The Astrophysical Journal (Jan 2024)

Small-scale Cosmic-Ray Anisotropy Observed by the GRAPES-3 Experiment at TeV Energies

  • M. Chakraborty,
  • S. Ahmad,
  • A. Chandra,
  • S. R. Dugad,
  • U. D. Goswami,
  • S. K. Gupta,
  • B. Hariharan,
  • Y. Hayashi,
  • P. Jagadeesan,
  • A. Jain,
  • P. Jain,
  • S. Kawakami,
  • T. Koi,
  • H. Kojima,
  • S. Mahapatra,
  • P. K. Mohanty,
  • R. Moharana,
  • Y. Muraki,
  • T. Nakamura,
  • P. K. Nayak,
  • T. Nonaka,
  • A. Oshima,
  • B. P. Pant,
  • D. Pattanaik,
  • S. Paul,
  • G. S. Pradhan,
  • M. Rameez,
  • K. Ramesh,
  • S. Saha,
  • R. Sahoo,
  • R. Scaria,
  • S. Shibata,
  • T. Tabata,
  • H. Takamaru,
  • K. Tanaka,
  • F. Varsi,
  • K. Yamazaki,
  • M. Zuberi

DOI
https://doi.org/10.3847/1538-4357/ad132b
Journal volume & issue
Vol. 961, no. 1
p. 87

Abstract

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GRAPES-3 is a mid-altitude (2200 m) and near-equatorial (11.°4N) air shower array, overlapping in its field of view for cosmic-ray observations with experiments that are located in the Northern and Southern Hemispheres. We analyze a sample of 3.7 × 10 ^9 cosmic-ray events collected by the GRAPES-3 experiment between 2013 January 1 and 2016 December 31 with a median energy of ∼16 TeV for study of small-scale (<60°) angular-scale anisotropies. We observed two structures, labeled A and B, that deviate from the expected isotropic distribution of cosmic rays in a statistically significant manner. Structure A spans 50°–80° in R.A. and from −15° to 30° in decl. The relative excess observed in structure A is at the level of (6.5 ± 1.3) × 10 ^−4 with a statistical significance of 6.8 standard deviations. Structure B is observed in the R.A. range 110°–140° and at decl. from −10° to 30°. The relative excess observed in this region is at the level of (4.9 ± 1.4) × 10 ^−4 with a statistical significance of 4.7 standard deviations. These structures are consistent with those reported by Milagro, ARGO-YBJ, and HAWC. These observations could provide a better understanding of the sources of cosmic rays, their propagation, and the magnetic structures in our Galaxy.

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