Physics
Scientist
Tata Institute of Fundamental Research, Homi Bhabha Marg, Colaba, Bombay-400 005, India
Angular resolution of an EAS array for gamma ray astronomy energies 5 X 10 (13) eV
Use of plexiglas sheets coated with wavelength-shifter dyes for detection of atmospheric Cherenkov radiation . A new technique for gamma ray astronomy at energies of ~ 1013-1014 eV
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