CTA is the next-generation ground-based gamma-ray observatory under construction to detect energies from 20 GeV to over 300 TeV with high precision using more than 100 telescopes at two hemispheric sites.
et al., Observation of TeV Gamma Rays from the Crab Nebula Using the Atmospheric Cerenkov Imaging Technique, ApJ 342 379ff (1989)
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The Cherenkov Telescope Array
CTA is the next-generation ground-based gamma-ray observatory under construction to detect energies from 20 GeV to over 300 TeV with high precision using more than 100 telescopes at two hemispheric sites.