We obtain mass distribution for flattened galaxies M94 and M101 whose rotation curves fail sphericity test in thin disk approximation by applying Iterative Spectral Method. The results obtained suggest smaller amount of dark matter (if any) than predicted by classical approach to modelling of rotation curves customarily assuming massive spherical halo.

PACS numbers: 98.80.--k, 95.35.+d, 98.35.Ce