Scaling properties of Planck clusters, colour-coded as a function of redshift. In all figures, R₅₀₀ and M₅₀₀ are estimated from the M₅₀₀–Y_X relation of Arnaud et al. (2010). Top left panel: the scaled density profiles of the new clusters confirmed with XMM-Newton observations. The radii are scaled to R₅₀₀. The density is scaled to the mean density within R₅₀₀. The thick lines denote the mean scaled profile for each sub-sample. The black line is the mean profile of the REXCESS sample (Arnaud et al. 2010). Other panels: scaling relations. Squares show the new clusters confirmed with XMM-Newton observations. Points show clusters in the Planck-ESZ sample with XMM-Newton archival data as presented in Planck Collaboration (2011c). Relations are plotted between the intrinsic Compton parameter, , and the mass M₅₀₀ (top right panel), between the X-ray luminosity and Y₅₀₀ (bottom left panel) and between mass and luminosity (bottom right panel). Each quantity is scaled with redshift, as expected from standard self-similar evolution. The lines in the left and middle panel denotes the predicted Y₅₀₀ scaling relations from the REXCESS X-ray observations (Arnaud et al. 2010). The line in the right panel is the Malmquist bias corrected M–L relation from the REXCESS sample (Pratt et al. 2009; Arnaud et al. 2010). The new clusters are on average less luminous at a given Y₅₀₀, or more massive at a given luminosity, than X-ray selected clusters. There is no evidence of non-standard evolution.