251 citations · 454 across the 13 of their papers we have counts for
13 papers
High-redshift quasars along the Main Sequence
A. Deconto-Machado, A. del Olmo, P. Marziani +2
We aim to evaluate the behaviour of our 22 high-redshift (2.2 < z < 3.7) and high-luminosity (47.39 < Lbol < 48.36) quasars in the context of the 4-Dimensional Eigenvector 1. Our a…
Stellar populations of galaxies in the ALHAMBRA survey up to . IV. Properties of quiescent galaxies on the stellar masssize plane
L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuan +7
We perform a comprehensive study of the stellar population properties of quiescent galaxies as a function of size and stellar mass to constrain the physical mechanism governing the…
Extreme quasars at high redshift
M. L. Martınez-Aldama, A. Del Olmo, P. Marziani +5
Context:Quasars radiating at extreme Eddington ratios (xA) are likely a prime mover of galactic evolution and have been hailed as potential distance indicators. Their properties ar…
Intrinsic and observed dual AGN fractions from major mergers
J. M. Solanes, J. D. Perea, G. Valentí-Rojas +4
A suite of 432 collisionless simulations of bound pairs of spiral galaxies with mass ratios 1:1 and 3:1, and global properties consistent with the CDM paradigm, is used to test…
Stellar populations of galaxies in the ALHAMBRA survey up to . III. The stellar content of the quiescent galaxy population during the last Gyr
L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuan +27
We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since up to the present ti…
High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis
K. Viironen, C. López-Sanjuan, C. Hernández-Monteagudo +30
Context. Knowing the exact shape of the UV luminosity function of high-redshift galaxies is important in order to understand the star formation history of the early universe. Howev…