The VIMOS-VLT deep survey - galaxy luminosity function per morphological type 
up to z = 1.2

Ilbert, O.; Lauger, S.; Tresse, L.; Buat, V.; Arnouts, S.; Le Fèvre, O.; Burgarella, D.; Zucca, E.; Bardelli, S.; Zamorani, G.; Bottini, D.; Garilli, B.; Le Brun, V.; Maccagni, D.; Picat, J. P.; Scaramella, R.; Scodeggio, M.; Vettolani, G.; Zanichelli, A.; Adami, C.; Arnaboldi, M.; Bolzonella, M.; Cappi, A.; Charlot, S.; Contini, T.; Foucaud, S.; Franzetti, P.; Gavignaud, I.; Guzzo, L.; Iovino, A.; McCracken, H. J.; Marano, B.; Marinoni, C.; Mathez, G.; Mazure, A.; Meneux, B.; Merighi, R.; Paltani, S.; Pellò, R.; Pollo, A.; Pozzetti, L.; Radovich, M.; Bondi, M.; Bongiorno, A.; Busarello, G.; Ciliegi, P.; Mellier, Y.; Merluzzi, P.; Ripepi, V.; Rizzo, D.

doi:10.1051/0004-6361:20053632

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The VIMOS-VLT deep survey - galaxy luminosity function per morphological type up to z = 1.2

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

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Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnouts, S., Le Fèvre, O., et al. (2006). The VIMOS-VLT deep survey - galaxy luminosity function per morphological type up to z = 1.2. Astronomy & Astrophysics, 453(3), 809-815. doi:10.1051/0004-6361:20053632.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-AEC3-7

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