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The Cherenkov Telescope Array

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arxiv 2305.12888 v1 pith:PMLNMH4M submitted 2023-05-22 astro-ph.IM astro-ph.HE

Werner Hofmann , Roberta Zanin This is my paper · ORCID
classification astro-ph.IMastro-ph.HE
keywords telescopearraycherenkovctaoenergywillcoveragegamma
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The Cherenkov Telescope Array Observatory (CTAO) is a next-generation facility for ground-based very high energy gamma ray astronomy. CTAO will be operated as an open observatory. With two sites, in the northern and southern hemispheres, the Cherenkov Telescope Array CTA will provide full-sky coverage, improving sensitivity by an order of magnitude over current instruments, with a wide gamma ray energy coverage from 20 GeV to 300 TeV. CTA will use telescope arrays composed of three types of telescopes, optimized to cover different energy ranges. The large telescopes covering the lowest energies provide rapid slewing capability, for follow-up of transients. Key Science Projects (KSPs) are developed to form a significant part of the CTAO observing program during the first decade of operation, providing legacy data sets such as surveys or deep observations of key targets.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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  3. Hunting Star-Forming Galaxies in the Gamma-Ray Domain

    astro-ph.HE 2025-04 conditional novelty 5.0 of 10

    A revised GeV Lgamma-SFR correlation and SFR-scaled spectra suggest about a dozen star-forming galaxies, including M83, M33, NGC 1068, NGC 4945, and Circinus, may be detectable by CTAO, LHAASO, or SWGO.

  4. Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies

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