Observations by J.Dickel, R.Gruendl, V.McIntyre, D.K.Milne (2001, 2002, 2003). Published in Astronomical Journal, 129, 790 (2005) (2005AJ....129..790D).

The project was intended to gather a data set with uniform uv-plane coverage, to produce images with sufficient spatial resolution and sensitivity to identify most of the SNRs and HII regions, and (together with Parkes observations) give a good representation of the smooth emission within the galaxy. The 6km antenna was included to allow discrimination of point sources.

The visibility data have been grouped into sets of pointings centered on the locations tabulated below. For full fidelity, all the visibility data should be used to generate images. However for small fields of interest one may be able to use the visibility data for just the relevant subfield.

The figure designations used in the electronic version of the paper differ from the tile designations used during observation. Here we show the correspondence. The positions in Table 1 of the paper refer to the centres of the displayed images, not the tile centres.

The 'match-filtered' images have been constructed from a subset of the uv-data; the long spacings at 8.6 GHz and the short spacings at 4.8 GHz have been excluded to give the same range of spatial frequency response at both freqencies.