a) SFR-stellar mass relation for BAT6 sample. The host of the GRB 060614A is plotted with a different symbol (diamond) to emphasise the dubious nature of the GRB. The colour-coding corresponds to redshifts as noted with the colour bar on the right sight of the plot. Small points with the same colour-coding correspond to the 0.3 <z< 1.0 VVDS survey of star-forming galaxies (Le Fèvre et al. 2013). In addition, we plot the median value of SFR-stellar mass relation at z ~ 0.7 (mean redshift of the VVDS sample and the BAT6 sample without the host of GRB 060614) as observed in the NEWFIRM medium band survey (NMBS; Whitaker et al. 2012). We note that the latter relation has a scatter of ± 0.34 dex (indicated by an error bar in the plots). With a dashed line we draw the extrapolation of the relation below the stellar mass completeness of the Whitaker et al. (2012) survey. b) Specific SFR-mass relation. The median value of the Whitaker et al. (2012) relation at z ~ 0.7 is plotted. The dotted line represents the relation plus the dispersion (0.34 dex).
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