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Povi?, M. ; Sánchez Portal, M. ; Pérez García, A. M. ; Bongiovanni, A. ; Cepa, J. ; Huertas Company, M. ; Lara López, M. A. ; Fernández Lorenzo, M. ; Ederoclite, A. ; Alfaro, E. ; Castañeda, H. ; Gallego Maestro, Jesús ; González Serrano, J. I. ; González, J. J. | EDP Sciencies | 2012-05Context. The connection between active galactic nuclei (AGN) and their host galaxies has been widely studied and found to be of great importance for providing answers to some fundamental questions related to AGN fuelling mechanisms, and both the[...]texto impreso
Huertas Company, M. ; Gravet, R. ; Cabrera Vives, G. ; Pérez González, Pablo Guillermo ; Kartaltepe, J. S. ; Barro, G. ; Bernardi, M. ; Mei, S. ; Shankar, F. ; Dimauro, P. ; Bell, E. F. ; Kocevski, D. ; Koo, D. C. ; Faber, S. M. ; Mcintosh, D. H. | University Chicago Press | 2015-11We present a catalog of visual-like H-band morphologies of ~50.000 galaxies (H_f160wtexto impreso
Huertas Company, M. ; Bernardi, M. ; Pérez González, Pablo Guillermo ; Ashby, M. L. N. ; Barro, G. ; Conselice, C. ; Daddi, E. ; Dekel, A. ; Dimauro, P. ; Faber, S. M. ; Grogin, N. A. ; Kartaltepe, J. S. ; Kocevski, D. D. ; Koekemoer, A. M. ; Koo, D. C. ; Mei, S. ; Shankar, F. | Wiley | 2016-11-11We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ? 3 to the present. Our sample consists of ?50?000 galaxies in the CANDELS fields (?880 arcmin^2), which we [...]texto impreso
Huertas Company, M. ; Pérez González, Pablo Guillermo ; Mei, S. ; Shankar, F. ; Bernardi, M. ; Daddi, E. ; Barro, G. ; Cabrera Vives, G. ; Cattaneo, A. ; Dimauro, P. ; Gravet, R. | American Astronomical Society | 2015-08-10We quantify the morphological evolution of z ~ 0 massive galaxies (M_*/M_? ?10^11.2 +/- 0.3) from z ~ 3 in the 5 CANDELS fields. The progenitors are selected using abundance matching techniques to account for the mass growth. At z
