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Euclid preparation : XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
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Self-consistent dynamical models with a finite extent : II. Radially truncated models
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Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at z ∼ 7
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The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved H <scp>i</scp> maps
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UV to submillimetre luminosity functions of TNG50 galaxies
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The distribution of dust in edge-on galaxies : I. The global structure
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MIGHTEE-HI : the relation between the HI gas in galaxies and the cosmic web
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Dust grain size evolution in local galaxies : a comparison between observations and simulations
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Dust masses for a large sample of core-collapse supernovae from optical emission line asymmetries : dust formation on 30-year time-scales
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SOFIA/HAWC+ observations of the Crab Nebula : dust properties from polarised emission