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

There exist strong evidence supporting the co-evolution of centralsupermassive black holes and their host galaxies. It is however still unclearwhat the exact role of nuclear activity, in the form of accretion onto thesesupermassive black holes, in this co-evolution is. We use a richmulti-wavelength dataset available for the North Ecliptic Pole field, mostnotably surveyed by the AKARI satellite infrared telescope to study the hostgalaxy properties of AGN. In particular we are interested in investigatingstar-formation in the host galaxies of radio-AGN and the putative radiofeedback mechanism, potentially responsible for the eventual quenching ofstar-formation. Using both broadband SED modeling and optical spectroscopy, wesimultaneously study the nu- clear and host galaxy components of our sources,as a function of their radio luminosity, bolo- metric luminosity, andradio-loudness. Here we present preliminary results concerning the AGN contentof the radio sources in this field, while offering tentative evidence that jetsare inefficient star-formation quenchers, except in their most powerful state.

Star-formation in the host galaxies of radio-AGN