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- A 210 Megaparsec Ionized Structure at z=6.8 Revealed by an Astrophysics Foundation Model
- Bayesian Inference of the Tip of the Red Giant Branch: I. One-Dimensional Analysis
- Resolved SED modelling with JWST and ALMA: the role of stellar mass surface density in regulating star formation in cosmic noon galaxies
- Little Red Dots are Direct-Collapse Black Hole-Forming Galaxies
- Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing
- CausticFlow: An Efficient Machine Learning Framework Combining Neural Differential Equations and Normalizing Flows for Binary Microlensing Parameter Inference
- Boundary-supported radial layering in Hoag-like ring galaxies
- A deep learning approach to member identification and mass estimation in galaxy clusters
- CHEX-MATE: AMALGAM weak-lensing analysis of 41 Planck Sunyaev--Zel'dovich-selected galaxy clusters
- Pushing HST to the limit. Detection completeness and morphology robustness of faint galaxies in the Extended Groth Strip field
- Constrain the size of broad-line region in NGC 1068 using submillimetre excess
- Model-dependent metallicities of young stellar populations in TIMER galaxies
- A possible detection of gas rotation in galaxy groups via the kinetic Sunyaev–Zeldovich effect
- Outflows in a super-Eddington quasar drive clumpy circumgalactic medium and extended H α nebulae at z ≳ 6
- Effects of Viscosity on Sloshing Cold Fronts in Galaxy Clusters
- Making Euclid VIS Imaging AI-ready: A Scalable Pipeline for Morphology, Anomaly Detection, and Similarity Search
- Optimizing Photometric Redshift Training Sets. I. Efficient Compression of the Galaxy Color–Redshift Relation with UMAP
- Cosmic web Lyα emission in a sample of overdense regions
- Are supernovae driving turbulence in the solar neighborhood?
- A unified stochastic random walk theory for Kolmogorov spectrum, halo mass functions, and halo density profiles
- Optical spectropolarimetry of extreme H α line profiles in seven active galactic nuclei
- ROLLIN': Rotating Globular Cluster Simulations: II. The complex morphology of globular clusters driven by multi-scale dynamics
- The Lumina Project: Intergalactic Clumping and Recombination Sinks
- Identifying the principal mechanism of star formation feedback
- Henrietta Leavitt's classical Cepheid relation