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XMM and NuSTAR Observations of an Optically Quiescent Quasar

  • Authors: Claire Greenwell, Poshak Gandhi, George Lansbury, Peter Boorman, Vincenzo Mainieri, Daniel Stern

Claire Greenwell et al 2022 The Astrophysical Journal Letters 934 .

  • Provider: AAS Journals

Caption: Figure 3.

Corner plot of results with (a) CABSZWABSPOW, restrictive prior on Γ (blue); (b) BNSPHERE, physically representative prior on Γ (orange), and (c) CABSZWABSPOW, fixed Γ = 1.9 (green). Best-fit values for each parameter are shown with a solid line. (Top right) L 2–10 vs. Γ contour with the IR-predicted luminosity shown (Stern 2015, dashed line)—the luminosity contours for the lightly obscured models are decisively below this level. Also shown are the results for the 12% scattered “leaky sphere”, which is closer to predicted (pink).

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