Table 2.
Fit parameters for the unknown AGNs (phenomenological jet model with accretion disk) identified as blazars.
| Source | CD | νLS | a1 | a2 | a3 | νs | νc | νcut, s | νcut, c | νt | ar | ṁ | MBH | RT | θT | lEdd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| SWIFT J0131.5−1007 | 25.00 | 7.00E+45 | 0.20 | 1.60 | 0.00 | 5.0E+12 | 5.0E+19 | 1.0E+15 | 1.0E+25 | 1.0E+11 | 0.10 | 1.00 | 2.50E+09 | 1.20 | 0.20 | 0.015 |
| SWIFT J0144.8−2754 | 10.00 | 1.00E+46 | 0.55 | 1.60 | 0.50 | 1.0E+13 | 5.0E+21 | 5.0E+15 | 5.0E+25 | 1.0E+11 | 0.00 | 1.50 | 1.00E+09 | 2.40 | 0.79 | 0.055 |
| SWIFT J0201.0+0329 | 10.00 | 2.00E+45 | 0.40 | 1.80 | 0.20 | 5.0E+12 | 2.0E+20 | 1.0E+15 | 1.0E+24 | 1.0E+11 | −0.10 | 0.25 | 1.50E+09 | 0.58 | 0.60 | 0.006 |
| SWIFT J1756.3+5237 | 0.30 | 3.00E+44 | 0.50 | 1.60 | 0.10 | 4.0E+13 | 1.0E+19 | 1.0E+16 | 1.0E+24 | 1.0E+11 | 0.10 | – | – | – | – | – |
| SWIFT J1810.0−6554 | 10.00 | 1.00E+44 | 0.30 | 1.60 | 0.60 | 2.0E+13 | 5.0E+20 | 1.0E+16 | 1.0E+25 | 1.0E+11 | 0.00 | – | – | – | – | – |
Notes. We only found the emission signature of an accretion disk in the first three objects. The meanings of the parameters used are as follows: CD Compton dominance ratio; νLS synchrotron peak luminosity in νL(ν) in erg s−1; a1, a2, a3 power-law slopes; νS synchrotron peak frequency in Hz; νC inverse-Compton peak frequency in Hz; νcut, S, νcut, C cutoff frequencies for low- and high-energy spectra in Hz; νT self-absorption frequency in Hz; ar power-law slope for ν < νT; ṁ accretion ratio in units of M⊙ yr−1; MBH black hole mass in M⊙; lEdd accretion disk Eddington ratio; RT obscuring torus radius in parsec; and θT obscuring torus covering angle.
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