Figure 17 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 17.

Broadband spectra and relative best-fit model for sources egs26, ser37, and ser148. The adopted best-fit model is the baseline one modified with the addition of a low-energy, ionized/neutral, partial-covering absorber. Black, red, green, and blue spectra refer to Chandra, XMM-Newton, NuSTAR-FPMA, and NuSTAR-FPMB, respectively.

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