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

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

doi:10.1051/0004-6361:200810397

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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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Charlot, S.
Cosmology, MPI for Astrophysics, Max Planck Society;

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Lamareille, F., Brinchmann, J., Contini, T., Walcher, C. J., Charlot, S., Pérez-Montero, E., et al. (2009). 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. Astronomy & Astrophysics, 495(1), 53-72. doi:10.1051/0004-6361:200810397.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-A3E7-2

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