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Table A.1

CJF sources detected in the γ-ray regime by Fermi-LAT.

Source Type z Fγ δ Fγ αγ δ αγ log (νLν)γ δlog (νLν)γ Var
(10-9phcm-2s-1) (ergs-1)
0003+380 G(Q) 0.229 0.6 0.3 2.86 0.13 44.57 0.22 N 4.899 0
0110+495 Q 0.389 0.7 0.3 2.29 0.18 45.33 0.19 N 1.049 0.646
0133+476 Q 0.859 9.6 0.6 2.34 0.03 47.33 0.03 Y 10.986 2.817
0212+735 Q 2.367 1 0.4 2.85 0.13 47.63 0.17 Y 16.068 7.121
0218+357 G(Q) 0.936 6.4 0.5 2.33 0.04 47.25 0.03 Y n/a n/a
0219+428 BL 0.444 24.9 1 1.93 0.02 47.15 0.02 Y 14.04 5.03
0227+403 Q 1.019 1.4 0.3 2.43 0.13 46.68 0.09 Y 4.013 1.07
0307+380 Q 0.816 0.6 0.3 2.49 0.15 46.05 0.22 Y 4.283 0
0316+413 G 0.018 17.3 0.8 2.13 0.02 43.89 0.02 Y 0.978 0.204
0346+800 Q(?) n/a 2 0.3 2.5 0.08 n/a n/a Y n/a n/a
0621+446 BL n/a 1 0.3 2.03 0.18 n/a n/a N n/a n/a
0633+734 Q 1.85 0.6 0.3 2.73 0.17 47.06 0.22 N 21.673 1.036
0650+453 Q 0.933 6.1 0.5 2.32 0.04 47.23 0.04 Y n/a n/a
0707+476 Q(BL) 1.292 0.9 0.3 2.51 0.13 46.77 0.14 N 4.248 4.439
0716+714 BL 0.31 13.1 0.7 2.15 0.03 46.38 0.02 Y n/a n/a
0749+540 BL n/a 1.2 0.3 1.95 0.16 n/a n/a N n/a n/a
0800+618 Q 3.044 0.6 0.2 2.83 0.13 47.74 0.14 Y 10.003 9.591
0814+425 BL 0.53 8.7 0.6 2.15 0.04 46.01 0.03 Y 2.72 1.834
0820+560 Q 1.409 0.9 0.3 2.87 0.11 46.91 0.14 Y 5.311 0
0836+710 Q 2.18 1.2 0.3 2.98 0.12 47.64 0.11 N 30.59 4.457
0917+449 Q 2.18 14 0.7 2.28 0.02 48.58 0.02 Y 14.246 5.506
0917+624 Q 1.446 1.1 0.3 2.7 0.15 47.01 0.12 N 3.214 1.026
0925+504 BL 0.37 0.7 0.2 1.91 0.23 45.43 0.12 N n/a n/a
0954+556 Q 0.895 10.5 0.6 2.05 0.03 47.50 0.02 N n/a n/a
0954+658 BL 0.368 0.5 0.3 2.51 0.16 45.06 0.26 N 9.874 0
1015+359 Q 1.226 0.5 0.2 2.71 0.15 46.46 0.17 N 10.273 1.59
1020+400 Q 1.254 0.6 0.2 2.45 0.17 46.56 0.14 N 13.169 5.094
1030+415 Q 1.12 1.1 0.3 2.48 0.12 46.69 0.12 N 4.186 2.408
1030+611 Q 1.401 2.2 0.3 2.46 0.08 45.74 0.06 Y 1.879 1.817
1039+811 Q 1.254 0.9 0.2 2.95 0.13 46.77 0.10 Y 10.125 1.553
1044+719 Q 1.15 1.6 0.3 2.47 0.13 46.88 0.08 N 3.039 0.643
1101+384 BL 0.031 26.1 1 1.81 0.02 44.73 0.02 Y 0.187 0.066
1144+402 Q 1.088 1 0.3 2.47 0.13 46.61 0.13 N n/a n/a
1206+415 BL n/a 0.5 0.2 1.85 0.22 n/a n/a N n/a n/a
1221+809 BL n/a 1 0.3 2.27 0.14 n/a n/a N n/a n/a
1246+586 BL n/a 4.5 0.4 2.18 0.06 n/a n/a N n/a n/a
1250+532 BL n/a 3 0.4 2.14 0.07 n/a n/a N n/a n/a
1306+360 Q 1.055 2.2 0.3 2.3 0.09 46.93 0.06 Y 4.611 0
1322+835 na 1.024 0.5 0.2 2.49 0.22 46.24 0.17 N n/a n/a
1357+769 BL(Q) n/a 1.1 0.2 2.25 0.16 n/a n/a N n/a n/a
1418+546 BL 0.151 0.9 0.2 2.77 0.17 44.34 0.10 N 2.562 0
1432+422 Q 1.24 0.7 0.2 2.25 0.2 46.63 0.12 N 17.69 0.678
1504+377 G(Q) 0.672 0.7 0.2 2.59 0.13 45.87 0.12 Y 10.547 1.655
1633+382 Q 1.807 6.8 0.5 2.47 0.04 48.05 0.03 Y 12.18 4.951
1641+399 Q 0.595 5.6 0.5 2.49 0.04 46.65 0.04 Y 6.114 0
1652+398 BL 0.034 8.3 0.6 1.85 0.04 44.29 0.03 Y 0.898 0
1700+685 G(Q) 0.301 3.7 0.4 2.28 0.06 45.78 0.05 Y 1.037 1.131
1722+401 Q(G) 1.049 2.9 0.4 2.37 0.07 47.04 0.06 Y 20.883 10.441
1726+455 Q 0.717 1.2 0.3 2.57 0.09 46.19 0.11 Y 5.686 0.812
1732+389 Q 0.97 6 0.5 2.22 0.05 47.29 0.04 Y 12.065 1.805
1739+522 Q 1.381 3.4 0.4 2.71 0.05 47.44 0.05 Y 11.475 9.021
1749+701 BL 0.77 2 0.3 2.05 0.1 46.60 0.07 N 14.805 4.992
1747+433 BL n/a 2.3 0.3 2.12 0.09 n/a n/a N n/a n/a
1803+784 BL 0.68 3 0.4 2.35 0.07 46.56 0.06 Y 13.567 2.993
1807+698 BL 0.051 1.9 0.3 2.6 0.08 43.67 0.07 N 0.398 0
1823+568 BL 0.664 2.7 0.4 2.34 0.07 46.49 0.06 Y 8.994 1.524
1849+670 Q 0.657 13.3 0.7 2.25 0.03 47.19 0.02 Y 8.65 0.567
1851+488 Q 1.25 0.9 0.3 2.6 0.12 46.73 0.14 N n/a n/a
2007+777 BL 0.342 1.4 0.3 2.42 0.16 45.45 0.09 N 1.953 0.849
2010+723 BL n/a 1.6 0.4 2.45 0.15 n/a n/a N n/a n/a
2023+760 BL n/a 1.1 0.3 2.52 0.18 n/a n/a N n/a n/a
2200+420 BL 0.069 7.1 0.6 2.38 0.04 44.59 0.04 Y 3.15 0.305

Notes. Columns (1)–(3) give the IAU name, type, and redshift of the source. In parentheses we give the alternative classification from the Fermi-LAT team, where applicable. Column (4) gives the γ-ray flux (detections are from the first Fermi-LAT catalog, Abdo et al. 2010a), Col. (5) gives the uncertainty for the γ-ray fluxes, Cols. (6) and (7) give the γ photon index and its uncertainty, Cols. (8) and (9) give the calculated γ-ray luminosity (in the log νLν form and in logarithmic scale) and the respective uncertainty, Col. (10) denotes sources with detected variability in γ-rays, and Cols. (11) and (12) show the maximum apparent jet speed for that source and its uncertainty.

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