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  1. ; ; ; ; ; ; ; ; ; ; et al ( , 37th International Cosmic Ray Conference (ICRC2021))
    We present a catalog of results of gamma-ray observations made by VERITAS, published from 2008 to 2020. VERITAS is a ground based imaging atmospheric Cherenkov telescope observatory located at the Fred Lawrence Whipple Observatory (FLWO) in southern Arizona, sensitive to gamma-ray photons with energies in the range of ∼ 100 GeV - 30 TeV. Its observation targets include galactic sources such as binary star systems, pulsar wind nebulae, and supernova remnants, extragalactic sources like active galactic nuclei, star forming galaxies, and gamma-ray bursts, and some unidentified objects. The catalog includes in digital form all of the high-level science results published in 112 papers using VERITAS data and currently contains data on 57 sources. The catalog has been made accessible via GitHub and at NASA's HEASARC.
    Free, publicly-accessible full text available March 18, 2023
  2. ; ; ; ; ; ; ; ; ; ; et al ( , Proc. of 37th International Cosmic Ray Conference - PoS(ICRC2021))
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  3. ; ; ; ; ; ; ; ; ; ; et al ( , Journal of Astronomical Telescopes, Instruments, and Systems)
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  4. ; ; ; ; ; ; ; ; ; ; et al ( , Proceedings Volume 11820, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III;)
    Hallibert, Pascal ; Hull, Tony B. ; Kim, Daewook ; Keller, Fanny (Ed.)
    The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA's medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dual-mirror optics. The SCT project has built and is currently operating a 9.7-m prototype SCT (pSCT) at the Fred Lawrence Whipple Observatory (FLWO); such optical design enables the use of a compact camera with state-of-the art silicon photomultiplier detectors. A partially-equipped camera has recently successfully detected the Crab Nebula with a statistical significance of 8.6 standard deviations. A funded upgrade of the pSCT focal plane sensors and electronics is currently ongoing, which will bring the total number of channels from 1600 to 11328 and the telescope field of view from about 2.7° to 8° . In this work, we will describe the technical and scientific performance of the pSCT.
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