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Bibliographical reference
Astroparticle Physics, Volume 111, p. 35-53.
Advertised on:
9
2019
Journal
Citations
55
Refereed citations
29
Description
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 20 GeV to 300 TeV). This achievement will be possible by using
tens of imaging Cherenkov telescopes of three successive sizes. They
will be arranged into two arrays, one per hemisphere, located on the La
Palma island (Spain) and in Paranal (Chile). We present here the
optimised and final telescope arrays for both CTA sites, as well as
their foreseen performance, resulting from the analysis of three
different large-scale Monte Carlo productions.
Related projects
Particle Astrophysics
The MAGIC Collaboration is integrated by 20 research institutes and university departments from Armenia, Bulgaria, Finland, Germany, Italy, Poland, Spain, Switzerland and USA. The collaboration comprises two 17m diameter telescopes, located at the Roque de los Muchachos Observatory, designed to measure the Cherenkov radiation associated with
Ramón
García López