Mass models for low surface brightness galaxies with high-resolution optical velocity fields

We present high-resolution optical velocity fields from DensePak integral field spectroscopy, along with derived rotation curves, for a sample of low surface brightness galaxies. In the limit of no baryons, we fit the NFW and pseudoisothermal halo models to the data and find the rotation curve shapes and halo central densities to be better described by the isothermal halo. For those galaxies with photometry, we present halo fits for three assumptions of the stellar mass-to-light ratio, Gamma*. We find that the velocity contribution from the baryons is significant enough in the maximum disk case that maximum disk and the NFW halo are mutually exclusive. We find a substantial cusp mass excess at the centers of the galaxies, with at least 2 times more mass expected in the cuspy CDM halo than is allowed by the data. We also find that to reconcile the data with Lambda CDM, similar to 20 km s(-1) noncircular motions are needed and/or the power spectrum has a lower amplitude on the scales that we probe.