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Fig. F.1.
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0.7-7 keV Chandra spectra of the 38 region segments, dX0 through dX37, over the diffuse emission. The flux density, FE, is in units of 10−14 erg s−1 cm−2 keV−1. The two highest energy bins corresponds to the two Fe-line bands of cold Fe K at 6.4 keV and Fe XXV at 6.7 keV.
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