Fig. 13
Effect of a forward moving shock wave applied to supernova at 10 kpc distance, modelled according to the Lawrence-Livermore model assuming an inverted hierarchy and θ13 > 0.9° was assumed. A forward shock wave can be distinguished from a static density profile and the case of no star matter effect. The 1 σ-band corresponding to measured detector noise (hatched area) has a width of about ± 1150 counts.
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