Nowhere to hide: Radio-faint AGN in the GOODS-N field
نویسندگان
چکیده
Obtaining a census of active galactic nuclei (AGN) activity across cosmic time is critical to our understanding galaxy evolution and formation. Many AGN classification techniques are compromised by dust obscuration. However, very long baseline interferometry (VLBI) can be used identify compact emission that only attributed activity. This the second in series papers dealing with radio population GOODS-N field. We review 14 different context VLBI-detected sample, use these investigate nature as well their host galaxies. find no single identification technique all VLBI objects AGN. Infrared colour-colour selection most notably incomplete. usage multiple schemes VLBI-selected AGN, independently verifying similar approaches other deep field surveys. In era large area surveys instruments such SKA ngVLA, multi-wavelength coverage, which relies heavily upon observations from space, often unavailable. Therefore, remains an integral component detecting jetted efficient inefficient accretion types. A substantial fraction (46%) have X-ray counterpart, likely due lack sensitivity band. high reside low or intermediate redshift dust-poor early-type These exhibit accretion. Finally, significant symbiotic dusty starburst - systems. present extensive compilation properties Appendix.
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ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2021
ISSN: ['0004-6361', '1432-0746']
DOI: https://doi.org/10.1051/0004-6361/202038591