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Table 10.

0.1–100 GeV Fermi-LAT results on MOJAVE γ-ray radio galaxies.

Source Name Redshift Flux (a) Spectral index (b) Curvature (c) TS Ref. (d)
0055+300 NGC 315 0.0165 (5.5 ± 1.3)×10−9 2.29 ± 0.11 * 77.3 [2]
0305+039 3C 78 0.0287 (7.0 ± 1.0)×10−9 1.96 ± 0.07 * 385 [1]
0309+411 NRAO 128 0.136 (5.7 ± 1.7)×10−9 2.29 ± 0.13 * 53.6 [2]
0316+413 3C 84 0.018 (3.36 ± 0.04)×10−7 2.006 ± 0.008 0.060 ± 0.004 9.63 × 104 [1]
0415+379 3C 111 0.0491 (3.4 ± 0.3)×10−8 2.75 ± 0.07 * 186 [1]
0430+052 3C 120 0.033 (2.8 ± 0.3)×10−8 2.70 ± 0.06 * 226 [1]
1128−047 PKS 1128−047 0.27 (7.6 ± 1.3)×10−9 2.46 ± 0.10 * 58.9 [2]
1228+126 M 87 0.00436 (1.9 ± 0.2)×10−8 2.08 ± 0.04 * 1410 [2]
1514+004 PKS 1514+00 0.052 (8.8 ± 1.6)×10−9 2.46 ± 0.10 * 82.3 [2]
1637+826 NGC 6251 0.0247 (2.2 ± 0.2)×10−8 2.28 ± 0.04 0.09 ± 0.02 1610 [2]

Notes. Sources reported as LAT detections here for the first time are highlighted in italic.

(a)

Fermi-LAT flux between 0.1 and 100 GeV in photons cm−2 s−1.

(b)

Fermi-LAT spectral index Γ, in case of power-law spectrum dN/dE = N0 × (E/E0)−Γ, or α in case of logParabola spectrum dN/dE = N0 × (E/Eb)−[α + βlog(E/Eb)].

(c)

Curvature parameter of logParabola spectrum β.

References.

(d)

MOJAVE reference paper for the VLBI results: [1] Lister et al. (2013); [2] Lister et al. (2016).

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