Properties of AGN coronae in the NuSTAR era

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A physical model of the broad-band continuum of AGN and its implications for the UV/X relation and optical variability (2018, background): “There is also an additional X-ray component which dominates over the soft X-ray excess beyond 1–2 keV, extending up to kTe ∼ 40–100 keV, with τ ∼ 1–2 (Fabian et al. 2015; Lubiński et al. 2016; Petrucci et al. 2017).”
X-Ray Emissions from Accreting White Dwarfs: A Review (2017, background): “However, recent observations appear to favor compact “corona” of very limited spatial extent (Fabian et al. 2015), unlike that envisioned for SS Cyg by (Ishida et al. 2009).”
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog (2017, background): “For two of the objects reported by Marinucci et al. (2016), 3C 382 (Ballantyne et al. 2014) and Fairall 9 (Fabian et al. 2015), the data did not allow to constrain the energy of the cutoff.”