32 citations · 249 across the 28 of their papers we have counts for
7 papers · 1 filter
GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
Zeleke Beyoro-Amado, Miguel Sánchez-Portal, Angel Bongiovanni +9
Although ZwCl0024+1652 galaxy cluster at has been thoroughly analysed, it lacks a comprehensive study of star formation and nuclear activity of its members. With GaLAxy…
Galaxy classification: deep learning on the OTELO and COSMOS databases
José A. de Diego, Jakub Nadolny, Ángel Bongiovanni +19
Context. The accurate classification of hundreds of thousands of galaxies observed in modern deep surveys is imperative if we want to understand the universe and its evolution. Aim…
The OTELO survey: Nature and mass-metallicity relation for H emitters at
Jakub Nadolny, Maritza A. Lara-López, Miguel Cerviño +14
A sample of low-mass H emission line sources (ELS) at was studied in the context of the mass-metallicty relation (MZR) and its possible evolution. We drew our sam…
The OTELO survey. A case study of [O III]4959,5007 emitters at <z> = 0.83
Ángel Bongiovanni, Marina Ramón-Pérez, Ana María Pérez García +22
The OTELO survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is designed for finding emission-line sources (ELSs). The survey design, obs…
The OTELO survey. III. Demography, morphology, IR luminosity and environment of AGN hosts
Marina Ramón-Pérez, Ángel Bongiovanni, Ana Mará Pérez García +16
We take advantage of the capabilities of the OTELO survey to select and study the AGN population in the field. We performed an analysis of the properties of these objects, includin…
The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue
Ángel Bongiovanni, Marina Ramón-Pérez, Ana Mará Pérez García +21
The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The OTELO survey aims to provide the deepest narrow-band survey to date…
The OTELO survey. II. The faint-end of the H luminosity function at z 0.40
Marina Ramón-Pérez, Ángel Bongiovanni, Ana María Pérez García +16
We take advantage of the capability of the OTELO survey to obtain the H luminosity function (LF) at . Because of the deepest coverage of OTELO, we are able to d…