tokens: We are grateful to the S 3 -SAX and HIPASS collaborations. SAM wishes to thank Stefan Westerlund, Laura Hoppmann, Jacinta Delhaize, Matthew Pearce, Rebecca Lange and Angus Wright for coding assistance and Taylem Frost for editorial work. We acknowledge use of the topcat software package ( http://www.star.bristol.ac.uk/∼mbt/topcat/ ) and miriad (Sault 1995 ) for data reduction. This research was conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020.
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