HI Global Scaling Relations in the WISE-WHISP Survey
  We present the global scaling relations between the neutral atomic hydrogen
gas, the stellar disk and the star forming disk in a sample of 228 nearby
galaxies that are both spatially and spectrally resolved in HI line emission.
We have used HI data from the Westerbork survey of HI in Irregular and Spiral
galaxies (WHISP) and Mid Infrared (3.4 $\mu m$, 11.6 $\mu m$) data from the
Wide-field Infrared Survey Explorer (WISE) survey, combining two datasets that
are well-suited to such a study in terms of uniformity, resolution and
sensitivity. We utilize the novel method of deriving scaling relations for
quantities enclosed within the stellar disk rather than integrating over the HI
disk and find the global scaling relations to be tighter when defined for
enclosed quantities. We also present new HI intensity maps for the WHISP survey
derived using a robust noise rejection technique along with corresponding
velocity fields.
