High-energy astrophysics
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- Supermassive black hole binaries in the multi-messenger context of ground and spaceborne VLBI
- Wind-confined jet collimation revealed by the acceleration-phase photosphere of GRB 220426A
- Enhancing the Angular Resolution of Large Array of imaging atmospheric Cherenkov Telescope (LACT) at Ultra-High Energies
- The first IXPE view of the eclipsing ADC source 4U 1822-37
- The impact of flickering variability and magnetisation on the dynamics, stability and morphology of radio-loud AGN jets
- Broad-band spectral-timing: simultaneous NICER and HXMT observations reveal an anticorrelation between the softest and hardest X-ray fluxes in MAXI J1820+070
- Strange Quark Stars and Spontaneous Scalarization
- Heavy Inert Doublet Reconciles LZ and IceCube
- Dissecting the variability of Sagittarius A* in the orbiting hotspot framework
- A comprehensive multi-wavelength study of two X-ray emitting Be stars
- Tomography analysis of the intermediate-luminosity Type Iax SN 2024pxl
- Stability of hybrid stars via catastrophe theory
- Plasma instability splits axion-photon conversion lines
- Composition-dependent acceleration of UHE Cosmic Rays in AGN electric fields
- 3D Radiation Hydrodynamics of Blue Supergiant Envelopes
- Dynamically Stable Magnetic Fields in Relativistic Neutron Stars: A Diverse Landscape of GRMHD Equilibria
- AstroGenesis: A Domain-Specific Multi-Agent AI for Astrophysical Research
- Finite-Temperature Axion-Admixed Neutron Stars in a Quarkyonic Crossover Framework
- First Pre-peak Ultraviolet Spectrum of a Tidal Disruption Event: A Fast Outflow Revealed Prior to Maximum Light in TDE2025aarm
- Performance-portable GPU acceleration of the hybrid particle-in-cell code dHybridR
- A Tentative Line-like GeV Excess in Fermi Blazar 4FGL J1754.2+3212: Implications for Jet Physics and Beyond
- Study of blazar variability through their flux distribution for CTAO long-term monitoring
- 4U 1624-490 as a possible intermediate-mass X-ray binary: constraints from XRISM and NuSTAR spectroscopy
- Radio component of the multi-messenger emission from the anticipated T Coronae Borealis outburst
- Gamma-ray emission toward supergiant shells in the Large Magellanic Cloud