@article{
 title = {The zCOSMOS Redshift Survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z~1},
 type = {article},
 year = {2009},
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 keywords = {Galaxy: formation,cosmology: large-scale structure of universe,galaxies: distances and redshifts,galaxies: evolution,galaxies: fundamental parameters,galaxies: structure},
 pages = {379-398},
 volume = {503},
 websites = {http://arxiv.org/abs/0906.4556,http://dx.doi.org/10.1051/0004-6361/200912213,http://arxiv.org/abs/0906.4556%0Ahttp://dx.doi.org/10.1051/0004-6361/200912213},
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 abstract = {For more than two decades we have known that galaxy morphological segregation is present in the Local Universe. It is important to see how this relation evolves with cosmic time. To investigate how galaxy assembly took place with cosmic time, we explore the evolution of the morphology-density relation up to redshift z~1 using about 10000 galaxies drawn from the zCOSMOS Galaxy Redshift Survey. Taking advantage of accurate HST/ACS morphologies from the COSMOS survey, of the well-characterised zCOSMOS 3D environment, and of a large sample of galaxies with spectroscopic redshift, we want to study here the evolution of the morphology-density relation up to z~1 and its dependence on galaxy luminosity and stellar mass. The multi-wavelength coverage of the field also allows a first study of the galaxy morphological segregation dependence on colour. We further attempt to disentangle between processes that occurred early in the history of the Universe or late in the life of galaxies. The zCOSMOS field benefits of high-resolution imaging in the F814W filter from the Advanced Camera for Survey (ACS). We use standard morphology classifiers, optimised for being robust against band-shifting and surface brightness dimming, and a new, objective, and automated method to convert morphological parameters into early, spiral, and irregular types. We use about 10000 galaxies down to I_AB=22.5 with a spectroscopic sampling rate of 33% to characterise the environment of galaxies up to z~1 from the 100 kpc scales of galaxy groups up to the 100 Mpc scales of the cosmic web. ABRIDGED},
 bibtype = {article},
 author = {Tasca, L. A. M. and Kneib, J. P. and Iovino, A. and Fevre, O. Le and Kovač, K. and Bolzonella, M. and Lilly, S. J. and Abraham, R. G. and Cassata, P. and Cucciati, O. and Guzzo, L. and Tresse, L. and Zamorani, G. and Capak, P. and Garilli, B. and Scodeggio, M. and Sheth, K. and Vergani, D. and Zucca, E. and Carollo, C. M. and Contini, T. and Mainieri, V. and Renzini, A. and Bardelli, S. and Bongiorno, A. and Caputi, K. and Coppa, G. and de la Torre, S. and de Ravel, L. and Franzetti, P. and Kampczyk, P. and Knobel, C. and Koekemoer, A. and Lamareille, F. and Borgne, J. F. Le and Brun, V. Le and Maier, C. and Mignoli, M. and Pello, R. and Peng, Y. and Montero, E. Perez and Ricciardelli, E. and Silverman, J. D. and Tanaka, M. and Abbas, U. and Bottini, D. and Cappi, A. and Cimatti, A. and Ilbert, O. and Leauthaud, A. and Maccagni, D. and Marinoni, C. and McCracken, H. J. and Memeo, P. and Meneux, B. and Oesch, P. and Porciani, C. and Pozzetti, L. and Scaramella, R. and Scarlata, C.},
 journal = {Astronomy and Astrophysics, Volume 503, Issue 2, 2009, pp.379-398}
}

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