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

Motivated by the discovery of high-energy astrophysical neutrinos with IceCube, we study the prospects for improved measurements of neutrinos of astrophysical origin with a surface array combined with IceCube or a next generation neutrino detector at the South Pole. Backgrounds in astrophysical neutrino searches are reduced by tagging muons and neutrinos of atmospheric origin by detecting the accompanying air shower. We consider various air shower array configurations, including different array layouts and detector station sizes, and study their air shower detection efficiency. We will report on the various approaches we have used to understand the capabilities of such arrays.

Simulation Studies for a Surface Veto Array to Identify Astrophysical Neutrinos at the South Pole