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Metal and dust evolution in ALMA REBELS galaxies: insights for future <i>JWST</i> observations
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From total destruction to complete survival: dust processing at different evolutionary stages in the supernova remnant Cassiopeia A
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MIGHTEE-H I : the M_HI – M* relation over the last billion years
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A Bayesian chemical evolution model of the DustPedia galaxy M74
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Origin of neutron-capture elements with the Gaia-ESO survey : the evolution of s- and r-process elements across the Milky Way
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Spatially resolved mock observations of stellar kinematics : full radiative transfer treatment of simulated galaxies
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MIGHTEE-H I : possible interactions with the galaxy NGC 895
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MIGHTEE-H I: the first MeerKAT H I mass function from an untargeted interferometric survey
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Population III X-ray binaries and their impact on the early universe
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The problem of dust attenuation in photometric decomposition of edge-on galaxies and possible solutions
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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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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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Size-selective accretion of dust on to CPDs : low CPD masses and filtration of larger grains