340 citations · 2.3k across the 100 of their papers we have counts for
100 papers
The Lockman--SpReSO project. Main properties of infrared selected star-forming galaxies
Mauro González-Otero, Jordi Cepa, Carmen P. Padilla-Torres +18
Methods.We applied distinct selection criteria to attain an SFG sample with minimal AGN contamination. Multiple approaches were used to estimate the intrinsic extinction, SFR and g…
The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
Mauro González-Otero, Carmen P. Padilla-Torres, J. Ignacio González-Serrano +20
Methods. We performed measurements of the \MgII, \MgI, \FeIIa, \FeIIb, and \FeIIc\ spectral lines present in the spectra of the selected sample to determine the EW and velocity of…
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…
HR-pyPopStar: high wavelength-resolution stellar populations evolutionary synthesis model
I. Millán-Irigoyen, M. Mollá, M. Cerviño +3
We present the HR-pyPopStar model, which provides a complete set (in ages) of high resolution (HR) Spectral Energy Distributions of Single Stellar Populations. The model uses the m…
Surface Brightness Fluctuations to constrain secondary stellar populations: Revealing very low-metallicity stars in massive galaxies
Pablo Rodriguez Beltran, Alexandre Vazdekis, Miguel Cervino +1
The aim of this work is to explore the potential of Surface Brightness Fluctuations (SBF) for studying composite stellar populations (CSP). To do so, we have computed the standard…
The OTELO survey: the star formation rate evolution of low-mass galaxies
Bernabé Cedrés, Ana María Pérez-García, Ricardo Pérez-Martínez +14
We present the analysis of a sample of \ha\,, \hb\ and \oii\ emission line galaxies from the \otelo\ survey, with masses typically below $log(M_*/M_\sun) \sim 9.4$ and redshifts be…