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- The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation
- Gravitational-wave parameter estimation with machine-learning generated surrogate waveforms
- Impact of the equation of state on core collapse supernovae I: the low-T/|W| instability
- Flashing with colours: Photometric indicators of an early interaction in type II supernovae
- Entering the Era of Circumplanetary Ring Detection with Direct Imaging
- Detecting Exoplanetary Rings with Roman CGI Reflected Light Phase Curve Observations
- Revisiting the Mass and Scale Dependence of the "Lensing is Low" Effect with DECADE
- ENFR: Evidence Networks with Flow-Matched References for Amortized Simulation-Based Model Inference
- Learning without relearning physical symmetry: an SO(3)-equivariant convolutional network (CNN) on the sphere
- Gravitational Waves as a Probe of Multi-Fluid Cosmologies: General Formalism and the Case of Cosmological Stasis
- A precessing AGN with S-shaped morphology discovered in MALS
- Foreground dependence of the 20 GeV Galactic halo gamma-ray excess and its proposed connection to the LUX-ZEPLIN event
- Characterizing the Martin Luther King Event: Sun to Earth Evolution of the January 19, 2026 Geomagnetic Storm
- BRISK: An accelerated wide-field imager for radio astronomy
- Hidden Sector Relic Abundances from an Effective Planck Mass
- Does the inverse distance ladder rule out late-time solutions to the Hubble tension? A model-independent test using DES-Dovekie supernovae and DESI DR2 BAO
- Survey of Orion Disks with ALMA (SODA) IV: Millimeter variability of protoplanetary disks
- A Hectospec Spectroscopic Census of Kinematic Members in the Orion Nebula Cluster
- Principle of no paradoxical Universe
- Andreev Beta Conversion and Bulk Viscosity in Superfluid Neutron-Star Matter
- Galaxy bias of radio AGN and star-forming galaxies from MIGHTEE and CMB lensing
- Possible detection of Baryon Acoustic Oscillations imprinted in the HI sources from the FASHI catalog
- The metric-affine mathringR2 scalaron: parameter-free inflation
- The Atmospheric Chemistry and Surface Interactions on Mars (ACSIOM) Workshop 2025
- Can coupled thawing quintessence reproduce DESI DR2? A test with two potentials