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S. Parlati

Researcher at California Institute of Technology

Publications -  78
Citations -  11226

S. Parlati is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Cosmic ray & Pierre Auger Observatory. The author has an hindex of 30, co-authored 77 publications receiving 10348 citations.

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Geant4 developments and applications

TL;DR: GeGeant4 as mentioned in this paper is a software toolkit for the simulation of the passage of particles through matter, it is used by a large number of experiments and projects in a variety of application domains, including high energy physics, astrophysics and space science, medical physics and radiation protection.
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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

J. Abraham, +452 more
- 09 Nov 2007 - 
TL;DR: In this article, the authors demonstrate that there is a correlation between the arrival directions of cosmic rays with energy above 6 x 10{sup 19} eV and the positions of active galactic nuclei lying within 75 Mpc.
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Observation of the suppression of the flux of cosmic rays above 4x10(19) eV

J. Abraham, +488 more
TL;DR: The energy spectrum of cosmic rays above 2.5 x 10;{18} eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described and the hypothesis of a single power law is rejected with a significance greater than 6 standard deviations.
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Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

J. Abraham, +492 more
- 08 Mar 2010 - 
TL;DR: In this article, the authors reported a measurement of the flux of cosmic rays with unprecedented precision and statistics using the Pierre Auger Observatory based on fluorescence observations in coincidence with at least one surface detector.
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The Fluorescence Detector of the Pierre Auger Observatory

J. Abraham, +529 more
TL;DR: The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays as discussed by the authors, which combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array.