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Table 1

Details of the 8.4 GHz TANAMI observations of Centaurus A.

Obs. date Array configurationa S peak b rmsb S total b S inner jet c b maj d b min d PAd
(yyyy-mm-dd) (Jy beam-1) (mJy beam-1) (Jy) (Jy) (mas) (mas) (°)

2007-11-10 AT-MP-HO-HH-CD-PKS 0.60 ± 0.09 0.40 ± 0.06 2.6 ± 0.4 2.5 ± 0.4 1.64 0.41 7.9
2008-06-09 AT-MP-HO-HH-CD-PKS 1.06 ± 0.16 0.63 ± 0.09 3.1 ± 0.5 2.7 ± 0.4 2.86 1.18 −12.7
2008-11-27 TC-OH-AT-MP-HO-CD-PKS-DSS43 0.74 ± 0.11 0.37 ± 0.06 4.0 ± 0.6 3.1 ± 0.5 0.98 0.59 31.4
2009-09-05 TC-OH-AT-MP-HO-CD-PKS-DSS43 0.76 ± 0.11 0.45 ± 0.07 4.0 ± 0.6 3.0 ± 0.4 2.29 0.58 15.6
2009-12-13 TC-AT-MP-HO-CD-PKS 1.03 ± 0.15 0.18 ± 0.03 3.8 ± 0.6 3.0 ± 0.4 3.33 0.78 26.3
2010-07-24 TC-AT-MP-HO-CD-PKS 1.21 ± 0.18 0.38 ± 0.06 4.2 ± 0.6 3.3 ± 0.5 2.60 0.87 21.4
2011-04-01 TC-WW-AT-MP-HO-HH-CD-PKS-DSS43 0.63 ± 0.09 0.31 ± 0.05 5.1 ± 0.8 3.8 ± 0.6 2.31 0.51 −0.7

Notes.

(a)

AT: Australia Telescope Compact Array; CD: Ceduna; HH: Hartebeesthoek; HO: Hobart; MP: Mopra; OH: GARS/O’Higgins, PKS: Parkes, TC: TIGO, DSS43: NASA’s Deep Space Network Tidbinbilla (70 m); WW: Warkworth;

(b)

Peak flux density; rms noise level and total flux density in the CLEAN-image;

(c)

TANAMI 8.4 GHz flux density of inner jet defined by −2 mas ≲ RArelative ≲ 15 mas and adopting an uncertainty of 15% (see Sect. 4.5);

(d)

Major and minor axes and position angle of restoring beam.

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