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1. Measurement of the proton-air cross section at √s=57 TeV with the Pierre Auger Observatory.

2. Measurement of the depth of maximum of extensive air showers above 10{18} eV.

3. Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV.

4. Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory.

5. Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

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