Predicted all-sky Galactic neutrino emission (solid lines) together with combined limits from IceCube and ANTARES (Albert et al. 2018) (dashed and dashed-dotted line for the KRAγ⁵ and KRAγ⁵⁰ model, respectively). The different colours represent neutrino emission from the same CR models for the γ-ray emission in Fig. 5. The blue line is the neutrino flux from the mixed CR Model A, and the orange and red lines show the emission assuming all CR species from Model A are H or Fe, respectively. The cyan curve shows the results for Model B.