Gamma-ray emission in radio galaxies under the VLBI scope - I. Parsec-scale jet kinematics and high-energy properties of γ-ray-detected TANAMI radio galaxies

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Volume 627 (July 2019)

A&A, 627 (2019) A148

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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/E_b)^{−[α + βlog(E/E_b)]}.

^(c)

Curvature parameter of logParabola spectrum β.

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