Abstract
We present a preliminary study of the velocity field in the neighbourhood of the Abell 1942 cluster of galaxies (z ≈ 0.22), for which both photometric and spectroscopic redshifts are available. Besides characterizing the dynamical stage of this particular cluster, the aim of this work is to search for efficient tools capable to provide reliable representations of the infall velocity fields for samples of clusters of galaxies, based solely on photometric redshifts.
