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Fig. 9


SFR-M relation in the main sample (black crosses) with average error bars shown in the bottom right corner and best fit estimate (black solid line). Green diamonds show the results for a sample of low redshift star forming galaxies (0.05 <z< 0.5, Bauermeister et al. 2013), red crosses are high redshift star forming galaxies (1 <z< 3 Tacconi et al. 2013), blue triangles local LIRGs at z 0.4 (Geach et al. 2011), magenta stars and cyan circles show local spirals (Leroy et al. 2008) and ULIRGs (Gao & Solomon 2004), respectively. The fits are from: local galaxies of Ciesla et al. (2014) and Peng et al. (2010; green dashed and red dotted line), galaxies at z = 2 and z = 4 in Rodighiero et al. (2011; blue dot-dashed line), and the compilation shown in Speagle et al. (2014; magenta double dotted line).

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