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Dark Energy Survey Year 3 results: $w$CDM cosmology from simulation-based inference with persistent homology on the sphere
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Dark Energy Survey Year 3 results: Simulation-based $w$CDM inference from weak lensing and galaxy clustering maps with deep learning: Analysis design
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Dark Energy Survey Year 3 results: likelihood-free, simulation-based $w$CDM inference with neural compression of weak-lensing map statistics
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COMAP Pathfinder -- Season 2 results I. Improved data selection and processing
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COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars
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Disruption of a massive molecular cloud by a supernova in the Galactic Centre: Initial results from the ACES project
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SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets
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COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrum
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COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"
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The Hubble Space Telescope Survey of M31 Satellite Galaxies IV. Survey Overview and Lifetime Star Formation Histories
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Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
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Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey
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Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method
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Weak Gravitational Lensing around Low Surface Brightness Galaxies in the DES Year 3 Data
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Effective field theory and inelastic dark matter results from XENON1T
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The Dark Energy Survey Supernova Program: An updated measurement of the Hubble constant using the Inverse Distance Ladder
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Constraining the Stellar-to-Halo Mass Relation with Galaxy Clustering and Weak Lensing from DES Year 3 Data
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Host traits and temperature predict biogeographical variation in seagrass disease prevalence.
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The Dark Energy Survey Supernova Program: Slow supernovae show cosmological time dilation out to $z \sim 1$
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The JWST Resolved Stellar Populations Early Release Science Program VII. Stress Testing the NIRCam Exposure Time Calculator
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SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos
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