SFR vs. stellar mass of emission line selected galaxies, color-coded according to their redshift. The two red triangles mark objects with two redshift solutions (only primary solution shown). Solid lines show the relations reported by Karim et al. (2011). Dashed lines are the best fit of relations with the same slopes to our data. The vertical grey dashed line marks the lower mass limit of the Karim et al. (2011) sample.