  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.
