40 citations · 134 across the 8 of their papers we have counts for
8 papers
Probing the Star Formation Main Sequence down to M at
Rosa M. Mérida, Pablo G. Pérez-González, Patricia Sánchez-Blázquez +8
We investigate the star formation main sequence (MS) (SFR-M) down to 10 using a sample of 34,061 newly-discovered ultra-faint ($27\lesssim i \less…
Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
Néstor Espino-Briones, Pablo G. Pérez-González, Jaime Zamorano +1
We study in detail the properties of the stellar populations of 111 massive ( dusty (FIR-selected) starburst () gal…
From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
L. Costantin, P. G. Pérez-González, J. Méndez-Abreu +9
We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface bri…
Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field
L. Rodríguez-Muñoz, G. Rodighiero, P. G. Pérez-González +21
We use a sample of 706 galaxies, selected as [OII]3727 ([OII]) emitters in the Survey for High- Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to stud…
A duality in the origin of bulges and spheroidal galaxies
L. Costantin, P. G. Pérez-González, J. Méndez-Abreu +11
Studying the resolved stellar populations of the different structural components which build massive galaxies directly unveils their assembly history. We aim at characterizing the…
SHARDS: Constraints on the dust attenuation law of star-forming galaxies at z~2
M. Tress, E. Mármol-Queraltó, I. Ferreras +11
We make use of SHARDS, an ultra-deep (<26.5AB) galaxy survey that provides optical photo-spectra at resolution R~50, via medium band filters (FWHM~150A). This dataset is combined w…