NuSTAR observations of Mrk 766: distinguishing reflection from absorption
arXiv:1808.00014 · doi:10.1093/mnras/sty2081
Abstract
We present two new NuSTAR observations of the narrow line Seyfert 1 (NLS1) galaxy Mrk 766 and give constraints on the two scenarios previously proposed to explain its spectrum and that of other NLS1s: relativistic reflection and partial covering. The NuSTAR spectra show a strong hard (>15 keV) X-ray excess, while simultaneous soft X-ray coverage of one of the observations provided by XMM-Newton constrains the ionised absorption in the source. The pure reflection model requires a black hole of high spin () viewed at a moderate inclination ( degrees). The pure partial covering model requires extreme parameters: the cut-off of the primary continuum is very low ( keV) in one observation and the intrinsic X-ray emission must provide a large fraction (75%) of the bolometric luminosity. Allowing a hybrid model with both partial covering and reflection provides more reasonable absorption parameters and relaxes the constraints on reflection parameters. The fractional variability reduces around the iron K band and at high energies including the Compton hump, suggesting that the reflected emission is less variable than the continuum.
arXiv comment14 pages, 10 figures, MNRAS accepted
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