The Fraction of Radio-Loud AGN in the Euclid Deep Field North
Abstract
Understanding how active galactic nuclei (AGN) evolve with cosmic time and interact with their host galaxies is central to constraining the role of AGN feedback in galaxy evolution. The availability of deep, wide-field surveys now allow for statistical studies of the relationship between radio AGN activity and host galaxy properties across the full AGN population. We examine the radio-loud AGN fraction as a function of redshift and stellar mass by combining LOFAR radio data with Euclid optical/NIR imaging.
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Astrophysical Phenomena and Observations
Astrophysics and Cosmic Phenomena
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 27 February 2026
- Language
- EN