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 9.

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

Source	Class	Flux ^(a)	Spectral index ^(b)	Curvature ^(c)	TS
0518−458	FR II	(1.63 ± 0.19)×10⁻⁸	2.63 ± 0.08	*	225.5
0521−365	RG/BLL	(1.17 ± 0.03)×10⁻⁷	2.33 ± 0.02	−0.074 ± 0.011	11313.2
0625−354	FR I/BLL	(1.07 ± 0.10)×10⁻⁸	1.88 ± 0.04	*	1150.4
1322−428	FR I	(1.73 ± 0.04)×10⁻⁷	2.68 ± 0.02	*	7500.0
1343−601	FR I	(6.85 ± 0.66)×10⁻⁸	2.58 ± 0.05	*	416.0
1600−489	MSO	(6.8 ± 0.4)×10⁻⁸	2.06 ± 0.02	*	2771.4
1718−649	GPS/CSO	(5.8 ± 2.2)×10⁻⁹	2.43 ± 0.18	*	44.3

Notes.

^(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/E_b)^{−[α + βlog(E/E_b)]}.

^(c)

Curvature parameter of logParabola spectrum β.

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