  Infall of cold dark matter on a galaxy may result in caustic rings where the
particle density is enhanced. They may be searched for as features in the
galactic rotation curves. Previous studies suggested the evidence for these
caustic rings with universal, that is common for different galaxies,
parameters. Here we test this hypothesis with a large independent set of
rotation curves by means of an improved statistical method. No evidence for
universal caustic rings is found in the new analysis.
