Table 1
Spectral fits to the NuSTAR data.
(i) Absorbed power law | |||
Γ | NH | χ2/d.o.f. | |
1.26 ± 0.10 | 3.0 ± 0.6 | – | 56.70/55 |
(ii) With enhanced Fe metallicity | |||
Γ | NH | NH(Fe) | χ2/d.o.f. |
1.41 ± 0.11 | 3.2 ± 0.5 | 4.5 ± 0.9 | 48.80/54 |
(iii) SW &N components | |||
Γ | NHSW | NHN | χ2/d.o.f. |
1.9 | 2.6-1.1+0.9 | 14-4+7 | 46.20/54 |
Notes. Model (i) is a single power law modified by cold absorption. The value Γ is the photon index and NH is the hydrogen equivalent column density in units of 1023 cm-2, measured in the galaxy rest frame. Model (ii) is the same as Model (i), except that \nH for Fe is fitted independently from the other elements. Model (iii) assumes both SW and N sources have the standard power-law slope Γ = 1.9 and are modified by varying absorbing columns. Unlike in Models (i) and (ii), the effects of Compton scattering within the respective absorbing tori, computed by e-torus Ikeda et al. 2009, are included (see text for details). A narrow Gaussian for the Fe K line at 6.4 keV is included in all the fits. The fits with Models (i) and (iii) correspond to Figs. 2a and b, respectively.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.