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ON THE EXTENDED KNOTTED DISKS OF GALAXIES
(2007-07)
The stellar disks of many spiral galaxies are twice as large as generally thought. We use archival data from the
Galaxy Evolution Explorer mission to quantify the statistical properties of young stellar clusters in the ...
Occurrence of LINER galaxies within the galaxy group environment
(Oxford University Press, 2017-05)
We study the properties of a sample of 3967 low-ionization nuclear emission-line region (LINER) galaxies selected from SDSS-DR7, with respect to their proximity to galaxy groups. The host galaxies of LINERs have been ...
Dissecting galaxy triplets in the Sloan Digital Sky Survey Data Release 10 - I. Stellar populations and emission line analysis
(Wiley Blackwell Publishing, Inc, 2016-04)
We identify isolated galaxy triplets in a volume-limited sample from the Sloan Digital Sky Survey Data Release 10. Our final sample has 80 galaxy systems in the redshift range 0.04 ≤ z ≤ 0.1, brighter than Mr = −20.5 + ...
Filaments in VIPERS: Galaxy quenching in the infalling regions of groups
(Wiley Blackwell Publishing, Inc, 2019-03)
We study the quenching of galaxies in different environments and its evolution in the redshift range 0.43 ≤ z ≤ 0.89. For this purpose, we identify galaxies inhabiting filaments, the isotropic infall region of groups, the ...
Ring galaxies in the EAGLE hydrodynamical simulations
(Wiley Blackwell Publishing, Inc, 2018-12)
We study the formation and evolution of ring galaxies in the Evolution and Assembly of GaLaxies and their Environments (EAGLE) simulations. We use the largest reference model Ref-L100N1504, a cubic cosmological volume of ...
The galaxy size – halo mass scaling relations and clustering properties of central and satellite galaxies
(Oxford University Press, 2021-08)
In this work, we combine size and stellar mass measurements from the Sloan Digital Sky Server (SDSS) with the group finder algorithm of Rodriguez & Merchán in order to determine the stellar and halo mass-size relations of ...
Following the crumbs: Statistical effects of ram pressure in galaxies
(Oxford University Press, 2020)
Early-type galaxies in the Antlia cluster: Catalogue and isophotal analysis
(Wiley Blackwell Publishing, Inc, 2018-06)
We present a statistical isophotal analysis of 138 early-type galaxies in the Antlia cluster, located at a distance of ~35 Mpc. The observational material consists of CCD images of four 36 ×36 arcmin2 fields obtained with ...
The evolution of the star formation rate function and cosmic star formation rate density of galaxies at z ∼ 1–4
(Royal Astronomical Society, 2017)
We investigate the evolution of the galaxy star formation rate function (SFRF) and cosmic star
formation rate density (CSFRD) of z ∼ 1–4 galaxies, using cosmological smoothed particle
hydrodynamic (SPH) simulations and ...