Highlights from the Telescope Array Experiment

Collaboration
Sep 25, 2023
18 pages
Published in:
  • PoS ICRC2023 (2024) 008
Contribution to:
  • Published: Sep 25, 2023
Experiments:

Citations per year

20222023202403
Abstract: (SISSA)
The Telescope Array (TA) is the largest ultra-high energy cosmic ray (UHECR) observatory in the Northern Hemisphere. Together with the TA Low Energy Extension (TALE), TA×\times4, and TALE infill detector, the TA measures the properties of UHECR-induced extensive air showers (EAS) in the energy region from 1015^{15} eV to over 1020^{20} eV. Each of these uses a hybrid system with an array of scintillators to sample the footprint of the EAS at the Earth's surface along with telescopes that measure the fluorescence and Cherenkov light from the EAS. The statistics at the highest energies are being enhanced with the TA×\times4 detector, half completed but still under construction, which will quadruple the surface detector area with telescopes. The TALE infill surface detectors were recently deployed to further lower the hybrid energy threshold of TALE. We present the status of the experiment and recent results on the energy spectrum, mass composition, and anisotropy, including new features in the energy spectrum at about 1019.2^{19.2} eV and in the UHECR arrival direction anisotropy.
  • showers: atmosphere
  • cosmic radiation: UHE
  • detector: surface
  • energy: threshold
  • radiation: Cherenkov
  • energy: low
  • hybrid
  • energy spectrum
  • anisotropy
  • statistics