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Figure 1: BeppoSAX MECS hardness ratio (4-10.5 keV)/(1.5-4 keV). |
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Figure 2:
EPIC-PN residuals around the iron line energy for
the second XMM- Newton observation when fitting with
a simple absorbed power law (upper panel), and with a power law plus a narrow Gaussian whose flux is fixed to
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Figure 3: Chandra HEG residuals when fitting with a simple absorbed power law around the iron line energy. |
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Figure 4:
Fe K![]() |
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Figure 5:
Fe K![]() |
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Figure 6:
Fe K![]() ![]() |
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