Rotation curves with the multistate Scalar Field Dark Matter model
  We use the concept of co-added rotation curves of Salucci et al. to
investigate the properties of axi-symmetric multistate Scalar Field Dark Matter
halos in low surface brightness galaxies and dwarf disc galaxies. We fit their
rotation curves in two-state configurations and we find that all of these can
be well fitted with a particle mass $\mu \sim (10^{-23} -
10^{-24})\rm{eV}/c^2$. Comparing our results with the standard cosmological
model, the well-known $\Lambda$-cold dark matter, by using the Bayesian
information criterion and the Akaike information criterion, we found that our
two-state model seemed to be preferred.
