Fig. 18


Significance () of the VHE γ-ray excess, centered on the new source HESS J1119−614, with the H.E.S.S. The PSF for this data set shown inset. The black circle at the center indicates the 68% uncertainty in the best-fit centroid of the VHE emission. The white circle represents the 70% containment region of the emission (R_SPEC, used also for spectral measurement). The approximate size of the radio shell of SNR G292.2−0.5 is shown as agreen circle and the PWN G292.15−0.54 as a green marker. The position of the pulsar PSR J1119−6127 is denoted by a cyan diamond. The FoV is 1.5° × 1.5°.

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