a) magnitude distribution for V_p and Q_p family members; b) solar phase angle distribution for V_p and Q_p family members; c) magnitude distribution for Q_p with a < 2.5 AU, within and outside the family; d) solar fase angle distribution for the sample in c). The family definition is taken from Nesvorny et al. (2012). The phase angle corresponds to the SDSS observation considered most representative according to Carvano et al. (2010).