394 citations · 839 across the 19 of their papers we have counts for
19 papers
The OTELO Survey: The main sequence of low-mass galaxies
Bernabé Cedrés, Jordi Cepa, Carmen P. Padilla--Torres +15
This paper describes the relationship between the star formation rate and the stellar mass, the so-called main sequence (MS), of low-mass galaxies at three different redshifts from…
Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
M. C. Zerbo, M. E. De Rossi, M. A. Lara-López +2
Effective yields, , are defined by fundamental galaxy properties (i.e., stellar mass --, gas mass -- and gas-phase metallicity). For a closed-b…
Metal-THINGS: a panchromatic analysis of the local scaling relationships of the dwarf irregular galaxy NGC 1569
L. E. Garduño, J. Zaragoza-Cardiel, M. A. Lara-López +12
We investigate several panchromatic scaling relations (SRs) for the dwarf irregular galaxy NGC 1569 using IFU data from the Metal-THINGS Survey. Among the spatially resolved proper…
The Lockman-SpReSO project. Description, target selection, observations and preliminary results
M. González-Otero, C. P. Padilla-Torres, J. Cepa +26
Context. Extragalactic surveys are a key tool for better understanding the evolution of galaxies. Both deep and wide-field surveys serve to provide a clearer emerging picture of th…
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 structure and characteristic scales of the HI gas in galactic disks
Sami Dib, Jonathan Braine, Maheswar Gopinathan +9
The spatial distribution of the HI gas in galaxies holds important clues on the physical processes that shape the structure and dynamics of the interstellar medium (ISM). In this w…
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…
The OTELO survey: Faint end of the luminosity function of [OII] emitters at <z>= 1.43
Bernabé Cedrés, Ángel Bongiovanni, Miguel Cerviño +15
In this paper, we aim to study the main properties and luminosity function (LF) of the [OII] emitters detected in the OTELO survey in order to characterise the star formation proce…
VALES VI: ISM enrichment in star-forming galaxies up to z0.2 using CO(1-0), CO(1-0) and CO(1-0) line luminosity ratios
H. Méndez-Hernández, E. Ibar, K. K. Knudsen +10
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) observations towards 27 low-redshift () star-forming galaxies taken from the Valparaíso ALMA/APEX Line…
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…
VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
V. Villanueva, E. Ibar, T. M. Hughes +24
We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterise galaxy populations up to : the Valparaíso…
Galaxy And Mass Assembly (GAMA): Stellar mass growth of spiral galaxies in the cosmic web
Mehmet Alpaslan, Meiert W. Grootes, Pamela M. Marcum +16
We look for correlated changes in stellar mass and star formation rate along filaments in the cosmic web by examining the stellar masses and UV-derived star formation rates (SFR) o…
Galaxy And Mass Assembly (GAMA): Stellar mass functions by Hubble type
Lee S. Kelvin, Simon P. Driver, Aaron S. G. Robotham +22
We present an estimate of the galaxy stellar mass function and its division by morphological type in the local (0.025 < z < 0.06) Universe. Adopting robust morphological classifica…
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…
Evolution of the Fundamental Plane of 0.2<z<1.2 Early-type galaxies in the EGS
M. Fernández Lorenzo, J. Cepa, A. Bongiovanni +5
The Fundamental Plane relates the structural properties of early-type galaxies such as its surface brightness and effective radius with its dynamics. The study of its evolution has…
Evolution of the infrared Tully-Fisher relation up to z=1.4
M. Fernández Lorenzo, J. Cepa, A. Bongiovanni +4
The Tully-Fisher relation (TFR) represents a connection between fundamental galaxy parameters, such as its total mass and the mass locked in stars. Therefore, the study of the evol…
A fundamental plane for field star-forming galaxies
M. A. Lara-López, J. Cepa, A. Bongiovanni +6
Star formation rate (SFR), metallicity and stellar mass are within the important parameters of star--forming galaxies that characterize their formation and evolution. They are know…
Evolution of the optical Tully-Fisher relation up to z=1.3
M. Fernández Lorenzo, J. Cepa, A. Bongiovanni +5
The study of the evolution of the Tully-Fisher relation has been controversial in the past years. The main difficulty is in determining the required parameters for intermediate and…