Figure 11 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 11.

Upper panel: absorption bias in the 8–24 keV band, assuming a BNTORUS model with ﹩{\rm{\Gamma }}=1.8﹩ for different redshifts as indicated. Black and light gray respectively indicate ﹩{\theta }_{\mathrm{oa}}=60﹩° and 30° (BNTORUS30 case). Lower panel: ratio between the 8–24 keV absorption bias between 60° and 30°.

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