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    <identifier>10.57760/sciencedb.j00186.01046</identifier>
    <datestamp>2026-05-18T19:11:30Z</datestamp>
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  <dc:date>2026-05-18</dc:date>
  <dc:title>HADAR&amp;rsquo;s observational prospects for cosmic-ray anisotropy dataset</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.j00186.01046</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>This dataset was generated using Monte Carlo simulation methods to evaluate the observational performance of HADAR&amp;mdash;a new type of wide-angle Cherenkov detector&amp;mdash;regarding large-scale cosmic-ray anisotropy in the energy range from 100 GeV to several hundred TeV. The data generation process strictly simulates the detector&amp;rsquo;s response functions, including the zenith-angle-dependent effective area and the discrimination capability between protons and photons across different energies. During the simulation, source positions are updated at 1-second intervals to precisely account for the effects of Earth's rotation on right ascension observations, ensuring statistical rigor in the spatial distribution at the detector's zenith.</dc:description>
  <dc:subject>HADAR; cosmic-ray; Monte Carlo; anisotropy</dc:subject>
  <dc:creator>Zhang Zi Hao</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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