A local infall from a cosmographic analysis of Pantheon+

Abstract 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 ≃ 120 h -1 Mpc.