
 |
44.150 | – | 7.628 | – | ||||
| (e) | – | 2450 ± 188 |
 |
– |
 |
44.130 | – | 7.753 | – | ||||
| S5 0836+71 (i) | 15.46 | 47.22 | 9.510 ± 0.450 | 0.816 ± 0.377 | – | 9700 ± 0 |
 |
– |
 |
– | 47.050 | – | 10.250 |
Notes. (1) Name of the sources. (2) and (3) Logarithmic value of the spectrum peak frequency νp in Hz and luminosity νpLνp in erg s−1 inferred from the SED fitting procedure. (4) and (5) BH mass in solar masses and Eddington ratio λEdd computed from the SED fitting procedure; the mean uncertainties are connected to different quantities (i.e., BH spin, viewing angle, uncertainty on the spectrum peak position). (6) and (7) velocity dispersion and FWHM in km s−1 related to the Hβ line (for PG 1247+267 and S5 0836+71, these measurements are related to the CIV line). (8) Light travel time in the rest-frame expressed in days. (9) and (10) Logarithmic value of the VP in solar masses computed using the velocity dispersion and the FWHM; the uncertainties are connected to τLT and σline (or FWHM); the systematic uncertainty is ∼0.5 dex (Peterson 2010). (11) and (12) Continuum luminosity at 5100 Å and 1350 Å in erg s−1 as reported in the corresponding reference paper. (13) and (14) Logarithmic value of the BH mass in solar masses computed using the Hβ (CIV) line FWHM and the luminosity at 5100 Å (1350 Å) as reported in the reference paper, through the SE relations described in Vestergaard & Peterson (2006). SE BH mass estimates have a systematic uncertainty of ∼0.5 dex (VesterOs). When a lower error is absent, it means that for that source only an upper limit is present.
References. (a)from Kaspi et al. (2000); (b)from Peterson et al. (2004); (c)from Grier et al. (2012); (d)from Bentz et al. (2009); (e)from Wang et al. (2014); (f)from Bentz et al. (2014); (g)from Denney et al. (2010); (h)from Trevese et al. (2014); (i)from Kaspi et al. (2007).
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