127 citations · 832 across the 44 of their papers we have counts for
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Massive Low Surface Brightness Galaxies in the EAGLE Simulation
Andrea Kulier, Gaspar Galaz, Nelson D. Padilla +1
We investigate the formation and properties of low surface brightness galaxies (LSBGs) with in the EAGLE hydrodynamical cosmological simulatio…
From the far-ultraviolet to the far-infrared -- galaxy emission at in the Shark semi-analytic model
Claudia del P. Lagos, Aaron S. G. Robotham, James W. Trayford +8
We combine the Shark semi-analytic model of galaxy formation with the ProSpect software tool for spectral energy distribution (SED) generation to study the multi-wavelength emissio…
Fade to grey: systematic variation of the galaxy attenuation curves with galaxy properties in EAGLE
James W. Trayford, Claudia del P. Lagos, Aaron S. G. Robotham +1
We present a simple model for galaxy attenuation by distilling SKIRT radiative transfer calculations for ~100,000 EAGLE galaxies at redshifts z=2-0. Our model adapts the two compon…
Non-parametric Morphologies of Galaxies in the EAGLE Simulation
Lucas A. Bignone, Susana E. Pedrosa, James W. Trayford +2
We study the optical morphology of galaxies in a large-scale hydrodynamic cosmological simulation, the EAGLE simulation. Galaxy morphologies were characterized using non-parametric…
An evolving and mass dependent - relation for galaxies
Antonios Katsianis, Xianzhong Zheng, Valentino Gonzalez +10
The scatter () of the specific star formation rates (sSFRs) of galaxies is a measure of the diversity in their star formation histories (SFHs) at a given mass…
Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
Ruari Mackenzie, Michele Fumagalli, Tom Theuns +12
We present results from a survey of galaxies in the fields of six z>3 Damped Lyman alpha systems (DLAs) using the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telesco…