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. Author manuscript; available in PMC: 2021 Oct 27.
Published in final edited form as: Astrophys J. 2019 Jul 30;880(2):95. doi: 10.3847/1538-4357/ab2880

Figure 44.

Figure 44.

The top panel shows the best-fit spectra resulting from the FSSC IEM using the Clean data class (with the Galactic diffuse index fixed). The bottom panel shows the resulting fractional count residuals. Black squares are for the Clean class (with the Galactic diffuse index fixed), green circles show the same fit but with the index of the Galactic diffuse component freed, and blue triangles are for the UltraCleanVeto (UCV) class (with Galactic diffuse index fixed). All components are fit in FM31, including the isotropic.