γ-ray emission in radio galaxies under the VLBI scope - II. The relationship between γ-ray emission and parsec-scale jets in radio galaxies

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Volume 641 (September 2020)

A&A, 641 (2020) A152

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Table 1.

Radio galaxies in the TANAMI sample.

B1950 name	Other name	Class ^(a)	Redshift	RA(J2000)	Dec(J2000)	4FGL ^(b)	Ref ^(c)
0518−458	Pictor A	FR II	0.035	79.957	−45.779	J0519.6−4544	[1]
0521−365	PKS 0521−36	RG/SSRQ	0.057	80.742	−36.459	J0522.9−3628	[2]
0625−354	PKS 0625−35	FR I/BLL	0.055	96.778	−35.487	J0627.0−3529	[3]
1258−321	PKS 1258−321	FR I	0.017	195.253	−32.441	−	[4]
1322−428	Centaurus A	FR I	0.0018	201.365	−43.019	J1325.5−4300	[5]
1333−337	IC 4296	FR I	0.013	204.162	−33.966	−	[4]
1343−601	Centaurus B	FR I	0.013	206.704	−60.408	J1346.3−6026	[6]
1549−790	PKS 1549−79	RG/CFS	0.15	239.245	−79.234	−	[7]
1600−489	PMN J1603−4904	GPS ^(d)	0.23	240.961	−49.068	J1603.8−4903	[8]
1718−649	PKS 1718−649	GPS/CSO	0.014	260.921	−65.010	J1724.2−6501	[9]
1733−565	PKS 1733−56	FR II	0.098	264.399	−56.567	−	[2]
1814−637	PKS 1814−63	CSS/CSO	0.065	274.896	−63.763	−	[7]
2027−308	PKS 2027−308	RG	0.539	307.741	−30.657	−	[10]
2152−699	PKS 2153−69	FR II	0.028	329.275	−69.690	J2156.0−6942 ^(e)	[11]

Notes.

^(a)

FR I: Fanaroff-Riley type 1; FR II: Fanaroff-Riley type 2; BLL: BL Lac; RG: Radio galaxy; SSRQ: Steep Spectrum Radio Quasar; CFS: Compact Flat Spectrum; GPS: Gigahertz Peaked Spectrum; CSO: Compact Symmetric Object; CSS: Compact Steep Spectrum (see O’Dea 1998 for a review on the GPS, CSO and CSS classes).

^(b)

Γ-ray counterpart source name from the 4FGL (Abdollahi et al. 2020), if applicable.

^(c)

Redshift reference: [1] Lauberts & Valentijn (1989), [2] Jones et al. (2009), [3] Quintana & Ramirez (1995), [4] Smith et al. (2000), [5] Graham (1978), [6] West & Tarenghi (1989), [7] Holt et al. (2008), [8] Goldoni et al. (2016), [9] Meyer et al. (2004), [10] Healey et al. (2008), [11] da Costa et al. (1991).

^(d)

Originally misclassified as BL Lac, this source has been classified as a young radio galaxy based on multi-wavelength studies (Müller et al. 2014a, 2015, 2016).

^(e)

See Sect. 3.3.

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