118 citations · 681 across the 17 of their papers we have counts for
7 papers · 1 filter
The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
Viviana Casasola, Simone Bianchi, Pieter De Vis +18
The purpose of this work is the characterization of the main scaling relations between all the ISM components (dust, atomic/molecular/total gas), gas-phase metallicity, and other g…
Predicting the global far-infrared SED of galaxies via machine learning techniques
W. Dobbels, M. Baes, S. Viaene +10
Dust plays an important role in shaping a galaxy's spectral energy distribution (SED). It absorbs ultraviolet (UV) to near-infrared (NIR) radiation and re-emits this energy in the…
Dust emissivity and absorption cross section in DustPedia late-type galaxies
S. Bianchi, V. Casasola, M. Baes +16
Aims: We compare the far-infrared to sub-millimetre dust emission properties measured in high Galactic latitude cirrus with those determined in a sample of 204 late-type DustPedia…
The First Maps of -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
Christopher J. R. Clark, Pieter De Vis, Maarten Baes +17
The dust mass absorption coefficient, , is the conversion function used to infer physical dust masses from observations of dust emission. However, it is notoriously poorly c…
Old and young stellar populations in DustPedia galaxies and their role in dust heating
A. Nersesian, E. M. Xilouris, S. Bianchi +19
Within the framework of the DustPedia project we investigate the properties of cosmic dust and its interaction with the stellar radiation (originating from different stellar popula…
Morphology-assisted galaxy mass-to-light predictions using deep learning
Wouter Dobbels, Serge Krier, Stephan Pirson +4
One of the most important properties of a galaxy is the total stellar mass, or equivalently the stellar mass-to-light ratio (M/L). It is not directly observable, but can be estimat…
The cosmic spectral energy distribution in the EAGLE simulation
Maarten Baes, Ana Trčka, Peter Camps +4
The cosmic spectral energy distribution (CSED) is the total emissivity as a function of wavelength of galaxies in a given cosmic volume. We compare the observed CSED from the UV to…