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Jing Zhou

Researcher at University of Chicago

Publications -  110
Citations -  8085

Jing Zhou is an academic researcher from University of Chicago. The author has contributed to research in topics: Pierre Auger Observatory & Cosmic ray. The author has an hindex of 36, co-authored 94 publications receiving 6828 citations. Previous affiliations of Jing Zhou include Istanbul University.

Papers
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

A. Aab, +627 more
TL;DR: In this paper, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 10(19) eV is presented, and upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky.
Journal ArticleDOI

Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

P. Abreu, +509 more
TL;DR: In this paper, the mean depth of cosmic ray air shower maximum and its dispersion were parametrized as functions of the first two moments of the ln A distribution and examined the goodness of this simple method through simulations of test mass distributions.
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Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

P. Abreu, +514 more
TL;DR: In this paper, the authors present comparative studies to identify and optimize the antenna design for the final configuration of the AERA consisting of 160 individual radio detector stations and rank the antennas with respect to the noise level added to the galactic signal.
Journal ArticleDOI

Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

Pierre Auger, +606 more
TL;DR: In this paper, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above $10^{19}$ eV is presented, and upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky.