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

Rotation curves with the multistate Scalar Field Dark Matter model