X-ray Flares in Gamma-Ray Bursts at High and Very-High-Energies

arXiv:2609.00684 · astro-ph.HE · Submitted 2026-09-01 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-01

Updated: 2026-09-01

Terminology

• Test Statistic — 5× in this paper
• Clustering — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Einstein Probe — 1× in this paper
• Gran Sasso Science Institute — 1× in this paper

Sources

• Synchrotron Self-Compton Model of TeV Afterglows in Gamma-Ray Bursts
• Camelidae on BOAT: observation of a second spectral component in GRB 221009A
• Detection of TeV emission during early afterglow from poorly localized GRBs with ground based IACTs
• Predicting Multiwavelength Emission Associated with X-Ray Flares and Extended Emission of Gamma-Ray Bursts
• Time-resolved leptonic modeling of the prompt emission of GRB 211211A
• From X-rays to High-Energy Gamma-rays: A Comprehensive Multi-Wavelength Study of Early Gamma-Ray Burst Afterglows
• Performance of LACT Array: Instrument Response Functions and Source Prospects

Related papers

• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
• Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
• XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
• SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
• Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion