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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 8.

Normalized SED shapes of dust-obscured and unobscured AGNs. Panels (a) and (b) show the entire AGN sample and those of AGNs with Lbol in the range of 1045–1046 erg s−1, respectively. Red and blue solid lines represent individual dust-obscured and unobscured AGN SEDs, respectively, normalized at the K-band wavelength. The red and blue dashed lines indicate the median-combined SEDs for the two populations. The orange dotted and magenta dotted–dashed lines represent the median-combined SEDs of moderately obscured (0.1 < E(B − V) < 0.2) and heavily obscured (E(B − V) > 0.2) AGNs, respectively. The red and blue error bars in the top-right corner show the representative 1σ confidence levels of the combined SED shapes for dust-obscured and unobscured AGNs, respectively. The orange and magenta error bars correspond to the same confidence levels for the moderately and heavily obscured AGN subsamples, respectively.

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