Radio-AGN in the AKARI-NEP field and their role in the evolution of galaxies
Marios Karouzos, Myungshin Im, and the AKARI-NEP team
TL;DR
This study investigates radio-loud AGN in the AKARI NEP field, revealing their association with massive, early-type galaxies and exploring their role in galaxy evolution through optical spectroscopy.
Contribution
It provides new insights into the properties of radio-loud AGN and their connection to galaxy evolution using combined photometric and spectroscopic data.
Findings
Radio-AGN are linked to early-type, massive galaxies.
Radio-AGN host galaxies have relatively old stellar populations.
Preliminary results suggest a role of radio-AGN in galaxy evolution.
Abstract
Radio-loud active galaxies have been found to exhibit a close connection to galactic mergers and host galaxy star-formation quenching. We present preliminary results of an optical spectroscopic investigation of the AKARI NEP field. We focus on the population of radio-loud AGN and use photometric and spectroscopic information to study both their star-formation and nuclear activity components. Preliminary results show that radio-AGN are associated with early type, massive galaxies with relatively old stellar populations.
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