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Performance of the Cherenkov Telescope Array
G. Maier, L. Arrabito, K. Bernlöhr +5
The Cherenkov Telescope Array (CTA) is expected to become the by far largest and most sensitive observatory for very-high-energy gamma rays in the energy range from 20 GeV to more…
Background for a gamma-ray satellite on a low-Earth orbit
P. Cumani, M. Hernanz, J. Kiener +2
The different background components in a low-Earth orbit have been modeled in the 10 keV to 100 GeV energy range. The model is based on data from previous instruments and it consid…
Limits on the flux of tau neutrinos from 1 PeV to 3 EeV with the MAGIC telescopes
MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +142
A search for tau neutrino induced showers with the MAGIC telescopes is presented. The MAGIC telescopes located at an altitude of 2200 m a.s.l. in the Canary Island of La Palma, can…
Nature of the low-energy, γ-like background for the Cherenkov Telescope Array
Julian Sitarek, Dorota Sobczyńska, Michał Szanecki +3
The upcoming Cherenkov Telescope Array (CTA) project is expected to provide unprecedented sensitivity in the low-energy (<~100 GeV) range for Cherenkov telescopes. Most of the rema…
Performance of the Cherenkov Telescope Array
G. Maier, L. Arrabito, K. Bernlöhr +4
The Cherenkov Telescope Array (CTA) will be the world's largest and by far most sensitive observatory for high-energy gamma rays. It will be capable of detecting gamma rays from ex…
Performance of the MAGIC telescopes under moonlight
D. Guberman, P. Colin
MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…
Baseline telescope layouts of the Cherenkov Telescope Array
P. Cumani, T. Hassan, L. Arrabito +4
The Cherenkov Telescope Array (CTA) will be the next generation of ground-based instrument for Very High Energy gamma-ray astronomy. It will improve the sensitivity of current tele…
Monte Carlo Performance Studies for the Site Selection of the Cherenkov Telescope Array
T. Hassan, L. Arrabito, K. Bernlöhr +13
The Cherenkov Telescope Array (CTA) represents the next generation of ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed at improving on the sensitivity…
Performance of the MAGIC telescopes under moonlight
MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +143
MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…
GAMMA-400 gamma-ray observatory
N. P. Topchiev, A. M. Galper, V. Bonvicini +71
The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electron…
A separation of electrons and protons in the GAMMA-400 gamma-ray telescope
A. A. Leonov, A. M. Galper, V. Bonvicini +63
The GAMMA-400 gamma-ray telescope is intended to measure the fluxes of gamma rays and cosmic-ray electrons and positrons in the energy range from 100 MeV to several TeV. Such measu…
Study of the Gamma-ray performance of the GAMMA-400 Calorimeter
P. Cumani, A. M. Galper, V. Bonvicini +73
GAMMA-400 is a new space mission, designed as a dual experiment, capable to study both high energy gamma rays (from 100 MeV to few TeV) and cosmic rays (electrons up to 20 Te…
The GAMMA-400 Space Mission
P. Cumani, A. M. Galper, V. Bonvicini +64
GAMMA-400 is a new space mission which will be installed on board the Russian space platform Navigator. It is scheduled to be launched at the beginning of the next decade. GAMMA-40…
The GAMMA-400 gamma-ray telescope characteristics. Angular resolution and electrons/protons separation
A. A. Leonov, A. M. Galper, V. Bonvicini +64
The measurements of gamma-ray fluxes and cosmic-ray electrons and positrons in the energy range from 100 MeV to several TeV, which will be implemented by the specially designed GAM…