We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750 m. An inflection of the spectrum is observed, confirming the presence of the so-called second-knee feature. The spectrum is then combined with that of the 1500 m array to produce a single measurement of the flux, linking this spectral feature with the three additional breaks at the highest energies. The combined spectrum, with an energy scale set calorimetrically via fluorescence telescopes and using a single detector type, results in the most statistically and systematically precise measurement of spectral breaks yet obtained. These measurements are critical for furthering our un...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We present a measurement of the cosmic-ray spectrum above 100PeV using the part of the surface detec...
International audienceWe present a measurement of the cosmic-ray spectrum above 100 PeV using the pa...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
Abstract We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the sur...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
We present a measurement of the cosmic-ray spectrum above 100PeV using the part of the surface detec...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We present a measurement of the cosmic-ray spectrum above 100PeV using the part of the surface detec...
International audienceWe present a measurement of the cosmic-ray spectrum above 100 PeV using the pa...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
Abstract We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the sur...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface dete...
We present a measurement of the cosmic-ray spectrum above 100PeV using the part of the surface detec...
We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...
We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using...