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A Deep Spectroscopic Study of a JWST-discovered, Faint, Broad-line AGN at z ∼ 5

Authors: Elaina Malczewski, Feige Wang, Jinyi Yang, Aaron J. Barth, Jaclyn B. Champagne, Xiaohui Fan, Anniek J. Gloudemans, Xiangyu Jin, Jiang-Tao Li, Alessandro Lupi, Chiara Mazzucchelli

Elaina Malczewski et al 2026 Research Notes of the AAS 10 .

Provider: AAS Journals

Caption: Figure 1.

Panel (A): 2D PRISM spectrum. Panel (B): 1D PRISM spectrum (truncated) with emission lines, power-law continuum, and Lyα and Hβ fitting. Panel (C): 1D G395M spectrum showing Hβ, [O III], and Hα. Panel (D): Left: G395M spectrum showing Hβ and [O III] Gaussian fits. Right: G395M spectrum showing Hα fit components. Panel (E): HST/WFC3 (F125W/F160W, GO 16187) and JWST/NIRCam (F115W/F200W/F365W, GO 2028) imaging. Panel (F): PRISM spectrum showing F_ν with LRD (orange) and quasar (green) template SEDs.

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