  A deep blind HI survey of the nearby spiral rich Ursa Major cluster has been
performed with the VLA in parallel with a wide-field R-band imaging campaign of
most VLA fields with the CFHT. The goal is to measure the slope of the HI mass
function down to HI masses of 10^7 Msun as well as the slope of the faint-end
of the luminosity function down to M(R)=-10. The VLA survey sampled 16% of the
Ursa Major cluster volume. Both the HIMF and the LF in Ursa Major are nearly
flat at their faint-ends. No free- floating HI clouds were detected.
