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Expanded Sample of Small Magellanic Cloud Ultraviolet Dust Extinction Curves: Correlations between the 2175 Å Bump, q <SUB>PAH</SUB>, Ultraviolet Extinction Shape, and N(H I)/A(V) |
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Age of Massive Galaxies at Redshift 8 |
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PHANGS-JWST: Data-processing Pipeline and First Full Public Data Release |
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PHANGS-HST Catalogs for ∼100,000 Star Clusters and Compact Associations in 38 Galaxies. I. Observed Properties |
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Generic low-atmosphere signatures of swirled-anemone jets |
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The SRG/eROSITA All-Sky Survey. Dark Energy Survey year 3 weak gravitational lensing by eRASS1 selected galaxy clusters |
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Combining magneto-hydrostatic constraints with Stokes profile inversions. IV. Imposing ∇⋅B = 0 condition |
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LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies |
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The Early Data Release of the Dark Energy Spectroscopic Instrument |
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Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal). I. The formation and evolution of the thin disc from the Gaia Catalogue of Nearby Stars |
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The colliding-wind binary HD 168112 |
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Search and analysis of giant radio galaxies with associated nuclei (SAGAN). IV. Interplay with the Supercluster environment |
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A fast neural emulator for interstellar chemistry |
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The CAVITY project: The spatially resolved stellar population properties of galaxies in voids |
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TESS Hunt for Young and Maturing Exoplanets (THYME). X. A Two-planet System in the 210 Myr MELANGE-5 Association |
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The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201 |
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Exploring galaxy evolution time-scales in clusters: insights from the projected phase space |
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CosmoMIA: cosmic web-based redshift space halo distribution |
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Update on WASP-19 |
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Precise characterisation of HD 15337 with CHEOPS: A laboratory for planet formation and evolution |
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HIP 41378 observed by CHEOPS: Where is planet d? |
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The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ∼ 2 |
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Galaxy merger challenge: A comparison study between machine learning-based detection methods |
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Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances, and intracluster light from a semi-empirical perspective |
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Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies |
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