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M

M. J. Chae

Researcher at Ewha Womans University

Publications -  16
Citations -  1224

M. J. Chae is an academic researcher from Ewha Womans University. The author has contributed to research in topics: Telescope & Cosmic ray. The author has an hindex of 11, co-authored 16 publications receiving 1157 citations.

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Indications of intermediate-scale anisotropy of cosmic rays with energy greater than 57 EeV in the northern sky measured with the surface detector of the Telescope Array experiment

Rasha Abbasi, +125 more
TL;DR: In this paper, the authors search for intermediate-scale anisotropy in the arrival directions of ultra-high-energy cosmic rays with energies above 57 EeV in the northern sky using data collected over a 5-year period by the surface detector of the Telescope Array experiment.
Journal ArticleDOI

Indications of Intermediate-Scale Anisotropy of Cosmic Rays with Energy Greater Than 57 EeV in the Northern Sky Measured with the Surface Detector of the Telescope Array Experiment

Rasha Abbasi, +124 more
TL;DR: In this paper, the authors search for intermediate-scale anisotropy in the arrival directions of ultra-high-energy cosmic rays with energies above 57~EeV in the northern sky using data collected over a 5 year period by the surface detector of the Telescope Array experiment.
Journal ArticleDOI

Study of Ultra-High Energy Cosmic Ray composition using Telescope Array’s Middle Drum detector and surface array in hybrid mode

Rasha Abbasi, +126 more
TL;DR: In this paper, the authors compare the results of the HiRes and PAO UHECR measurements to the results obtained by the QGSJetII-03 and QGS jet-01c models.
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

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

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.