CANGAROO-III Observation of TeV Gamma Rays from the vicinity of PSR B1 706-44
R.Enomoto, J.Kushida, T.Nakamori, T.Kifune, G.V.Bicknell, R.W.Clay,, P.G.Edwards, S.Gunji, S.Hara, T.Hara, T.Hattori, S.Hayashi, Y.Higashi,, Y.Hirai, K.Inoue, H.Ishioka, S.Kabuki, F.Kajino, H.Katagiri, A.Kawachi,, R.Kiuchi, H.Kubo, T.Kunisawa, T.Matoba, Y.Matsubara, I.Matsuzawa

TL;DR
This paper reports the detection of extended TeV gamma-ray emission near pulsar PSR B1706-44 using the CANGAROO-III telescope, highlighting uncertainties due to background emission and complex Galactic structures.
Contribution
First detection of extended TeV gamma-ray emission around PSR B1706-44 with analysis of background uncertainties and complex Galactic emission effects.
Findings
Detection of extended TeV gamma-ray emission near PSR B1706-44
Variability in signal strength based on background estimation methods
Complex structure of gamma-ray emission in the Galactic plane
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 B170644. 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 B170644.
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