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 origin of the high-energy emission of blazars is still a matter ofdebate. To investigate the emission mechanism of extragalactic outflows and topin down the location of the emission, we have constructed a broadband spectralenergy distribution (SED) database covering from the radio to the gamma-rayband for the complete MOJAVE sample, which consists of 135 relativisticallybeamed AGN with well-studied parsec-scale jets. Typically, the broadband SEDsof blazars shows a double-humped profile. It is believed that the lower-energyhump is due to synchrotron emission from the radio jet, and the higher-energyhump is generated by i) inverse-Compton upscattered seed photons (leptonic),ii) proton-induced shower (hadronic). Combining the results of high-resolutionVLBI observations and the gamma-ray properties of the MOJAVE sources, weattempt to reveal the origin of the high-energy emission in relativistic jets,and search for correlations between VLBI and high-energy properties.

The broadband emission properties of AGN jets