Each column presents distributions of different parameters of the DPS (red) and the NBCS (black). We show different morphological classifications in each row: in the top row the full samples, followed by Sa, Sb-d, S0s, elliptical, merger and galaxies without classification (see Sect. 3.2). From left to right: first column: star formation rate inside the 3″ SDSS fibre (SFR_fibre), second column: total star formation rate (SFR_Total) (Brinchmann et al. 2004), third column: stellar mass M_* (Kauffmann et al. 2003). last column: extinction computed with the Balmer decrements Hα/Hβ (Domínguez et al. 2013). We use the non-parametric emission line fit to estimate emission line fluxes taken from Chilingarian et al. (2017). We display the mean and the standard deviation for each distribution.