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Black Hole Properties of Type 1 Active Galactic Nuclei in the North Ecliptic Pole Wide Field. I. Mid-infrared Sources with Optical Counterparts

  • Authors: Dohyeong Kim, Myungshin Im, Hyunjin Shim, Minjin Kim, Gu Lim, Junyeong Park, Hayeong Jeong, Yongjung Kim, Yongmin Yoon, Seong Jin Kim, Yoshiki Toba, Tomotsugu Goto, Nagisa Oi, Hyunmi Song

Dohyeong Kim et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 10.

﹩\mathrm{log}\left({\lambda }_{{\rm{Edd}}}\right)﹩ values vs. redshifts. Filled blue triangles, yellow squares, and magenta circles correspond to unobscured (E(B − V) ≤ 0.1), moderately obscured (0.1 < E(B − V) ≤ 0.2), and heavily obscured (E(B − V) > 0.2) AGNs, respectively. (a) Colored polygons indicate the median ﹩\mathrm{log}\left({\lambda }_{{\rm{Edd}}}\right)﹩ and 1σ dispersions in eight redshift bins. (b) Median ﹩\mathrm{log}\left({\lambda }_{{\rm{Edd}}}\right)﹩ values in the same eight redshift bins are shown with 1σ dispersions.

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