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- The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-day Location
- Galaxy Clusters from the DESI Legacy Imaging Surveys. IV. Alignment of Member Galaxy Orientations at z < 0.5
- ALESS–JWST: Dust-driven Morphologies and Hidden Stellar Mass in z ∼ 3 Submillimeter Galaxies
- Black Hole Occupation Fraction: Dependence on Black Hole Mass Threshold, Environment, Resolution, and Redshift
- Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data
- Lensing in the Blue. III. Weak-lensing Shape Catalogs of 30 Merging Galaxy Clusters
- The evolution of the spin alignments of dark matter halos in the cosmic web
- Cosmic rays in galaxy halos I: the circumgalactic transport rate and a dynamically significant cosmic-ray reservoir
- Tidal shells as clocks of galaxy mergers and tests of cosmological models
- The Carousel Lens III: Joint lens convergence and source kinematic modeling
- Simulating and Characterizing Non-Gaussian Small-Scale Polarized Emission
- Validating an X-ray-based method for identifying Fermi blazars
- No Significant Excess in Typical Variability in CLAS+ Changing-Look AGN Candidates in Rubin DP2
- Combining Multiple Incomplete Astronomical Surveys to Estimate Galaxy Flux Distributions
- Simulation-Informed Dust Masses in Typical 6<z<14 JWST Galaxies
- Ejected and Rejected: Strong Scatterings in Dense Star Clusters
- Not so dead after all: young stars in the massive S0 NGC 3115
- Extra! Extra! X-ray Emission!: X-rays in Romulus25, Part II - Physical Drivers of X-ray Emission in the CGM
- Resolving the thermal component of stellar feedback with the "anchor-and-refine" scheme in galactic simulations
- Hot off the Stacks: X-rays in Romulus25, Part I - Comparisons to Observations from eRosita
- Seeing Unseen Gravitational Wave Inspirals at the Galactic Center
- A GLIMPSE of Dark Matter: JWST Constraints on Early Structure Formation
- Identifying Scientifically Interesting Galaxies with Vision-Language Models
- Dark matter haloes from dwarf to massive galaxies: no systematic inner-density tension with ΛCDM hydrodynamical simulations
- HII-CHI-mistry for active galactic nuclei: optical sulphur abundances without empirical ionisation correction factors