  Epicyclic frequencies are usually observed in X-ray binaries and constitute a
powerful astrophysical mean to probe the strong gravitational field around a
compact object. We consider them in the equatorial plane around a general
stationary and axially symmetric wormhole. We first search for the wormholes'
existence, distinguishing them from a Kerr black hole. Once there will be
available observational data on wormholes, we present a strategy to reconstruct
the related metrics. Finally, we discuss the implications of our approach and
outline possible future perspectives.
