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most citedDepth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Composition Implications

309 citations · 1.9k across the 31 of their papers we have counts for

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15 papers · 1 filter

astro-ph.HE2014★ 309 cited

Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Composition Implications

Pierre Auger Collaboration

Using the data taken at the Pierre Auger Observatory between December 2004 and December 2012, we have examined the implications of the distributions of depths of atmospheric shower…

astro-ph.HE2014★ 37 cited

A search for point sources of EeV photons

Pierre Auger Collaboration, A. Aab, P. Abreu +483

Measurements of air showers made using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point…

astro-ph.HE2013★ 56 cited

Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

Pierre Auger Collaboration

The observation of ultrahigh energy (UHE) neutrinos has become a priority in experimental astroparticle physics. UHE neutrinos can be detected with a variety of techniques. In part…

astro-ph.HE2012★ 41 cited

Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

Mariangela Settimo

The energy spectrum of ultra-high energy cosmic rays above 10 eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and Sept…

astro-ph.HE2012★ 20 cited

Search for microwave emission from ultrahigh energy cosmic rays

J. Alvarez-Muñiz, A. Berlin, M. Bogdan +17

We present a search for microwave emission from air showers induced by ultrahigh energy cosmic rays with the microwave detection of air showers experiment. No events were found, ru…

astro-ph.HE2012★ 78 cited

A search for ultra-high energy neutrinos in highly inclined events at the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +497

The Surface Detector of the Pierre Auger Observatory is sensitive to neutrinos of all flavours above 0.1 EeV. These interact through charged and neutral currents in the atmosphere…