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We report the results of a successful 24 hour 6.7 GHz VLBI experiment usingthe 30 meter radio telescope WARK30M near Warkworth, New Zealand, recentlyconverted from a radio telecommunications antenna, and two radio telescopeslocated in Australia: Hobart 26-m and Ceduna 30-m. The geocentric position ofWARK30M is determined with a 100 mm uncertainty for the vertical component and10 mm for the horizontal components. We report correlated flux densities at 6.7GHz of 175 radio sources associated with Fermi gamma-ray sources. A parsecscale emission from the radio source 1031-837 is detected, and its associationwith the gamma-ray object 2FGL J1032.9-8401 is established with a highlikelihood ratio. We conclude that the new Pacific area radio telescope WARK30Mis ready to operate for scientific projects.

First scientific VLBI observations using New Zealand 30 metre radio telescope WARK30M