Correlation between the extinction-corrected Hα SFR and the total stellar mass of the galaxies. Solid line represents the fit of Elbaz et al. (2007) with a slope of 0.77 for galaxies in the 0.04 <z< 0.1 range, while dashed lines correspond to the dispersion of this fit. Type-2 AGN host galaxies dominate the high-mass end in the main sequence plot for our galaxies. They show somewhat smaller SFR values for the same stellar mass. This fact could be because of a fraction of Hα emission absorbed by the AGN or in the circumnuclear region or, alternatively, the presence of the type-2 AGN might impact the internal evolution of the galaxy quenching the SF.