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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 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; 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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