Table A.1
TANAMI VLBI observed sources.
Namea | Common namea | Classb | z c | First epoch | B16d | Radio | γ-ray | Inside HESE(> 100 TeV) |
image | samplee | samplef | R 50 | |||||
|
||||||||
0047–579 | [HB89] 0047–579 | Q | 1.797 | Paper I | Y | Y | ||
0055–328 | PKS 0055–328 | B | 1.370 | This Work | Y | |||
0144–522 | PKS 0144–522 | G | 0.098 | This Work | ||||
0208–512 | [HB89] 0208–512 | Q | 0.999 | Paper I | Y | Y | Y | |
0227–369 | PKS 0227–369 | Q | 2.115 | This Work | Y | |||
0235–618 | PKS 0235–618 | Q | 0.465 | This Workh | HESE-20 | |||
0244–470 | PKS 0244–470 | Q | 1.385 | This Work | Y | Y | ||
0302–623 | PKS 0302–623 | Q | 1.351 | This Workh | Y | HESE-20 | ||
0308–611 | PKS 0308–611 | Q | 1.480 | This Workh | Y | HESE-20 | ||
0332–376 | PMN J0334–3725 | B | >0.39 | This Work | Y | |||
0332–403 | [HB89] 0332–403 | B | 1.351 | Paper I | Y | Y | Y | |
0402–362 | PKS 0402–362 | Q | 1.417 | This Work | Y | Y | ||
0405–385 | [HB89] 0405–385 | Q | 1.285 | Paper I | Y | |||
0412–536 | PMNJ0413–5332 | Q | 1.024 | This Work | Y | |||
0426–380 | PKS 0426–380 | Q | 1.110 | This Work | Y | Y | ||
0438–436 | [HB89] 0438–436 | Q | 2.863 | Paper I | Y | Y | ||
0447–439 | PKS 0447–439 | B | – | This Work | Y | Y | ||
0454–463 | [HB89] 0454–463 | Q | 0.853 | Paper I | Y | Y | ||
0506–612 | [HB89] 0506–612 | Q | 1.093 | Paper I | Y | |||
0516–621 | PKS 0516–621 | Q | 1.300 | This Work | Y | |||
0518–458 | Pic A | G | 0.035 | Paper I | Y | |||
0521–365 | ESO 362– G 021 | G | 0.055 | Paper I | Y | Y | Y | |
0524–485 | PKS 0524–485 | Q | 1.300 | This Work | Y | |||
0527–359 | PMNJ0529–3555 | U | 0.323 | This Work | Y | |||
0530–485 | PMNJ0531–4827 | Q | – | This Work | Y | |||
0537–441 | [HB89] 0537–441 | Q | 0.894 | Paper I | Y | Y | Y | |
0625–354 | PKS 0625–35 | B | 0.055 | Paper I | Y | Y | ||
0637–752 | [HB89] 0637–752 | Q | 0.653 | Paper I | Y | Y | HESE-30 | |
0646–306 | PKS 0646–306 | Q | 0.455 | This Work | HESE-39 | |||
0700–661 | PKS 0700–661 | B | >0.39 | This Work | Y | |||
0717–432 | PMN J0718–4319 | U | – | This Work | Y | |||
0736–770 | PKS0736–770 | Q | – | This Work | Y | HESE-30 | ||
0745–330 | PKS0745–330 | U | – | This Work | Y | |||
0812–736 | PMN J0810–7530 | U | – | This Work | Y | HESE-30 | ||
0902–350 | 1FGLJ0904.7–3514 | U | – | This Work | ||||
0943–761 | PKS 0943–76 | G | 0.270 | – j | ||||
1057–797 | PKS 1057–79 | B | 0.581 | This Work | Y | |||
1101–536 | PKS 1101–536 | B | >0.15 | Krauß et al. (2015) | Y | HESE-4 | ||
1104–445 | [HB89] 1104–445 | Q | 1.598 | Paper I | Y | Y | HESE-4 | |
1144–379 | [HB89] 1144–379 | Q | 1.048 | Paper I | Y | |||
1257–326 | PKS 1257–326 | Q | 1.256 | Paper I | Y | |||
1258–321 | ESO443–G024 | G | 0.017 | This Work | Y | |||
1313–333 | [HB89] 1313–333 | Q | 1.210 | Paper I | Y | |||
1322–428 | Cen A | G | 0.002 | Paper I | Y | Y | HESE-35 | |
1323–526 | PMN J1326–5256 | B | >0.24 | Paper I | Y | HESE-35 | ||
1325–558 | PMN J1329–5608 | B | >0.13 | This Work | Y | Y | HESE-35 | |
1333–337 | IC 4296 | G | 0.012 | Paper I | Y | HESE-48 | ||
1343–601 | Cen B | G | 0.013 | This Work | HESE-35 | |||
1344–376 | PMN J1347–3750 | Q | 1.300 | This Work | Y | HESE-48 | ||
1409–651 | Circinus Galaxy | G | 0.001 | – j | HESE-35 | |||
1424–418 | [HB89] 1424–418 | Q | 1.522 | Paper I | Y | Y | Y | HESE-35 |
1440–389 | PKS 1440–389 | B | >0.14 | This Work | Y | |||
1454–354 | PKS 1454–354 | Q | 1.424 | Paper I | Y | Y | Y | |
1501–343 | PMN J1505–3432 | B | 1.554 | Paper I | Y | |||
1505–496 | PMN J1508–4953 | Q | 0.776 | This Work | Y | HESE-35 | ||
1549–790 | PKS 1549–79 | G | 0.150 | Paper I | Y | Y | ||
1600–445 | PMN J1604–4441 | U | >0.01 | This Work | Y | |||
1600–489 | PMN J1603–4904 | G | 0.230g | Müller et al. (2014) | Y | Y | ||
1606–667 | PMN J1610–6649 | U | – | This Work | Y | |||
1610–771 | [HB89] 1610–771 | Q | 1.710 | Paper I | Y | Y | ||
1613–586 | PMN J1617–5848 | Q | – | This Work | Y | HESE-52 | ||
1646–506 | PMNJ1650–5044 | U | 0.090 | This Work | Y | Y | HESE-52 | |
1653–329 | SwiftJ1656.3–3302 | Q | 2.400 | Krauß et al. (2014) | HESE-2, HESE-14 | |||
1714–336 | PMN J1717–3342 | B | – | Paper I | Y | Y | HESE-2, HESE-14 | |
1716–771 | PKS 1716–771 | U | – | Paper I | Y | |||
1718–649 | NGC 6328 | G | 0.010 | Paper I | Y | Y | ||
1733–565 | PKS 1733–56 | G | 0.098 | Paper I | Y | Y | HESE-52 | |
1759–396 | PMN J1802–3940 | Q | 1.320 | Paper I | Y | Y | HESE-2, HESE-14 | |
1804–502 | PMN J1808–5011 | Q | 1.606 | Paper I | Y | HESE-2 | ||
1814–637 | PKS 1814–63 | G | 0.063 | Paper I | Y | |||
1915–458 | PKS 1915–458 | Q | 2.470 | This Work | HESE-2, HESE-12 | |||
1933–400 | PKS 1933–400 | Q | 0.965 | Paper I | Y | HESE-2 | ||
1954–388 | [HB89] 1954–388 | Q | 0.630 | Paper I | Y | Y | HESE-2 | |
2004–447 | PKS 2004–447 | G | 0.240 | Schulz et al. (2016) | HESE-2,HESE-12 | |||
2005–489 | [HB89] 2005–489 | B | 0.071 | Paper I | Y | HESE-12 | ||
2027–308 | ESO 462– G 027 | G | 0.539 | Paper I | Y | HESE-2 | ||
2052–474 | [HB89] 2052–474 | Q | 1.489 | Paper I | Y | Y | Y | |
2106–413 | [HB89] 2106–413 | Q | 1.058 | Paper I | Y | Y | ||
2123–463 | PKS 2123–463 | Q | 1.46i | This Work | ||||
2136–428 | PMNJ2139–4235 | B | – | This Work | Y | Y | ||
2142–758 | PKS 2142–75 | Q | 1.139 | This Work | Y | |||
2149–306 | PKS 2149–306 | Q | 2.345 | Paper I | Y | |||
2152–699 | ESO 075– G 041 | G | 0.028 | Paper I | Y | |||
2154–838 | PKS 2155–83 | Q | – | This Work | ||||
2155–304 | [HB89] 2155–304 | B | 0.116 | Paper I | Y | Y | ||
2204–540 | [HB89] 2204–540 | Q | 1.206 | Paper I | Y | Y | ||
2326–477 | [HB89] 2326–477 | Q | 1.299 | Paper I | Y | Y | ||
2355–534 | [HB89] 2355–534 | Q | 1.006 | Paper I | Y |
Notes.
Optical classification after Véron-Cetty & Véron (2006) and Shaw et al. (2012, 2013) with Q: quasar, B: BL Lac, G: galaxy, U: unidentified object.
Source included in the radio-γ correlation study of the first year of Fermi/LAT data by Böck et al. (2016, B16).
The radio-selected subsample includes all sources south of declination − 30° from the catalog of Stickel et al. (1994) above a limiting radio flux density of S5 GHz> 2 Jy with a flat radio spectrum (α> −0.5, S ~ ν+ α) between 2.7 GHz and 5 GHz (22 sources).
The γ-ray sample includes the γ-ray brightest AGN south of declination − 30° in the 3LAC catalog (22 sources).
Redshift measurement by Goldoni et al. (2016).
Results of TANAMI VLBI observations quasi-simultaneous to the IceCube events were presented in Krauß et al. (2014).
Redshift measurement by D’Ammando et al. (2012).
See Fig. 3.
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