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Fig. 1


(u,v)-plane of two representative TANAMI VLBI observations at 8.4 GHz showing the improved coverage at − 38° (left) and − 62° (right) declination due to including new telescopes since 2011 (compare to Fig. 12 in Paper I). The intermediate (u,v)-range is covered due to baselines to Warkworth (left) and Katherine and Yarragadee (right). The long baselines are provided by TIGO and Hartebeesthoek.

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