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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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MIGHTEE-H I: the M_HI – M* relation over the last billion years
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Self-consistent dynamical models with a finite extent – III. Truncated power-law spheres
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The atomic-to-molecular hydrogen transition in the TNG50 simulation : using realistic UV fields to create spatially resolved H I maps
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Non-parametric galaxy morphology from stellar and nebular emission with the CALIFA sample
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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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Spatially resolved mock observations of stellar kinematics : full radiative transfer treatment of simulated galaxies
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Paradigmatic examples for testing models of optical light polarization by spheroidal dust
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MIGHTEE-H I : possible interactions with the galaxy NGC 895