As part of the widefield continuum and polarisation capability demonstration, a full Stokes image of the region in the southern constellation Tucana, made over the frequency 700–1000 MHz, will be made available to those users interested in accessing the data.
Observations were made in September, using a square beam footprint and two pointings for each observation. The final image covers an area of approximately 31 square degrees with image noise over most of that area at approximately 0.45 mJy/beam.
Images of the area have been made for Stokes quantities I, Q, U and V. While the data are not polarimetrically calibrated, they demonstrate that all polarisation products are correlated and passed through the system software.