Fig. 6

Evolution of the radio spectral index, , with redshift, as inferred from our
stacking analysis. Red circles and error bars correspond to the median and
interquartile range observed in our study in regions of the parameter space not
affected by incompleteness (see values and green lines reported in Fig. 5). Stars show results from Ivison et al. (2010a), while triangles show results from Bourne et al. (2011). Both studies are based on a
stacking analysis, but Ivison et al. (2010a)
applied it to a sample of 24 μm-selected galaxies while Bourne et al. (2011) applied it to a
stellar-mass-selected galaxy sample. The light grey region shows the range of
values (i.e. 0.7 ± 0.4) observed by Ibar et al. (2009) in a population of sub-mJy
radio galaxies. The dark grey region presents the range of
values (i.e. 0.75 ± 0.29) observed in a population
of SMGs at zs2 (Ibar et
al. 2010). Note that the ranges of values observed in Ibar et al. (2009, 2010)
correspond to the intrinsic dispersion observed in these galaxy populations and not
to measurement errors on the mean radio spectral indices.
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