Abstract
Observation by the CANGAROO-III stereoscopic system of the Imaging Cherenkov Telescope has detected extended emission of TeV gamma rays in the vicinity of the pulsar PSR B1706-44. The strength of the signal observed as gamma-ray-like events varies when we apply different ways of emulating background events. The reason for such uncertainties is argued in relevance to gamma rays embedded in the "OFF-source data," that is, unknown sources and diffuse emission in the Galactic plane, namely, the existence of a complex structure of TeV gamma-ray emission around PSR B1706-44. © 2009 The American Astronomical Society. All rights reserved.
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Enomoto, R., Kushida, J., Nakamori, T., Kifune, T., Bicknell, G. V., Clay, R. W., … Yukawa, Y. (2009). Cangaroo-III observation of tev gamma rays from the vicinity of PSR B1706-44. Astrophysical Journal, 703(2), 1725–1733. https://doi.org/10.1088/0004-637X/703/2/1725
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