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- Cosmic-Ray Signals from Dark Matter Annihilation into Scalars with Baryon Number
- The formation of the first cosmic structures in hybrid Milgromian cosmology
- De-lensing cosmic birefringence with joint reconstruction
- GPUPhot: Kernel-Based Algorithms for Point-Source Detection and Photometry with a Spatially Variable PSF
- Gauge-invariant non-universal scalar couplings in teleparallel gravity
- Can cosmic voids ease the Hubble tension? Local expansion in w0waCDM
- Hybrid stars with hyperons: structure based on QCD sum rule coupling constants
- Direct evidence of non-ideal MHD in the solar wind and switchbacks
- Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model
- Episodic Star Formation - II. The Origin of the Fundamental Metallicity Relation
- The Neptunian ridge through the lens of TESS
- Mercury (Hg): a relativistic N-body simulation for Horndeski gravity
- The Giant Planet Mass Function Across Stellar Mass and Metallicity: Massive Stars Make Massive Planets
- Detection of the Galaxy--Galaxy--Temperature Skewed Bispectrum
- Nonlinear gauge maps and the structure of Goldstone loops in canonical inflation
- Chemical and dynamical evolution of prestellar cores, the dawn of star and planet formation
- Episodic Protostellar Outflows: A Proper Motion Study in Serpens South
- Toward the one- and two-loop EFTofLSS for Simons Observatory CMB lensing
- VLITE Observations of the Hubble Ultra Deep Field
- Baryonic feedback and intrinsic alignments in profile: a frequentist view of DES Y3 cosmic shear
- Multiprobe strategies for Kinematic Lensing with the Roman Space Telescope High Latitude Wide Area Survey
- A heteroskedasticity and autocorrelation consistent test for process noise calibration of Kalman filters in multi-sensor orbit determination
- A Physics Informed Neural Network Approach to Decipher Environmental Confinement of Molecular Clouds in the Third Galactic Quadrant
- DBI Softens Stiff-Phase Gravitational-Wave Spectra
- HCN detection in the Kreutz sungrazing comet C/2026 A1 (MAPS) shortly before its disruption