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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 2.

Best-fit SED results and corresponding photometric data for four randomly selected type 1 AGNs. Blue triangles, green squares, purple triangles, red circles, and yellow stars represent the photometric data from Subaru HSC (N. Oi et al. 2021), FLAMINGOS KPNO (Y. Jeon et al. 2014), AKARI IRC (S. J. Kim et al. 2012), WISE (T. H. Jarrett et al. 2011), and Spitzer IRAC (H. Nayyeri et al. 2018), respectively. The solid black line shows the best-fit SED model, while the dashed red, dotted blue, dotted–dashed green, and dot-dotted–dashed purple lines represent the reddened spectra of AGN, elliptical, spiral, and irregular galaxies, respectively.

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