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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Blazars are a highly-variable, radio-loud subclass of active galactic nuclei(AGN). In order to better understand such objects we must be able to easilyidentify candidate blazars from the growing population of unidentified sources.Working towards this goal we attempt to identify new gamma-ray blazarcandidates from a sample of 102 previously unidentified sources. These sourcesare selected from Astronomer's Telegrams and the literature on the basis ofnon-periodic variability and multi-wavelength behavior. We then attempt toassociate these objects to an IR counterpart in the WISE all-sky survey. We areable to identify sixteen candidate sources whose IR colors are consistent withthose of the blazar population. Of those sixteen, thirteen sources have IRcolors indicative of being gamma-ray emitting blazar candidates. These sourcesall possess archival multi-wavelength observations that support theirblazar-like nature.

Identification of New Gamma-Ray Blazar Candidates With Multifrequency Archival Observations