We present a model independent analysis of the Pantheon+ supernova sample and study the dependence of the recovered values of H_0, q_0 and j_0 on the redshift cut and on the modeling of peculiar velocities. In addition to the bulk velocity discussed previously, we also find a significant infall that we attribute to the presence of an overdensity out to a radius of R\simeq 120h^{-1}Mpc.
