“…A wise attitude is to wait for further data from all the running experiments which, in the the next few years, can reveal if these two hints at ∼ 2σ level will fluctuate down, or will consistently grow and confirm the preference for NO at a cumulative level > 3σ. On a longer time frame, discovery-level tests of the mass spectrum ordering will be provided by next-generation projects [41], not only with large-volume atmospheric neutrinos [186,187,188,189] but also with medium-baseline reactors such as JUNO [190] and new long-baseline accelerator facilities such as T2HK [191], DUNE [192] and ESSnuSB [193]. Finally, for discrete hypotheses like NO versus IO, the statistical interpretation of ∆χ 2 in terms of N σ remains effectively applicable, but must be taken with a grain of salt [194].…”