Angular resolution of an EAS array for gamma ray astronomy energies 5 X 10 (13) eV

Details Angular resolution of an EAS array for gamma ray astronomy energies 5 X 10 (13) eV Angular resolution of an EAS array for gamma ray astronomy energies 5 X 10 (13) eV

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3..469a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 469-472 (SEE N85-34862 23-93)

Physics

Angular Resolution, Arrays, Cerenkov Radiation, Cosmic Ray Showers, Gamma Ray Bursts, Gamma Ray Telescopes, Interstellar Magnetic Fields, Directivity, India, Rates (Per Time), Scintillation Counters

Scientific paper

A 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.

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