The starting point of our analysis is the Planck cosmology sample (PSZ1-cosmo) described in Planck Collaboration XX (2014A&A...571A..20P). It is a high-purity subsample constructed from the first release of the Planck catalogue of SZ sources (Planck Collaboration XXIX, 2014A&A...571A..29P, Cat. VIII/91), by imposing a signal-to-noise ratio (S/N) threshold of 7 and applying a mask, that excludes the galactic plane and point sources leaving 65 per cent of the sky for the survey. It contains 189 bona fide clusters with associated redshifts and has been used for the cosmological analysis with cluster number counts described in Planck Collaboration XX (2014A&A...571A..20P). (2 data files).