A. Del Moro
The NuSTAR Extragalactic Survey: Average Broadband X-Ray Spectral Properties of the NuSTAR-detected AGNs
Del Moro, A.; Alexander, D.M.; Aird, J.A.; Bauer, F.E.; Civano, F.; Mullaney, J.R.; Ballantyne, D.R.; Brandt, W.N.; Comastri, A.; Gandhi, P.; Harrison, F.A.; Lansbury, G.B.; Lanz, L.; Luo, B.; Marchesi, S.; Puccetti, S.; Ricci, C.; Saez, C.; Stern, D.; Treister, E.; Zappacosta, L.
Authors
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
J.A. Aird
F.E. Bauer
F. Civano
J.R. Mullaney
D.R. Ballantyne
W.N. Brandt
A. Comastri
P. Gandhi
F.A. Harrison
G.B. Lansbury
L. Lanz
B. Luo
S. Marchesi
S. Puccetti
C. Ricci
C. Saez
D. Stern
E. Treister
L. Zappacosta
Abstract
We present a study of the average X-ray spectral properties of the sources detected by the NuSTAR extragalactic survey, comprising observations of the E-CDFS, EGS and COSMOS fields. The sample includes 182 NuSTAR sources (64 detected at 8-24 keV), with 3-24 keV fluxes ranging between f3−24keV≈10−14 and 6×10−13 erg/cm2/s (f8−24keV≈3×10−14−3×10−13 erg/cm2/s) and redshifts of z=0.04−3.21. We produce composite spectra from the Chandra+NuSTAR data (E≈2−40 keV, rest frame) for all the sources with redshift identifications (95%) and investigate the intrinsic, average spectra of the sources, divided into broad-line (BL) and narrow-line (NL) AGN, and also in different bins of X-ray column density and luminosity. The average power-law photon index for the whole sample is Γ=1.65+0.03−0.03, flatter than Γ≈1.8 typically found for AGN. While the spectral slope of BL and X-ray unabsorbed AGN is consistent with typical values (Γ=1.79+0.01−0.01), a significant flattening is seen in NL AGN and heavily-absorbed sources (Γ=1.60+0.08−0.05 and Γ=1.38+0.12−0.12, respectively), likely due to the effect of absorption and to the contribution from Compton reflection to the high-energy flux (E>10 keV). We find that the typical reflection fraction in our spectra is R≈0.5 (for Γ=1.8), with a tentative indication of an increase of the reflection strength with column density. While there is no significant evidence for a dependence of the photon index with X-ray luminosity in our sample, we find that R decreases with luminosity, with relatively high levels of reflection (R≈1.2) for L10−40keV<1044 erg/s and R≈0.3 for L10−40keV>1044 erg/s AGN, assuming Γ=1.8.
Citation
Del Moro, A., Alexander, D., Aird, J., Bauer, F., Civano, F., Mullaney, J., …Zappacosta, L. (2017). The NuSTAR Extragalactic Survey: Average Broadband X-Ray Spectral Properties of the NuSTAR-detected AGNs. Astrophysical Journal, 849(1), Article 57. https://doi.org/10.3847/1538-4357/aa9115
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 2, 2017 |
Online Publication Date | Oct 31, 2017 |
Publication Date | Oct 31, 2017 |
Deposit Date | Nov 29, 2017 |
Publicly Available Date | Nov 29, 2017 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 849 |
Issue | 1 |
Article Number | 57 |
DOI | https://doi.org/10.3847/1538-4357/aa9115 |
Public URL | https://durham-repository.worktribe.com/output/1339035 |
Files
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Copyright Statement
© 2017. The American Astronomical Society. All rights reserved.
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