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 Tools annual

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 Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

The multi-wavelength pulsed emission from young pulsars and millisecondpulsars can be well modeled with the single-pole 3-dimension annular gap andcore gap model. To distinguish our single magnetic pole model from two-polemodels (e.g. outer gap model and two-pole caustic model), the convincing valuesof the magnetic inclination angle and the viewing angle will play a key role.

Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars