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All-flavour search for neutrinos from dark matter annihilations in the Milky Way with IceCube/DeepCore

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Academic year: 2021

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Figure

Fig. 1 Schematic overview of the IceCube string layout seen from above. Gray-filled markers indicate IceCube strings and black markers indicate the DeepCore strings with denser DOM spacing
Fig. 2 The score distribution for the BDT trained on the b b ¯ 100 GeV signal channel (left) and for the BDT trained on the W + W − 300 GeV signal channel (right)
Fig. 3 Left All-flavour neutrino effective area as a function of energy for the two event selections of the analysis, the low-energy (LE) and high-energy (HE) selections
Fig. 5 Distributions of the ψ angles of the final event samples. The bin contents are directly proportional to the number of observed events, to which we choose not to assign any statistical uncertainty
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