English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Zendy Plus

Presents the zaia usage as premium feature

ZAIA

Presents the pdf analysis as premium feature

PDF Analysis

Insights

Presents the summarisation as premium feature

Summarisation

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the access of premium content as premium feature

Premium Content

Zendy Tools

Zendy Open

Air-shower measurements in the primary energy range beyond 10 TeV can be usedto address important questions of astroparticle and particle physics. The mostprominent among these questions are the search for the origin of chargedGalactic cosmic rays and the so-far little understood transition from Galacticto extra-galactic cosmic rays. A very promising avenue towards answering thesefundamental questions is the construction of an air-shower detector withsufficient sensitivity for gamma-rays to identify the accelerators and largeexposure to achieve accurate spectroscopy of local cosmic rays. With the newground-based large-area (up to 100 square-km) wide-angle (Omega ~ 0.6-0.85 sr)air-shower detector concept HiSCORE (Hundred*i Square-km Cosmic ORiginExplorer), we aim at exploring the cosmic ray and gamma-ray sky(accelerator-sky) in the energy range from few 10s of TeV to 1 EeV using thenon-imaging air-Cherenkov detection technique. The full detector simulation ispresented here. The resulting sensitivity of a HiSCORE-type detector togamma-rays will extend the energy range so far accessed by other experimentsbeyond energies of 50 - 100 TeV, thereby opening up the ultra high energygamma-ray (UHE gamma-rays, E > 10 TeV) observation window.

The HiSCORE concept for gamma-ray and cosmic-ray astrophysics beyond 10\,TeV