56 citations · 105 across the 10 of their papers we have counts for
10 papers
Non-Sequential Neural Network for Simultaneous, Consistent Classification and Photometric Redshifts of OTELO Galaxies
José A. de Diego, Jakub Nadolny, Ángel Bongiovanni +17
Context. Computational techniques are essential for mining large databases produced in modern surveys with value-added products. Aims. This paper presents a machine learning proced…
The OTELO survey: Revealing a population of low-luminosity current/active star-forming galaxies at z
Rocío Navarro Martínez, Ana María Pérez-García, Ricardo Pérez-Martínez +16
We study a sample of H emission line sources at 0.9 to identify the star-forming (SF) galaxies sample and characterise them in terms of line luminosity, stellar mass, SFR…
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…
Fast outflows in broad absorption line quasars and their connection with CSS/GPS sources
G. Bruni, K. -H. Mack, F. M. Montenegro-Montes +2
Broad absorption line quasars are among the objects presenting the fastest outflows. The launching mechanism itself is not completely understood. Models in which they could be laun…
San Pedro Martir observations of microvariability in obscured quasars
Jana Polednikova, Alessandro Ederoclite, Jordi Cepa +9
Fast brightness variations are a unique tool to probe the innermost regions of active galactic nuclei (AGN). These variations are called microvariability or intra-night variability…
Investigating the radio-loud phase of broad absorption line quasars
G. Bruni, J. I. González-Serrano, M. Pedani +5
Broad absorption lines (BALs) are present in the spectra of ~20% of quasars (QSOs); this indicates fast outflows (up to 0.2c) that intercept the observer's line of sight. These QSO…
The parsec-scale structure of radio-loud broad absorption line quasars
G. Bruni, D. Dallacasa, K. -H. Mack +4
Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood as yet. Their UV spectra show BALs in the blue wings of the UV resonance lines, owing to i…
X-ray luminosity functions of different morphological and X-ray type AGN populations
M. Pović, A. M. Pérez García, M. Sánchez-Portal +12
Luminosity functions are one of the most important observational clues when studying galaxy evolution over cosmic time. In this paper we present the X-ray luminosity functions of X…
AGN-Host Galaxy Connection: Morphology and Colours of X-ray Selected AGN at z < 2
M. Pović, M. Sánchez-Portal, A. M. Pérez García +11
The connection between AGN and their host galaxies has been widely studied over recent years, showing it to be of great importance for providing answers to some fundamental questio…
VLBA imaging of radio-loud Broad Absorption Line QSOs
F. M. Montenegro-Montes, K. -H. Mack, C. R. Benn +5
Broad Absorption Line Quasars (BAL QSOs) have been found to be associated with extremely compact radio sources. These reduced dimensions can be either due to projection effects or…