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By using the deepest available mid and far infrared surveys in the CANDELS,GOODS and COSMOS fields we study the evolution of the Main Sequence (MS) ofstar forming galaxies (SFGs) from z~0 to` ~2.5 at stellar masses larger than10^{10} M_{\odot}. The MS slope and scatter are consistent with a re-scaledversion of the local relation and distribution, shifted at higher values of SFRaccording to ~(1+z)^{3.2}. The relation exhibits a bending at the high mass endand a slightly increasing scatter as a function of the stellar mass. We showthat the previously reported evolution of the MS slope, in the considered massand redshift range, is due to a selection effect. The distribution of galaxiesin the MS region at fixed stellar mass is well represented by a singlelog-normal distribution at all redshifts and masses, with starburst galaxies(SBs) occupying the tail at high SFR.

The main sequence of star forming galaxies II. A non evolving slope at the high mass end