Showing 1–20 of 43 results
/ Date/ Name
Nov 10, 2011Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger ObservatorySep 18, 2012Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger ObservatoryNov 30, 2011The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger ObservatoryNov 28, 2011The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger ObservatoryJan 24, 2011Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger ObservatoryJun 11, 2009The Cosmic Ray Energy Spectrum and Related Measurements with the Pierre Auger ObservatoryJun 11, 2009Studies of Cosmic Ray Composition and Air Shower Structure with the Pierre Auger ObservatoryJun 12, 2009Calibration and Monitoring of the Pierre Auger ObservatoryJun 11, 2014A search for point sources of EeV photonsMar 17, 2017Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger ObservatoryAug 3, 2000Origin of the highest energy cosmic rays observedMay 5, 2016Prototype muon detectors for the AMIGA component of the Pierre Auger ObservatorySep 27, 2016Evidence for a mixed mass composition at the `ankle' in the cosmic-ray spectrumJul 24, 2011The Pierre Auger Observatory III: Other Astrophysical ObservationsJul 24, 2011The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related MeasurementsOct 26, 2016Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger ObservatoryJun 12, 2009Operations of and Future Plans for the Pierre Auger ObservatoryMar 14, 2011Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger ObservatoryJul 24, 2011The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction modelsJul 24, 2011The Pierre Auger Observatory V: Enhancements