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- When precise inference is wrong: Diagnosing model misspecification with applications to cosmic dawn and reionisation
- Chaos and loss: reevaluating the loss-cone formalism in the context of chaotic diving orbits in flattened potentials
- SEAMLESS Survey: A Closer Look at Seven Local Volume Dwarf Galaxies in Diverse Environments
- What becomes of JWST/NIRCam-selected high-redshift massive galaxies?
- The δ Scuti instability strip and period-luminosity relation as seen by TESS and Gaia DR3
- PRISMS GHZ8: Evidence for a Young Burst and Potential Merger Activity at z=10.23
- The Conditional CMB Visibility of High-Redshift X-Ray Cavities in Galaxy clusters
- From Dispersion to Metallicity: Probing the Milky Way Circumgalactic Medium with Fast Radio Bursts
- The unresolved high-mass frontier of the black hole Fundamental Plane
- An Empirically Calibrated [C II] Luminosity-Halo Mass Relation for Line Intensity Mapping
- The IRAC Distant Cluster Survey
- UNIONS: Red and blue alignments of DESI DR1 galaxies
- On the Proper 3D Modeling of Orbits in Wide Binary Gravity Tests
- Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) VIII. First interstellar detection of fully deuterated methyl cyanide
- Playing CHESS with stars II. Homogeneous analysis of high-resolution optical spectra for a sample of 135 giants in 14 bulge globular clusters
- Toward a Complete Interpretation of Global 21 cm Absorption Signals Using the Radio CMB
- A compact NH2D source without NH3 counterpart in the S187 high-mass star-forming region
- Celia: Catalog Embeddings Learned from cosmologIcal simulAtions
- What kinds of strong star--black-hole encounters in AGN disks occur, and how often?
- GroArnold: A Framework for Constructing Action-based Models for Triaxial Galaxies and Dark Matter Halos
- Super-Eddington Accretion and Early-Stage Feedback in Ton S180
- Evolution of Binaries Under Stochastic Perturbations
- A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies
- Extracting non-Gaussian information of line-intensity maps with weighted skew spectra
- Can the ∼ 5 kpc starburst ring in MW create eROSITA bubbles?