Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques
The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy g...
The Cherenkov detectors used in astroparticle physics are found in the most varied of environments. ...
The Gamma Cherenkov Telescope (GCT) is one of the designs proposed for the Small Sized Telescope (SS...
Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray as...
The technique of gamma-ray astronomy at very high energies (VHE: > 100 GeV) with ground-based imagin...
The interaction of very-high-energy astrophysical gamma rays with the Earth’s atmosphere produces ex...
A new method of shower-image analysis is presented which appears very powerful as applied to those C...
The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrum from 100 GeV to 50 ...
Considerable progress has been made in the last half-decade in the field of very high energy (VHE) g...
The Whipple Observatory 10 m gamma-ray telescope has been used to search for TeV gamma-ray emission ...
Turver and Weekes proposed using a system of phototubes in the focal plane of a large reflector to g...
This project is to search for Very High Energy (VHE) (10¹¹ eV to 10¹⁴ eV) gamma rays from the Crab n...
All along the 20th century, astronomy has been extended to the whole electromagnetic wavelengths, al...
The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy g...
The high energy end of gamma-ray source spectra might provide important clues regarding the nature o...
The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy g...
The Cherenkov detectors used in astroparticle physics are found in the most varied of environments. ...
The Gamma Cherenkov Telescope (GCT) is one of the designs proposed for the Small Sized Telescope (SS...
Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray as...
The technique of gamma-ray astronomy at very high energies (VHE: > 100 GeV) with ground-based imagin...
The interaction of very-high-energy astrophysical gamma rays with the Earth’s atmosphere produces ex...
A new method of shower-image analysis is presented which appears very powerful as applied to those C...
The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrum from 100 GeV to 50 ...
Considerable progress has been made in the last half-decade in the field of very high energy (VHE) g...
The Whipple Observatory 10 m gamma-ray telescope has been used to search for TeV gamma-ray emission ...
Turver and Weekes proposed using a system of phototubes in the focal plane of a large reflector to g...
This project is to search for Very High Energy (VHE) (10¹¹ eV to 10¹⁴ eV) gamma rays from the Crab n...
All along the 20th century, astronomy has been extended to the whole electromagnetic wavelengths, al...
The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy g...
The high energy end of gamma-ray source spectra might provide important clues regarding the nature o...
The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy g...
The Cherenkov detectors used in astroparticle physics are found in the most varied of environments. ...
The Gamma Cherenkov Telescope (GCT) is one of the designs proposed for the Small Sized Telescope (SS...