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 5:

Limiting B-band absolute magnitudes (AB system) of our wide and deep samples of star-forming galaxies, in order to define volume-limited samples, as a function of the redshift ranges and for various k-correction completeness levels.
	z<0.5		z<0.7		z<0.9
	50%	95%	50%	95%	50%	95%
wide	-19.1	-19.6	-19.9	-20.3	-20.5	-20.9
deep	-17.5	-18.3	-18.2	-18.9	-18.6	-19.3

Source LaTeX | All tables | In the text

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