Free Access

Fig. 2


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).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.