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The IceCube Neutrino Observatory has discovered a diffuse neutrino flux ofastrophysical origin and measures its properties in various detection channels.With more than 10 years of data, we use multiple data samples from differentdetection channels for a combined fit of the diffuse astrophysical neutrinospectrum. This leverages the complementary information of different neutrinoevent signatures. For the first time, we use a coherent modelling of the signaland background, as well as the detector response and corresponding systematicuncertainties. The detector response is continuously varied during thesimulation in order to generate a general purpose Monte Carlo set, which iscentral to our approach. We present a combined fit yielding a measurement ofthe diffuse astrophysical neutrino flux properties with unprecedentedprecision.

Measurement of the astrophysical diffuse neutrino flux in a combined fit of IceCube's high energy neutrino data