A new array for the study of ultra high energy gamma-ray sources

Details A new array for the study of ultra high energy gamma-ray sources A new array for the study of ultra high energy gamma-ray sources

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3..426b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 426-429 (SEE N85-34862 23-93)

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Applications

Angular Resolution, Cosmic Ray Showers, Gamma Rays, Point Sources, Scintillation Counters, Signal To Noise Ratios, Arrays, Calibrating, Cerenkov Counters, Data Recording, Laser Applications, Photomultiplier Tubes, Time Measurement

Scientific paper

This paper describes the design and operation of a 32×1 m2 array of scintillation detectors for the detection of 1015eV cosmic rays with an expected angular resolution of <1°, thus improving the present signal/background ratio for γ-ray sources. Data are recorded on a hybrid CAMAC and "in-house" system which uses a laser and Pöckel-Cell arrangement to routinely calibrate the timing stability of the detectors.

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