The angular resolution of GRAPES-3 EAS array after improved timing and shower front curvature correction based on age and size
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(2020)
摘要
The angular resolution of an extensive air shower (EAS) array plays a critical role in determining its sensitivity for the detection of point gamma-ray sources in the multi-TeV energy range. The GRAPES-3, an EAS array located at Ooty in India (11.4 degrees N, 76.7 degrees E, 2200 m altitude) is designed to study gamma-rays in the TeV-PeV energy range. It comprises of a dense array of 400 plastic scintillators deployed over an area of 25000 m(2) and a large area (560 m(2)) muon telescope. The development of a new statistical method has allowed the real time determination of propagation delay of each detector in the GRAPES-3 array. The shape of the shower front is known to be curved and here the details of a new method developed for accurate measurement of the shower front curvature is presented. These two developments have led to a sizable improvement in the angular resolution of the GRAPES-3 array. It is shown that the curvature depends on the size and the age of an EAS. By employing two different techniques, namely, the odd-even and the left-right methods, independent estimates of the angular resolution are obtained. The odd-even method estimates the best achievable resolution of the array. For obtaining the angular resolution, the left-right method is used after implementing the size and age dependent curvature correction. A comparison of the angular resolution as a function of EAS energy by these two methods shows them be virtually indistinguishable. The angular resolution of the GRAPES-3 array is 47' for energies E>5 TeV and improves to 17' at E>100 TeV, eventually approaching 10' at E>500 TeV.
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关键词
cosmic ray experiments,cosmic rays detectors,gamma ray detectors,gamma ray experiments
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