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Astroparticle studies at the Pierre Auger Observatory
Lili Yang, invited lecture at foreign university

Abstract: The Pierre Auger Observatory (PAO), the world’s largest cosmic ray detector combines a large surface detector (SD) with an air fluorescence detector (FD). It is designed to observe extensive air showers (EAS) of billions of secondary particles induced by the UHECRs in the earths’ atmosphere. The “hybrid” design (i.e., detected simultaneously by SD and FD) provides wealth of information about shower development and excellent event reconstruction. Together with observations of UHECRs, the Surface Detector (SD) of the PAO is sensitive to UHE neutrinos through the observation of deeply initiated inclined down-going showers produced by neutrino interactions in the atmosphere, which method has been well established. On the other hand, high-energy photons can also be discriminated from background of charged cosmic rays based on their characters of the shower front. In this talk, I will give a review on recent results from PAO and introduce the ultra-high energy multi-messenger studies from PAO.
Keywords: Pierre Auger Observatory, cosmic rays, ultra-high energy
Published in RUNG: 17.01.2018; Views: 3783; Downloads: 0
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173.
Results from the Pierre Auger Observatory
Ivan De Mitri, Andrej Filipčič, Samo Stanič, Darko Veberič, Danilo Zavrtanik, Marko Zavrtanik, 2015, published scientific conference contribution

Keywords: Pierre Auger Observatory, Ultra High Energy Cosmic Rays (UHECR), UHECR energy spectrum, UHECR mass composition
Published in RUNG: 27.06.2017; Views: 4183; Downloads: 0
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Searches for correlation between UHECR events and high-energy gamma-ray Fermi-LAT data
Gabrijela Zaharijas, 2016, original scientific article

Keywords: ultra-high-energy cosmic rays, Pierre Auger, Fermi LAT
Published in RUNG: 07.03.2017; Views: 4309; Downloads: 0
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