Enhancing the Angular Resolution of Large Array of imaging atmospheric Cherenkov Telescope (LACT) at Ultra-High Energies
astro-ph.HE, astro-ph.IM
Submitted: 2026-05-31
Updated: 2026-09-24
Terminology
Sources
- Layout optimization and Performance of Large Array of imaging atmospheric Cherenkov Telescope (LACT)
- Improving the H.E.S.S. angular resolution using the Disp method
- Performance of LACT Array: Instrument Response Functions and Source Prospects
- Analysis optimisation for more than 10 TeV gamma-ray astronomy with IACTs
- The Disp Method for Analysing Large Zenith Angle Gamma-Ray Data
- CTLearn: Deep Learning for Gamma-ray Astronomy
- Performance of a proposed event-type based analysis for the Cherenkov Telescope Array
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