activity
20182021
most citedOld and young stellar populations in DustPedia galaxies and their role in dust heating

116 citations · 411 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

17 papers · 1 filter

astro-ph.GA2024

The TNG50-SKIRT Atlas: wavelength dependence of the effective radius

Maarten Baes, Aleksandr Mosenkov, Raymond Kelly +17

Galaxy sizes correlate with many other important properties of galaxies, and the cosmic evolution of galaxy sizes is an important observational diagnostic for constraining galaxy e…

astro-ph.GA2024

The TNG50-SKIRT Atlas: post-processing methodology and first data release

Maarten Baes, Andrea Gebek, Ana Trcka +17

Galaxy morphology is a powerful diagnostic to assess the realism of cosmological hydrodynamical simulations. Determining the morphology of simulated galaxies requires the generatio…

astro-ph.GA202133 cited

High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project

Anand Utsav Kapoor, Peter Camps, Maarten Baes +6

We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiat…

astro-ph.GA20217 cited

Probing the spectral shape of dust emission with the DustPedia galaxy sample

Angelos Nersesian, Wouter Dobbels, Manolis E. Xilouris +10

The objective of this paper is to understand the variance of the far-infrared (FIR) spectral energy distribution (SED) of the DustPedia galaxies, and its link with the stellar and…

astro-ph.GA2020

High-resolution, 3D radiative transfer modelling V. A detailed model of the M51 interacting pair

Angelos Nersesian, Sebastien Viaene, Ilse De Looze +13

Investigating the dust heating mechanisms in galaxies provides a deeper understanding of how the internal energy balance drives their evolution. Over the last decade, radiative tra…

astro-ph.GA202024 cited

High-resolution, 3D radiative transfer modelling IV. AGN-powered dust heating in NGC 1068

S. Viaene, A. Nersesian, J. Fritz +18

Dust emission, an important diagnostic of star formation and ISM mass throughout the Universe, can be powered by sources unrelated to ongoing star formation. In the framework of th…