High-energy astrophysics
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- GW230814: Investigation of a Loud Gravitational-wave Signal Observed with a Single Detector
- Open Data from LIGO, Virgo, and KAGRA through the First Part of the Fourth Observing Run
- GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- GWTC-4.0: Updating the Gravitational-wave Transient Catalog with Observations from the First Part of the Fourth LIGO–Virgo–KAGRA Observing Run
- Exceptional points and resonance in black hole ringdown
- Improved proper motion and gravity tests with PSR J1913+1102
- Constraints on Late-Time Flaring from Luminous Fast Blue Optical Transients using the Transiting Exoplanet Survey Satellite and the Zwicky Transient Facility
- Eccentricity in Disguise? Insights from GW231123 and Numerically Simulated Binary Black Hole Merger Signals
- Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
- Квантование масс и спинов чёрных дыр: аналитический закон, проверка на 35 событиях LIGO GWTC-3 и вывод из геометрии L8a21
- A 44-min periodic radio transient in a supernova remnant
- The giant pulse population of PSR B0355+54
- Linearized stability of T-duality quantum-inspired thin-shell wormholes
- Magnetic, thermal and rotational evolution of isolated neutron stars
- Aligned Hierarchical Black Hole Mergers in Active-Galactic-Nuclei Disks Revealed by GWTC-4
- Short Gravitational-Wave Transients as Probes of Cosmic Domain Walls
- A micronova burst in the intermediate polar IGR J17014-4306
- Dynamical tidal response of Schwarzschild Black Holes
- SVOM/VT: Instrument Overview, Science Objectives, and First-year Performance
- The Gamma-Ray Monitor Onboard the SVOM Satellite
- ECLAIRs: The SVOM High-energy Transient Trigger Camera
- The SVOM Mission, Its Profile and Its System
- The Radio--X-ray Correlation of High-Redshift AGN: A Numerical Study of Inverse-Compton Scattering of the CMB Photons in Relativistic Jets
- BOOM and Babamul : A Real-time, Multi-survey, Optical Alert Broker System Operating at Scale
- Reconstructing the gravitational waveform from its probe limit