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Creators/Authors contains: "Brown, Anthony M"

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  1. ; ; ; ; ; ; ; ; ; ; et al (, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment)
    The Trinity Demonstrator is a proof of concept prototype for the Trinity Neutrino Observatory, which is sensitive to astrophysical neutrinos above PeV energies. The Demonstrator is a one-square meter class imaging atmospheric Cherenkov telescope deployed on Frisco Peak, Utah, and remotely operated. The light-collection surface is equipped with 77 mirror facets with 15 cm diameter, and its field of view is instrumented with a 256-pixel silicon-photomultiplier camera yielding a angular resolution. The camera signals are digitized with a 100 MS/s, and 12-bit resolution switched capacitor array readout. We discuss the Demonstrator’s design, the telescope’s deployment on Frisco Peak, and its commissioning. 
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    Free, publicly-accessible full text available November 1, 2026
  2. ; ; ; ; ; ; ; ; ; ; et al (, Journal of Astronomical Telescopes, Instruments, and Systems)
    Full Text Available 
  3. ; ; ; ; ; ; ; ; ; ; 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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    Full Text Available