Figure 7
Expected sensitivity for the effective annihilation cross-section, in the case of γ-ray observations of the Sagittarius galaxy and for DM particles annihilating into WW. The band represents the astrophysical uncertainty.

Expected sensitivity for the effective annihilation cross-section, in the case of γ-ray observations of the Sagittarius galaxy and for DM particles annihilating into WW. The band represents the astrophysical uncertainty.

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