Revealing the burning and soft heart of the bright bare active galactic nucleus ESO 141-G55: X-ray broadband and SED analysis

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Fig. 2.

Data-to-model ratio of the simultaneous 2022 XMM-Newton-pn (black) and NuSTAR (blue) spectrum of ESO 141-G55 fit with a Galactic (N_H(Gal) = 5.7 × 10²⁰ cm⁻²) absorbed power-law continuum model over the 3–5 keV energy range. Top panel: Extrapolation over the 0.3–79 keV broadband X-ray energy range. Bottom panel: Zoom-in on the Fe Kα line. The vertical dashed green line corresponds to 6.4 keV.

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