  We have measured the relationships between HI mass, stellar mass and star
formation rate using the HI Parkes All Sky-Survey Catalogue (HICAT) and the
Wide-field Infrared Survey Explorer (WISE). Of the 3,513 HICAT sources, we find
3.4 micron counterparts for 2,896 sources (80%) and provide new WISE matched
aperture photometry for these galaxies. For our principal sample of spiral
galaxies with W1 $\le$ 10 mag and z $\le$ 0.01, we identify HI detections for
93% of the sample. We measure lower HI-stellar mass relationships that HI
selected samples that do not include spiral galaxies with little HI gas. Our
observations of the spiral sample show that HI mass increases with stellar mass
with a power-law index 0.35; however, this value is dependent on T-type, which
affects both the median and the dispersion of HI mass. We also observe an upper
limit on the HI gas fraction, which is consistent with a halo spin parameter
model. We measure the star formation efficiency of spiral galaxies to be
constant 10$^{-9.57}$ yr$^{-1}$ $\pm$ 0.4 dex for 2.5 orders of magnitude in
stellar mass, despite the higher stellar mass spiral showing evidence of
quenched star formation.
