Tracing Obscured AGN Contribution and Number Fraction Across 0 < z < 6 with JWST
Angel Rodriguez Barbosa, Tomotsugu Goto, Daryl Joe D. Santos, Chih-Teng Ling, Tetsuya Hashimoto, Ece Kilerci, Priyanka Jalan, Terry Long Phan, Deriyan Senjaya, Vignesh V. V. Rao, Bahareh S. Salmasi
Institute of Astronomy, National Tsing Hua University · Department of Physics, National Tsing Hua University · Department of Physics, De La Salle University · Department of Astronomical Science SOKENDAI · Department of Physics, National Chung Hsing University · Department of Astronomy and Space Sciences, Istanbul University · Institute of Astronomy, National Tsing Hua University · Institute of Astronomy, National Tsing Hua University · Department of Physics, National Tsing Hua University · Department of Physics, National Chung Hsing University · Institute of Astronomy, National Tsing Hua University
astro-ph.GA
Submitted: 2026-07-28
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- MEOW: The increase in the obscured AGN fraction in mid-infrared from 0 < z < 6 with JWST MIRI
- JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields
- Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
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