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- Reconstructing the Large-Scale Velocity Field from DESI DR1 with Bayesian Inference
- Disruption limits around triaxial bodies and implications for ring-bearing minor bodies
- The TNG50-SKIRT Atlas: Multi-wavelength properties of galaxy discs in the TNG50 simulation
- Limits to research in astrophysics
- A Unified AI Framework for Rapid and Accurate Waveform Generation of Compact Binary Coalescences
- Quark deconfinement as a natural trigger of Type-I critical collapse: black holes from neutron stars deemed stable
- Multimuon Events from Cosmic Rays with the ALICE Detector
- Outer pressure bumps beyond the dust disc: Missing Outer Rings in the exoALMA Sample: Physical Mechanisms Suppressing Dust Ring Formation Despite Strong Pressure Bumps
- Feature-Based and Deep Learning Methods for Astronomical Light Curve Classification
- MAGIC's interferometric diameters of θ Ophiuchi and β CMa and comparison with asteroseismic modelling
- Efficient Identification and Analysis of Space debris Trails in Time-Domain Astronomy
- Probing the Faint Outskirts of Star-Forming Galaxies with 1<z<9 Using Stacked Images
- A Detailed Polarimetric Imaging Study of Type II Solar Radio Burst with the MWA: Detection of Linear Polarization
- Up in smoke: carbon-destruction in the terrestrial planet-forming region of a young Class I disk
- The Survival Paradox of Close-In Planets Orbiting Red Clump Giants
- Late-time echoes from planar wave-packet scattering by an ultracompact star
- Structural axes of sources in the SUMSS survey and their alignments
- Photometric calibration of the 4m ILMT data
- Stress-Testing Small-Scale Cosmological Inference With Empirical Galaxy--Halo Connection Models
- Spin Spherical Fourier Neural Operators: Efficient Equivariant Learning for Vector and Spin Fields on the Sphere
- How Fast do Black Holes Spin?
- HI Emission Recovery in the Low-Redshift Radio Population: Host-Galaxy and Radio-Luminosity Dependence in FASHI and LoTSS
- Fitting Resonant Exoplanets Orbits. I. Properties and Applications of Fixed-Point Orbits
- Constraining Dust Properties Along the Minor Axis of Andromeda
- Measuring the ultraviolet background at z≃3 from the quasar proximity effect in DESI DR1