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 Geminga gamma ray source was first detected by the SAS-2 gamma-raysatellite observatory and the COS-B x-ray satellite observatory, and has beenidentified as a radio-quiet pulsar associated with a 300,000 year old supernovaremnant. Geminga is one of the brightest GeV sources as seen by the Large AreaTelescope on board the Fermi gamma-ray satellite observatory. A ground baseddetection was accomplished by the Milagro extensive air shower array atenergies greater than 20 TeV. During 2007 VERITAS performed observations tosearch for TeV gamma ray emission from the Geminga pulsar and the region nearGeminga. In this paper, we describe these measurements and the new analysis ofthese observations.

Search for TeV Emission from Geminga by VERITAS