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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 3.

Examples of spectral fitting results for the C IV, Mg II, Hβ, and Hα line complexes. In the upper panels, the black lines show the rest-frame continuum-subtracted spectra. The dashed blue and dotted green lines represent the broad and narrow emission-line models, respectively, and the solid red lines indicate the combined best-fit model of the broad and narrow lines. The lower panels show the fitting residuals.

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