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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 7.

Dust-obscured AGN fraction as a function of redshift in four bolometric luminosity subsamples. The filled blue, red, green, and purple circles and lines denote the fractions for L_bol ranges of 10^44.5–10^45.0, 10^45.0–10^45.5, 10^45.5–10^46.0, and 10^45.5–10^46.0, respectively. Only cases where the number of AGNs is at least ten are shown to avoid the effects of small number statistics.

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