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Atmospheric monitoring and inter-calibration of the telescope optical throughput efficiencies using the trigger rates of the Cherenkov Telescope Array

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00521230" target="_blank" >RIV/68378271:_____/19:00521230 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/19:10405122

  • Result on the web

    <a href="https://doi.org/10.1016/j.astropartphys.2019.02.002" target="_blank" >https://doi.org/10.1016/j.astropartphys.2019.02.002</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.astropartphys.2019.02.002" target="_blank" >10.1016/j.astropartphys.2019.02.002</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Atmospheric monitoring and inter-calibration of the telescope optical throughput efficiencies using the trigger rates of the Cherenkov Telescope Array

  • Original language description

    We discuss a calibration method for imaging atmospheric Cherenkov telescope arrays, based on the detection of cosmic rays. The focus lies on the monitoring of transmission of Cherenkov light in the atmosphere and on the relative calibration of telescope optical throughput efficiencies. We present an approach that addresses both issues by surveying and comparing trigger rates of telescopes in a stereoscopic configuration. A Monte Carlo feasibility study was conducted to explore dependencies of stereo trigger rates on the array layout and observing conditions of the Cherenkov Telescope Array (CTA). Analytical expressions for most of these dependencies have been found and implemented in an extension of the method of the Cherenkov Transparency Coefficient (CTC). In the investigated examples, the resolution of the method for the atmospheric and array calibration has been shown to be 4% and 4–7%, respectively.n

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2019

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astroparticle Physics

  • ISSN

    0927-6505

  • e-ISSN

  • Volume of the periodical

    109

  • Issue of the periodical within the volume

    May

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    13

  • Pages from-to

    12-24

  • UT code for WoS article

    000464087300002

  • EID of the result in the Scopus database

    2-s2.0-85061673904