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Table 3

Upper limits on the γ-ray emission of TANAMI sources not associated with 1FGL sources.

Namea Source Common name TS F (0.1–100 GeV) L (0.1–100 GeV) Score (8.4 GHz) TBb IDc z Sep.d Conf95γe
[10-8 ph cm-2 s-1] [erg s-1] [Jy] [K] [degree] [degree]
0438−436 J0440−4333 [HB89] 0438−436 2 ≤ 1.1 ≤ 6.8 × 1047 0.59 ± 0.09 1.4 × 1011 Q 2.863 1.69 0.02
0518−458 J0519−4546 PICTOR A 11 ≤ 1.8 ≤ 2.7 × 1043 0.55 ± 0.09 2.7 × 1010 G 0.035 1.86 0.25
0527−359 J0529−3555 PMN J0529−3555 0 ≤ 1.1 ≤ 2.1 × 1045 0.323 1.51 0.10
1104−445 J1107−4449 [HB89] 1104−445 2 ≤ 1.4 ≤ 1.7 × 1047 1.41 ± 0.22 2.7 × 1011 Q 1.598 0.77 0.21
1257−326 J1300−3253 PKS 1257−326 2 ≤ 2.1 ≤ 1.4 × 1047 0.13 ± 0.02 3.9 × 1010 Q 1.256 0.35 0.13
1258−321 J1301−3226 ESO 443- G 024 18 ≤ 2.4 ≤ 8.3 × 1042 G 0.017 0.56 0.13
1333−337 J1336−3357 IC 4296 0 ≤ 0.9 ≤ 1.5 × 1042 0.22 ± 0.04 6.2 × 109 G 0.012 4.27 0.07
1549−790 J1556−7914 PKS 1549−79 5 ≤ 2.2 ≤ 7.3 × 1044 0.36 ± 0.06 1.6 × 1010 G 0.150 2.23 0.09
1718−649 J1723−6500 NGC 6328 4 ≤ 0.8 ≤ 9.3 × 1041 G 0.010 3.57 0.17
1716−771 J1723−7713 PKS 1716−771 9 ≤ 2.0 0.43 ± 0.07 9.0 × 1010 ∗ 1.45 0.08
1733−565 J1737−5634 PKS 1733−56 0 ≤ 0.8 ≤ 1.0 × 1044 0.18 ± 0.03 4.9 × 1010 G 0.098 4.83 0.10
1804−502 J1808−5011 PMN J1808−5011 23 ≤ 2.2 ≤ 2.9 × 1047 0.45 ± 0.07 5.9 × 1012 Q 1.606 2.28 0.15
1814−637 J1819−6345 PKS 1814−63 5 ≤ 2.1 ≤ 1.1 × 1044 0.32 ± 0.05 6.5 × 1010 G 0.063 1.95 0.18
1934−638 J1939−6342 PKS 1934−63 0 ≤ 0.9 ≤ 4.5 × 1044 G 0.180 5.74 0.40
2027−308 J2030−3039 PKS 2027−308 5 ≤ 1.8 ≤ 1.3 × 1046 0.08 ± 0.02 4.7 × 109 0.539 2.09 0.14
2106−413 J2109−4110 [HB89] 2106−413 0 ≤ 0.6 ≤ 2.4 × 1046 1.04 ± 0.16 1.6 × 1011 Q 1.058 2.94 0.12
2152−699 J2157−6941 ESO 075- G 041 5 ≤ 1.7 ≤ 1.6 × 1043 0.43 ± 0.07 4.1 × 1010 G 0.028 2.45 0.21
2355−534 J2357−5311 [HB89] 2355−534 2 ≤ 1.7 ≤ 6.2 × 1046 1.53 ± 0.23 5.0 × 1011 Q 1.006 0.40 0.28

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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