Table 2.
Input parameters used to model the SED.
| Coord. | z | M | Ld | Rdiss | RBLR |  |
B | Γ | θv | γb | γmax | s1 | s2 | Pj |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [1] | [2] | [3] | [4] | [5] | [6] | [7] | [8] | [9] | [10] | [11] | [12] | [13] | [14] | [15] |
| 081333.32+350810.8 | 4.922 | 4e9 | 6.2e46 (0.12) | 1.2e3 (1e3) | 790 | 5e42 | 1.7 | 13 | 5.2 | 150 | 3e3 | 0 | 2.6 | 3.8e46 |
| 4.922 | 4e9 | 6.2e46 (0.12) | 1.2e3 (1e3) | 790 | 5e43 | 1.7 | 13 | 8 | 150 | 3e3 | 0 | 2.6 | 1.6e47 | |
| 085111.59+142337.7 | 4.307 | 4e9 | 3.6e46 (0.07) | 720 (600) | 603 | 4e42 | 1.1 | 13 | 3 | 100 | 4e3 | 0.75 | 2.7 | 3.2e46 |
| 4.307 | 4e9 | 3.6e46 (0.07) | 720 (600) | 603 | 4e43 | 1.3 | 13 | 6 | 100 | 4e3 | 0.75 | 2.7 | 2.9e47 | |
| 103717.72+182303.0 | 4.051 | 1e9 | 2.6e46 (0.20) | 180 (600) | 510 | 2e42 | 7.1 | 13 | 3.5 | 250 | 3e3 | 0 | 2.6 | 1.2e46 |
| 4.051 | 1e9 | 2.6e46 (0.20) | 180 (600) | 510 | 2e43 | 7.1 | 13 | 6 | 250 | 3e3 | 0 | 2.6 | 5.1e46 | |
| 4.051 | 1e9 | 2.6e46 (0.20) | 180 (600) | 510 | 8e43 | 7.1 | 13 | 8 | 250 | 3e3 | 0 | 2.6 | 1.8e47 | |
| 105320.42–001649.7 | 4.304 | 1.5e9 | 5.3e46 (0.27) | 248 (550) | 725 | 4e42 | 3.7 | 13 | 5 | 60 | 4e3 | 0 | 2.6 | 2.6e46 |
| 4.304 | 1.5e9 | 5.3e46 (0.27) | 248 (550) | 725 | 8e42 | 3.7 | 13 | 6 | 60 | 4e3 | 0 | 2.6 | 4.7e46 | |
| 4.304 | 1.5e9 | 5.3e46 (0.27) | 248 (550) | 725 | 5e43 | 3.7 | 13 | 8 | 60 | 4e3 | 0 | 2.6 | 2.7e47 | |
| 123142.17+381658.9 | 4.137 | 7e8 | 1.8e46 (0.2) | 147 (700) | 427 | 3e42 | 4.4 | 11 | 3 | 70 | 3e3 | 0 | 2.6 | 1.1e46 |
| 4.137 | 7e8 | 1.8e46 (0.2) | 147 (700) | 427 | 3e43 | 4.4 | 11 | 6 | 70 | 3e3 | 0 | 2.6 | 9.7e46 | |
| 4.137 | 7e8 | 1.8e46 (0.2) | 147 (700) | 427 | 1e44 | 5.5 | 11 | 8 | 70 | 3e3 | 0 | 2.6 | 3.3e47 | |
| 123503.03–000331.7 | 4.723 | 2e9 | 1.8e46 (0.07) | 660 (1100) | 427 | 1.5e42 | 0.9 | 13 | 3 | 50 | 3e3 | 0 | 2.7 | 9.5e45 |
| 4.723 | 2e9 | 1.8e46 (0.07) | 660 (1100) | 427 | 1.5e43 | 1.2 | 13 | 6 | 50 | 3e3 | 0 | 2.7 | 7.6e46 | |
| 124230.58+542257.3 | 4.730 | 3.5e9 | 3.6e46 (0.08) | 1050 (1000) | 603 | 6e42 | 0.8 | 13 | 6 | 300 | 3e3 | 1 | 2.4 | 4.7e46 |
| 4.730 | 3.5e9 | 3.6e46 (0.08) | 1050 (1000) | 603 | 1e44 | 1.0 | 13 | 10 | 300 | 3e3 | 1 | 2.4 | 5.1e47 | |
| 141209.96+062406.8 | 4.467 | 6e8 | 4.9e46 (0.63) | 216 (1200) | 701 | 3e42 | 4.9 | 11 | 3 | 80 | 3e3 | 1 | 2.6 | 2.5e46 |
| 4.467 | 6e8 | 4.9e46 (0.63) | 216 (1200) | 701 | 7e42 | 5.4 | 10 | 5 | 100 | 3e3 | 1 | 2.6 | 4.1e46 | |
| 165913.23+210115.8 | 4.784 | 2.5e9 | 3.3e46 (0.1) | 450 (600) | 570 | 3e42 | 1.6 | 13 | 3 | 300 | 4e3 | 1 | 2.5 | 1.6e46 |
| 4.784 | 2.5e9 | 3.3e46 (0.1) | 450 (600) | 570 | 2e44 | 1.6 | 13 | 8 | 300 | 4e3 | 1 | 2.5 | 8.7e47 | |
| 231448.71+020151.1 | 4.110 | 1.5e9 | 2.9e46 (0.15) | 225 (500) | 540 | 5e42 | 3.4 | 10 | 3 | 200 | 5e3 | −0.5 | 2.8 | 1.6e46 |
| 4.110 | 1.5e9 | 2.9e46 (0.15) | 225 (500) | 540 | 4e43 | 3.4 | 10 | 6 | 200 | 5e3 | −0.5 | 2.8 | 6.3e46 |
Notes. Column [1] RA and Dec (J2000); Col. [2]: redshift; Col. [3]: black hole mass in solar masses; Col. [4]: accretion disk luminosity, in erg s−1 and (in parenthesis) in units of LEdd; Col. [5]: dissipation radius in units of 1015 cm and (in parenthesis) in units of RS; Col. [6]: size of the BLR in units of 1015 cm. Note that RBLR is a derived quantity, not an independent input parameter, listed for an easy comparison with Rdiss; Col. [7]: power injected in the blob calculated in the comoving frame, in erg s−1; Col. [8]: magnetic field in Gauss; Col. [9]: bulk Lorentz factor at Rdiss; Col. [10]: viewing angle in degrees; Cols. [11] and [12]: break and maximum random Lorentz factors of the injected electrons; Cols. [13] and [14]: slopes of the injected electron distribution [Q(γ)] below and above γb; Col. [15]: total jet power calculated as the sum of all power components (in erg s−1). For all cases, the X-ray corona luminosity LX = 0.3Ld. Its spectral shape is assumed to be ∝ν−1exp(−hν/150 keV).
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