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

F. Lamareille; J. Brinchmann; T. Contini; C. J. Walcher; S. Charlot; E. Pérez-Montero; G. Zamorani; L. Pozzetti; M. Bolzonella; B. Garilli; S. Paltani; A. Bongiorno; O. Le Fèvre; D. Bottini; V. Le Brun; D. Maccagni; R. Scaramella; M. Scodeggio; L. Tresse; G. Vettolani; A. Zanichelli; C. Adami; S. Arnouts; S. Bardelli; A. Cappi; P. Ciliegi; S. Foucaud; P. Franzetti; I. Gavignaud; L. Guzzo; O. Ilbert; A. Iovino; H. J. McCracken; B. Marano; C. Marinoni; A. Mazure; B. Meneux; R. Merighi; R. Pellò; A. Pollo; M. Radovich; D. Vergani; E. Zucca; A. Romano; A. Grado; L. Limatola

doi:10.1051/0004-6361:200810397

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Volume 495 / No 1 (February III 2009)

A&A, 495 1 (2009) 53-72

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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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