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Table 9:

Evolution of the mass-to-light ratio for the wide and deep samples. This evolution is computed as an absolute rest-frame B-band magnitude evolution at constant stellar mass, from the comparison of the luminosity-metallicity (see Fig. 12 and Table 6) and mass-metallicity (see Fig. 13 and Table 7) relations.
  $\Delta M_{{\rm AB}}(B)$
Redshift range wide deep
 0.0<z<0.5 -0.06 0.65
 0.5<z<0.7 -0.61 -0.10
 0.7<z<0.9 -1.19 -0.45

Source LaTeX | All tables | In the text

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