Fig. 1
HESS J1825−137 and HESS J1826−130 γ-ray excess map (E > 0.2 TeV) extracted from the on-line material of the HGPS (H.E.S.S. Collaboration 2018).1 The wedge shows in units of 10−13 ph cm−2 s−1 the TeV flux.The plus signs indicate the position of the pulsars PSR J1826−1334 and PSR J1826−1256, and the diamonds the best-fit position of the TeV sources.
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