Fig. 4.
Comparison of the Fe-Kα fluxes among different satellites, instruments, years, and regions. Open squares, filled circles, and filled triangle show the Fe-Kα fluxes obtained by Chandra, XMM-Newton, and Hitomi, respectively. Error bars show 90% confidence ranges.

Comparison of the Fe-Kα fluxes among different satellites, instruments, years, and regions. Open squares, filled circles, and filled triangle show the Fe-Kα fluxes obtained by Chandra, XMM-Newton, and Hitomi, respectively. Error bars show 90% confidence ranges.

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