Figure 6 from The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample

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The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample

Authors: L. Zappacosta, A. Comastri, F. Civano, S. Puccetti, F. Fiore, J. Aird, A. Del Moro, G. B. Lansbury, G. Lanzuisi, A. Goulding, J. R. Mullaney, D. Stern, M. Ajello, D. M. Alexander, D. R. Ballantyne, F. E. Bauer, W. N. Brandt, C.-T. J. Chen, D. Farrah, F. A. Harrison, P. Gandhi, L. Lanz, A. Masini, S. Marchesi, C. Ricci, and E. Treister

2018 The Astrophysical Journal 854 33.

Provider: AAS Journals

Caption: Figure 6.

Upper panel: intrinsic 10–40 keV luminosity measured on the coronal primary component only (i.e., unabsorbed luminosity computed after removing the Compton-reflection term) vs. unabsorbed 10–40 keV luminosity measured on the unabsorbed baseline best-fit model (i.e., including the Compton-reflection term). Uncertainties in the baseline spectral modeling are reported in light colors. The dotted line shows a relation with slope 1. Lower panel: ratio between unabsorbed and intrinsic luminosities. Red diamonds show the sources exhibiting ﹩R\gt 1﹩.

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