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• W3213728290 abstract "γ-ray is a unique probe for extreme events in the universe. Detecting the γ-ray provides an important opportunity to understand the composition of universe, the evolution of stars, the origin of cosmic rays, etc. γ-ray astronomy involves in various frontier scientific issues, and the observed energy spectrum spans over a wide range from a few hundreds of keV to a few hundreds of TeV. Different γ-ray telescopes are in need for different scientific goals and spectral bands. In this work, 5 kinds of space- and ground-based γ-ray observing techniques were summarized, including the Coded-aperture telescopes, Compton telescopes, Pair-production telescopes, Imaging Atmospheric Cherenkov Telescopes, and Extensive Air Shower Arrays. The progress in γ-ray astronomy in the past 70 years, motivated by the observation capability, was reviewed. Great achievements have been made in the high-energy domain and very-high-energy domain, while because of the limited missions conducted, as well as a lower sensitivity comparing with other domains, discoveries in low- and medium-energy are few, and due to the high observation difficulty, as well as the late start, relevant scientific yields in ultra- and extremely-high energy are limited. Moreover, the future planned missions and capabilities of the γ-ray telescopes and their possible scientific outputs were discussed. Among these missions, low- and medium-energy space telescopes e-ASTROGAM (enhanced-ASTROGAM), AMEGO (All-sky Medium Energy Gamma-ray Observatory), and very-high-energy ground-based arrays LHAASO (Large High Altitude Air Shower Observatory) and CTA (Cherenkov Telescope Array) greatly improve sensitivity than their corresponding last generation, thus expect very likely to further expand our knowledge on the γ-universe." @default.
• W3213728290 created "2021-11-22" @default.
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• W3213728290 date "2021-07-01" @default.
• W3213728290 modified "2023-09-26" @default.
• W3213728290 title "The Review of γ-ray Astronomical Observing Techniques" @default.
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• W3213728290 doi "https://doi.org/10.1016/j.chinastron.2021.08.002" @default.
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