Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey - I. The evolution of the mass-metallicity relation up to z ~ 0.9

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Table 4:

Limiting masses (in logarithm of solar masses) of our various samples in order to define volume-limited samples, as a function of the redshift ranges and for various mass-to-light completeness levels.
	z<0.5			z<0.6			z<0.7			z<0.8			z<0.9
	50%	80%	95%	50%	80%	95%	50%	80%	95%	50%	80%	95%	50%	80%	95%
wide (all)	9.6	10.0	10.2	9.7	10.2	10.4	9.9	10.3	10.6	10.0	10.5	10.7	10.2	10.6	10.9
wide (star-forming)	9.3	9.6	9.9	9.4	9.7	10.1	9.6	9.9	10.2	9.7	10.0	10.3	9.8	10.1	10.4
deep (all)	8.7	9.2	9.5	8.9	9.3	9.7	9.0	9.5	9.9	9.1	9.6	10.0	9.2	9.7	10.1
deep (star-forming)	8.6	8.9	9.2	8.7	9.0	9.3	8.8	9.0	9.3	8.8	9.1	9.4	8.9	9.2	9.5

Source LaTeX | All tables | In the text

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