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/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The Tibet air shower array, which has an effective area of 37,000 squaremeters and is located at 4300 m in altitude, has been observing air showersinduced by cosmic rays with energies above a few TeV. We are planning to add alarge muon detector array to it for the purpose of increasing its sensitivityto cosmic gamma rays in the 100 TeV (10 - 1000 TeV) energy region bydiscriminating them from cosmic-ray hadrons. We report on the possibility ofdetection of gamma rays in the 100 TeV energy region in our field of view,based on the improved sensitivity of our air shower array deduced from the fullMonte Carlo simulation.

Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : physics goal and overview