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After a series of cuts to remove background events, they are left with two events, against an estimated background of 1 +/- 0.4 events - no statistically significant signal is observed. They set a limit on the possible flux of extra-terrestrial neutrinos which is considerably more restrictive than previous studies. Their limit is just starting to constrain models of GZK neutrino production. Clearly, a more sensitive experiment is needed.
ANITAs ability to observe a large chunk of Antarctica in one shot is a big plus. However, balloons have a limited observation time. And, the up-to-650 km separation between the source and the detector inevitably means that ANITA can only see the most energetic neutrino interactions. By placing our antennae directly in the Antarctic ice, ARIANNA will be able to see a wider range of neutrino energies, covering most of the GZK energy range.