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Table 2

Properties of additional γ-ray detections of TANAMI sources in the 1FGL period.

Namea Source Common name TS F (0.1–100 GeV) LAT Γ L (0.1–100 GeV) Score (8.4 GHz) TBb IDc z Sep.c Conf95γd
[10-8 ph cm-2 s-1] [erg s-1] [Jy] [K] [degree] [degree]
1505−496 J1508−4953 PMN J1508−4953 68 4.0 ± 0.9 2.18 ± 0.09 (9.8 ± 1.8) × 1046 0.50 ± 0.08 2.2 × 1012 Q 0.776 0.89 0.05
2149−306 J2151−3027 PKS 2149−306 61 5.1 ± 0.9 2.99 ± 0.16 (2.2 ± 0.5) × 1048 1.27 ± 0.20 1.4 × 1012 Q 2.345 1.51 0.02
2326−477 J2329−4730 [HB89] 2326−477 27 3.0 ± 1.0 3.0 ± 0.4 (2.2 ± 0.9) × 1047 0.81 ± 0.13 9.7 × 1010 Q 1.299 0.32 0.16

Notes.

(a)

Name in B1950.0 IAU format;

(b)

brightness temperatures available in the 1FGL period; for sources without measured redshift a lower limit based on z = 0 is indicated with a star (∗);

(c)

classifications as described in Sect. 2.1: Q: Quasar, B: BL Lac, G: galaxy;

(d)

angular separation of the radio position of the TANAMI source and the closest 1FGL source;

(e)

semimajor axis of the 95% confidence region of the position of the closest 1FGL source.

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