H-R diagram for the new members of IC 348 spectroscopically confirmed (filled circles with white crosses), as well as the previously known brown dwarf members of the cluster (open circles). The models are the Dusty isochrones (Chabrier et al. 2000) for 1, 3, 5, 10, and 30 Myr, labelled with mass in units of M_⊙. Additionally, candidates classified as having an uncertain membership status are shown as triangles.