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Simulation-based inference of galaxy properties from JWST pixels |
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Simulation-based inference of galaxy properties from JWST pixels |
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DESI DR1 Lyα 1D power spectrum: the Fast Fourier Transform estimator measurement |
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LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data |
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The spatially resolved effect of mergers on the stellar mass assembly of MaNGA galaxies |
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Euclid: Early Release Observations ─ Interplay between dwarf galaxies and their globular clusters in the Perseus galaxy cluster |
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Atmospheric composition and circulation of the ultra-hot Jupiter WASP-121b with joint NIRPS, HARPS and CRIRES+ transit spectroscopy |
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Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory |
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GX 340+0: In and Out of Focus |
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GATOS. VIII. On the Physical Origin of the Extended Mid-infrared Emission in Active Galactic Nuclei |
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Flavor Phenomenology of Light Dark Sectors |
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Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagittarii |
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Euclid: Star clusters in IC 342, NGC 2403, and Holmberg II |
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Early Coformation of the Milky Way's Thin and Thick Disks at Redshift z > 2 |
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Observation of undepleted phosphine in the atmosphere of a low-temperature brown dwarf |
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UNIONS: The Ultraviolet Near-infrared Optical Northern Survey |
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From simulations to observations: Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS |
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Excitation of Molecular Hydrogen in Seyferts: NGC 5506 and NGC 3081 |
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Optical and near-infrared polarization of the black hole X-ray binary A0620−00 in quiescence |
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Euclid: Finding strong gravitational lenses in the early release observations using convolutional neural networks |
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A Comprehensive Characterization of Galaxy-cool CGM Connections at z < 0.4 with DESI Year 1 Data |
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Dark Energy Survey Year 6 results: cell-based coadds and METADETECTION weak lensing shape catalogue |
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TESS Subgiant and Lower-red-giant Asteroseismology in the Continuous Viewing Zones |
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Using active learning to improve quasar identification for the DESI spectra processing pipeline |
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