The acquisition of HI Parkes All Shy Survey (HIPASS) southern sky data comm
enced at the Australia Telescope National Facility's Parkes 64-m telescope
in 1997 February, and was completed in 2000 March. HIPASS is the deepest HI
survey yet of the sky south of declination +2 degrees, and is sensitive to
emission out to 170 h(75)(-1) Mpc. The characteristic root mean square noi
se in the survey images is 13.3 mJy. This paper describes the survey observ
ations, which comprise 23 020 eight-degree scans of 9-min duration, and det
ails the techniques used to calibrate and image the data. The processing al
gorithms are successfully designed to be statistically robust to the presen
ce of interference signals, and are particular to imaging point (or nearly
point) sources. Specifically, a major improvement in image quality is obtai
ned by designing a median-gridding algorithm which uses the median estimato
r in place of the mean estimator.