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APOD: 2026 September 25 – Globular Star Cluster Omega Centauri
LZ nuclear recoil event from inelastic singlet-doublet scalar dark matter
A Fast and Scalable Transformer Pipeline for Binary Black Hole Detection
New benchmarks for direct detection of freeze-in dark matter in vector portal models
Testing a cosmological teleparallel modified f(T) model with parametric H(z)
Supermassive black hole binaries in the multi-messenger context of ground and spaceborne VLBI
Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates
Wind-confined jet collimation revealed by the acceleration-phase photosphere of GRB 220426A
Simulating the convection in red super-giant stars: wobbling jets in common envelope evolution
Does DESI prefer Damped Oscillating Dark Energy over Cosmological constant?
Spectra and Ionization Efficiencies of Charged Decay Particles in Kilonova Ejecta
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions
Illuminating the Local Universe: Large-Scale Structure from ZTF Type Ia Supernovae
Dispersion Measure Distribution of Unlocalized Fast Radio Bursts as a Probe of the Hubble Constant
Gaussian Process Inference of Stochastic Magneto-Active Dynamics and Viscosity in Swift J1727.8-1613
Ising noise filter: physics-informed filtering for particle detectors
Parallel adaptive reweighting importance sampling for Bayesian astrophysics
Radiating Bondi Flows I: Dimensionless Framework and Constant Opacity Solutions
ENhanced Galactic Atmospheres With Arepo: Resolving the CGM at 200 pc with the ENGAWA Simulations
Detection of a puzzling dual-superorbital hard X-ray modulation in the X-ray binary GX 301-2
Superradiant and dynamical spin-down of neutron stars with gravitational wave implications
Event Horizon Telescope Pattern Speeds in the Visibility Domain
Magnetic Field Configurations in Binary Neutron Star Mergers I: Post-merger Remnant and Disk
Discovering $\mu$Hz gravitational waves and ultra-light dark matter with binary resonances
Detecting Extragalactic Axion-like Dark Matter with Polarization Measurements of Fast Radio Bursts
Angular Correlations of Cosmic Microwave Background Spectrum Distortions from Photon Diffusion
The third law of black hole thermodynamics and the mass-to-charge ratio of scalar fields
Stiffness corrections for f-mode neutron star universal relations
Plasma Effects Suppress Mixing-Induced Collisional Freeze-In
Environmental Imprints of Dark Matter and Accretion Disks on Eccentric EMRIs around Kerr Black Holes
Multi-messenger and multi-band signal from first-order phase transitions in proto-neutron stars
Is MOND an Emergent Effective Law of a Complex Dark Matter Sector?
Monte Carlo sampling of first-order QED processes in laser and pulsar plasmas
NASA: Crew-14 mission with Roscosmos astronaut will head to the ISS in 2027
Expedition 75 astronauts continue science work as Crew-13 readies for launch
NASA Shares SpaceX Crew-14 Assignments for Space Station Mission
NASA’s Hubble Telescope Reaches Milestone, Looks for Elusive Supernova
Geomagnetic activity index Kp (GFZ Potsdam, NOAA): 0–3 quiet, 5 and above is a magnetic storm.
Flares are classed by the strength of their X-rays: A and B are weak, C moderate, M strong (can briefly disturb radio), X the most powerful. Each class is 10 times stronger than the one before.