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Table 8.

γ-ray properties of Fermi-LAT detected TANAMI radio galaxies in the same energy range of the 3FGL, over 103 months of data.

Source Class Fermi-LAT name Flux (a) Spectral index (b) Curvature (c) TS
0518−458 FR II 3FGL J0519.2−4542 (4.69 ± 0.68)×10−10 2.71 ± 0.21 * 104.5
0521−365 RG/BLL 3FGL J0522.9−3628 (4.32 ± 0.14)×10−9 2.84 ± 0.20 −0.04 ± 0.04 3523.5
0625−354 FR I/BLL 3FGL J0627.0−3529 (1.41 ± 0.09)×10−9 1.90 ± 0.06 * 938.6
1322−428 FR I 3FGL J1325.4−4301 (3.46 ± 0.14)×10−9 2.46 ± 0.05 * 1775.7
1343−601 FR I 3FGL J1346.6−6027 (2.06 ± 0.17)×10−9 2.48 ± 0.09 * 264.3

Notes.

(a)

Fermi-LAT flux between 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.

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