A compact and light-weight refractive telescope for the observation of extensive air showers
arXiv:1804.01781 · doi:10.1088/1748-0221/13/07/P07024
Abstract
A general purpose instrument for imaging of Cherenkov light or fluorescence light emitted by extensive air showers is presented. Its refractive optics allows for a compact and light-weight design with a wide field-of-view of 12°. The optical system features a 0.5 m diameter Fresnel lens and a camera with 61 pixels composed of Winston cones and large-sized 6x6 mm photo sensors. As photo sensors, semi conductor light sensors (SiPMs) are utilized. The camera provides a high photon detection efficiency together with robust operation. The enclosed optics permit operation in regions of harsh environmental conditions. The low price of the telescope allows the production of a large number of telescopes and the application of the instrument in various projects, such as FAMOUS for the Pierre Auger Observatory, HAWC's Eye for HAWC or IceAct for IceCube. In this paper the novel design of this telescope and first measurements are presented.
arXiv commentSubmitted to JINST, second (minor) revision
References in corpus (20)
- Design Concepts for the Cherenkov Telescope Array
- The Pierre Auger Cosmic Ray Observatory
- Observations of the Crab Nebula with H.E.S.S
- The IceCube Neutrino Observatory: Instrumentation and Online Systems
- The surface detector array of the Telescope Array experiment
- The Fluorescence Detector of the Pierre Auger Observatory
- VERITAS: the Very Energetic Radiation Imaging Telescope Array System
- Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory
- VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope
- Design and Operation of FACT -- The First G-APD Cherenkov Telescope
- Monocular Measurement of the Spectrum of UHE Cosmic Rays by the FADC Detector of the HiRes Experiment
- Extensive Air Showers and Ultra High-Energy Cosmic Rays: A Historical Review
- Calibration and performance of the photon sensor response of FACT -- The First G-APD Cherenkov telescope
- Very-high energy gamma-ray astronomy: A 23-year success story in high-energy astroparticle physics
- TARGET: A Digitizing And Trigger ASIC For The Cherenkov Telescope Array
- FACT - Long-term stability and observations during strong Moon light
- Design constraints on Cherenkov telescopes with Davies-Cotton reflectors
- Photosensor Characterization for the Cherenkov Telescope Array: Silicon Photomultiplier versus Multi-Anode Photomultiplier Tube
- Status of the Silicon Photomultiplier Telescope FAMOUS for the Fluorescence Detection of UHECRs
- Design study of an air-Cherenkov telescope for harsh environments with efficient air-shower detection at 100 TeV
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- An integrated general purpose SiPM based optical module with a high dynamic range
- Atmospheric Cherenkov Telescopes as a Potential Veto Array for Neutrino Astronomy
- Design and Performance of the first IceAct Demonstrator at the South Pole
- Calibration of 122 SensL MicroFJ-60035 SiPMs and the reduction of optical crosstalk due to coupled light guides
- Three-year performance of the IceAct telescopes at the IceCube Neutrino Observatory