activity
20142019
most citedThe EAGLE project: Simulating the evolution and assembly of galaxies and their environments

3.7k citations · 4.4k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA201936 cited

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…

astro-ph.GA201680 cited

The Herschel Exploitation of Local Galaxy Andromeda (HELGA) VII: A SKIRT radiative transfer model and insights on dust heating

S. Viaene, M. Baes, A. Tamm +17

The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in gala…

astro-ph.GA20166 cited

Radiative transfer in disc galaxies V. The accuracy of the KB approximation

Dukhang Lee, Maarten Baes, Kwang-Il Seon +3

We investigate the accuracy of an approximate radiative transfer technique that was first proposed by Kylafis & Bahcall (hereafter the KB approximation) and has been popular in mod…

astro-ph.GA2016127 cited

Far-infrared and dust properties of present-day galaxies in the EAGLE simulations

Peter Camps, James W. Trayford, Maarten Baes +3

The EAGLE cosmological simulations reproduce the observed galaxy stellar mass function and many galaxy properties. In this work, we study the dust-related properties of present-day…

astro-ph.IM2014304 cited

SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture

Peter Camps, Maarten Baes

We discuss the architecture and design principles that underpin the latest version of SKIRT, a state-of-the-art open source code for simulating continuum radiation transfer in dust…

astro-ph.GA201499 cited

High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51

Ilse De Looze, Jacopo Fritz, Maarten Baes +20

Context: Dust reprocesses about half of the stellar radiation in galaxies. The thermal re-emission by dust of absorbed energy is considered driven merely by young stars and, conseq…