Table 2
Model parameter for the spectral energy density in the two assumptions of a blob dissipating just beyond the BLR (Rdiss = 0.2 pc, model a) or far away from the SMBH (Rdiss = 6.8 pc, model b).
| Model | a | b |
|---|---|---|
| Rdiss (pc) | 0.29 | 6.8 |
| Blob radius (cm) | 7.7 × 1016 | 1.4 × 1017 |
| Ld (erg s−1) | 1.5 × 1046 | |
| RBLR (pc) | 0.13 | |
| RTorus (pc) | 3.24 | |
| fBLR | 0.1 | |
| fTorus | 0.3 | |
 (cm) |
6 × 1014 | |
| Γbulk | 20 | 30 |
| Angle of view (deg) | 2 | 2 |
| γmin | 1 | 1 |
| γmax | 6.1 × 103 | 1.5 × 104 |
| γbreak | 0.95 × 103 | 2.00 × 103 |
| Density at γbreak (cm−3) | 3.9 × 10−2 | 2.0 × 10−3 |
| s1 | 1.1 | 1.5 |
| s2 | 3.5 | 3.5 |
| B (G) | 4.6 × 10−1 | 4.3 × 10−2 |
Notes. The parameter fBLR is the fraction of the disk luminosity that is reprocessed by the BLR and re-emitted as broad emission lines, fTorus is the fraction of the disk luminosity that is reprocessed by the dusty torus, ϵaccr is the accretion efficiency, and RS is the Schwarzschild radius of the SMBH.
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