Extended Data Fig. 6: Sgr dSph spectra derived from template analysis using different Galactic diffuse emission models.
From: Gamma-ray emission from the Sagittarius dwarf spheroidal galaxy due to millisecond pulsars
In all cases the spectrum shown is the flux averaged over the entire ROI, not the flux within the footprint of the Sgr dSph template. The fiducial model is our default choice (first entry in Table 1), while other lines correspond to alternate foregrounds - models 2D A (red), 2D B (black), and 2D C (blue) for the Galactic IC foreground, and models Interpolated (dark green) and GALPROP 3D-gas (light green) for the Galactic hadronic + bremsstrahlung foreground. The error bars display 1σ statistical errors. See Table 1 and text for details.
