Abstract In this article we discuss the possibility of using the observations by GLAST of standard gamma sources, as the Crab Nebula, to calibrate imaging air Cherenkov detectors, MAGIC in particular, and optimise their energy resolution. We show that at around 100 GeV the absolute energy calibration uncertainty of Cherenkov telescopes can be reduced to ≲10% by means of such cross-calibration procedure
The continuum high-energy gamma-ray emission between 1 GeV and 105 GeV from the Crab Nebul...
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La...
The interaction of very-high-energy astrophysical gamma rays with the Earthâs atmosphere produces ex...
n this article we discuss the possibility of using the observations by GLAST of standard gamma sourc...
A project to construct a 17 m diameter imaging air Cherenkov telescope, called the MAGIC Telescope, ...
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes located on the Canary island ...
The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, which will co...
Imaging atmospheric Cherenkov telescopes (IACT) observe the sky in the highest energy ranges. From ...
During its first cycle, the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescope was perf...
The ``Gamma Ray Astronomy at ALmeria'' (GRAAL) experiment uses 63 heliostat-mirrors with a total mir...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
The MAGIC telescopes exploit the cosmic gamma rays impacting our atmosphere to monitor the night sky...
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La...
Aims. We measure the Crab Nebula γ-ray spectral energy distribution in the ~100 TeV energy domain an...
The detection of the Crab Nebula via the Cherenkov imaging technique places TeV astronomy on a secur...
The continuum high-energy gamma-ray emission between 1 GeV and 105 GeV from the Crab Nebul...
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La...
The interaction of very-high-energy astrophysical gamma rays with the Earthâs atmosphere produces ex...
n this article we discuss the possibility of using the observations by GLAST of standard gamma sourc...
A project to construct a 17 m diameter imaging air Cherenkov telescope, called the MAGIC Telescope, ...
The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes located on the Canary island ...
The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, which will co...
Imaging atmospheric Cherenkov telescopes (IACT) observe the sky in the highest energy ranges. From ...
During its first cycle, the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescope was perf...
The ``Gamma Ray Astronomy at ALmeria'' (GRAAL) experiment uses 63 heliostat-mirrors with a total mir...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
The MAGIC telescopes exploit the cosmic gamma rays impacting our atmosphere to monitor the night sky...
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La...
Aims. We measure the Crab Nebula γ-ray spectral energy distribution in the ~100 TeV energy domain an...
The detection of the Crab Nebula via the Cherenkov imaging technique places TeV astronomy on a secur...
The continuum high-energy gamma-ray emission between 1 GeV and 105 GeV from the Crab Nebul...
MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La...
The interaction of very-high-energy astrophysical gamma rays with the Earthâs atmosphere produces ex...