High-energy astrophysics
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- First results from PADRE/MeDDEA: X-rays from a flare and its CME
- JWST unveils a dust-obscured supernova associated with a gamma-ray burst
- Assessing the detectability and identification of pulsar halos with H.E.S.S. and CTAO
- Sub-MeV gamma-ray lines from an endothermic interpretation of the LZ recoil candidate
- A Probabilistic Method for Estimating VLBI Jet-Component Ejection Epochs. Application to MOJAVE 15 GHz VLBA Kinematics
- Observations of Repeating Tidal Disruption Events
- Evidence for an extended Galactic proton component beyond the cosmic-ray knee
- Testing Spin Prior Assumptions of Binary Black Hole Parameter Inference and Their Astrophysical Implications
- Probing Solar Chameleons with XENONnT Ionization-Only Data
- Fundamental differences in the X-ray accretion properties of low and high-excitation radio galaxies
- Finite-source magnification residuals from a cNFW-inspired perturbation of an effective spinning black hole binary lens
- Evidence for a Delayed Progenitor Population for CHIME non-repeating Fast Radio Bursts from a Self-Consistent Forward and Backward Inference Framework
- Fermi bubbles detected in ∼100 TeV neutrinos
- A Potential Black Hole Mimicker From Non-Minimal Coupling
- Radiation-induced electron spin polarization in ultrarelativistic kinetic turbulence
- Pulse profiles of tall accretion columns in X-ray pulsars
- Global Spline Fit: A unified data-driven view of the cosmic-ray spectrum and mass composition from GeV to the highest energies
- AGN hosting jets. II: Deriving fundamental information from semi-analytical models and the LoTSS sample
- 15-Year X-ray Study Links Variable Mass Accretion to Changing Look Behavior in AGN NGC 7582
- Constraints on Supermassive Black Hole Binaries from the Lack of Resolvable Sources in the NANOGrav 15-yr Dataset
- Spin wandering of an accreting neutron star near torque balance: implications for gravitational wave searches
- Polarization Signatures of Sgr A* with Tilted Hybrid Magnetic Fields
- Epeak-α Correlation in Time Resolved GRB Spectra: A Bottom-Up Approach with Optically Thin Inverse Compton Scattering Model
- A statistical hardness classification of ultraluminous X-ray sources using long-term Swift/XRT monitoring
- Long-term X-ray variability of the NLS1 Ark 564