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

Employing the 12 NaI detectors in the Fermi GBM, the Earth OccultationTechnique (EOT) can be used to measure the fluxes of x-ray and gamma-raysources. Each time a source passes behind the Earth (or emerges from behind theEarth), a step-like feature is produced in the detector count rate. With apredefined catalog of source positions, the times of the occultation steps canbe calculated, the individual steps fit, and the fluxes derived. However, inorder to find new sources and generate a complete catalog, a method is neededfor generating an image of the sky. An imaging algorithm has been developed togenerate all-sky images using the GBM data. Here we present imaging resultsfrom ~2.5 years of data in the 12-25 keV and 100-300 keV energy bands.

Searching for Unmodeled Sources Using the Earth Occultation Data from the Fermi GBM