ASTRI is a Flagship Project financed by the Italian Ministry of Education, University and Research, and led by the Italian National Institute of Astrophysics, INAF. The Cherenkov Telescope Array (CTA) will be a next-generation ground-based observatory for very high energy gamma-ray astronomy. It will consist of two arrays of dishes, a southern-hemisphere array at ESO’s Paranal Observatory and a northern array on the island of La Palma, Spain. The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The Cherenkov Telescope Array (CTA) is the observatory for ground-based gamma-ray astron-omy that will shape the domain of TeV astronomy for the next decades. CTA will comprise more than 100 imaging air Cherenkov telescopes deployed on two sites, one in the northern hemisphere on La Palma and one in the southern hemisphere in Chile. On Wednesday, 10 October 2018, more than 200 guests from around the world gathered on the northern array site of the Cherenkov Telescope Array (CTA) to … A breakthrough in very high energy Astrophysics Very high energy gamma-rays differs fundamentally from that detected by astronomical instruments at lower energies: GeV to TeV gamma-rays cannot conceivably be generated thermally by emission from hot celestial objects. The experiment is designed to observe air showers induced by cosmic rays with extremely high energy. HAWC is located on the flanks of the Sierra Negra volcano near Puebla, Mexico at an altitude of 4100 meters (13,500 feet). Cherenkov Telescope Array (CTA) is an international project with a goal to construct ground-based astronomical observatories, designed to detect high-energy gamma rays using atmospheric blue-flash (Cherenkov light) imaging techniques. The detector has an instantaneous field of view covering 15% of the sky, and during each 24 hour period HAWC observes two-thirds of the sky. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. CTA will begin operation in ~2020 and will be the world’s largest and most sensitive gamma-ray observatory. The Cherenkov Telescope Array (CTA) is a ~ 200M€ international project, involving ~1000 scientists and engineers from 27 countries. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The Cherenkov Telescope Array is conceived to help fill this gap in our knowledge.

Two observatories are planned, one in … It does this using a combination of ground array and air-fluorescence techniques.

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