Image Details
Caption: Figure 9.
Integrated spectrum from Obs. 3A from a portion of the stray light region. A similar-sized region was used to estimate the background. The base model spectrum here consists of a hot accretion disk component and a soft nonthermal power law, though this leaves strong residuals near the Fe line (middle). We find that after the addition of a broad Fe line and absorption features associated with disk winds in this system that we obtain a reasonable fit to the data.
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