Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout
The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current ground-based instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy (from
Angüner, E. O. et al.
Fecha de publicación:
9
2019