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Fig. 5


Comparison between some MS slopes present in the literature and the slopes derived in this work using all SF galaxies (black stars) and only SF galaxies with log10(M/M0) > 9.5 (empty stars). All other slopes are taken from: Oliver et al. (2010; red triangles), Karim et al. (2011; magenta triangles), Rodighiero et al. (2011; red circles), Whitaker et al. (2014; red squares), Johnston et al. (2015; green circles), Shivaei et al. (2015; blue triangles) and Kurczynski et al. (2016; green squares). The red continuous line shows the relation derived by Speagle et al. (2014) and the dotted red lines are the median inter-publication scatter around the fit.

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