Different parameters distributions of the DPS (red), the CS (blue) and the NBCS (black). The surfaces of all histograms are normalised to unity. In the upper left panel, we compute the absolute AB magnitude in the r-band with Galactic dust and K-corrections estimated by Chilingarian et al. (2017). The lower left panel shows the specific star formation ratio (SSFR) computed by Brinchmann et al. (2004). The middle upper (resp. lower) panel presents the absolute luminosity of the [OIII]λ5008 (resp. Hαλ6565) emission line. The absolute luminosity is calculated using the flux of the non-parametric emission line fit provided by Chilingarian et al. (2017). The right upper panel computes the age assumed by a single stellar population fit by Chilingarian et al. (2017). The right lower panel shows the stellar metallicity computed by Chilingarian et al. (2017).