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Angular Resolution of an EAS Array for Gamma Ray Astronomy at Energies Greater Than 5 x 10 (13) EvA 24 detector extensive air shower array is being operated at Ootacamund (2300 m altitude, 11.4 deg N latitude) in southern India for a study of arrival directions of showers of energies greater than 5 x 10 to the 13th power eV. Various configurations of the array of detectors have been used to estimate the accuracy in determination of arrival angle of showers with such an array. These studies show that it is possible to achieve an angular resolution of better than 2 deg with the Ooty array for search for point sources of Cosmic gamma rays at energies above 5 x 10 to the 13th power eV.
Document ID
19850026672
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Apte, A. R.
(Tata Inst. of Fundamental Research Bombay, India)
Gopalakrishnan, N. V.
(Tata Inst. of Fundamental Research Bombay, India)
Tonwar, S. C.
(Tata Inst. of Fundamental Research Bombay, India)
Uma, V.
(Tata Inst. of Fundamental Research Bombay, India)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 3
Subject Category
Space Radiation
Report/Patent Number
OG-9.5-8
Accession Number
85N34985
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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