![]() |
Figure 1:
|
| Open with DEXTER | |
![]() |
Figure 2: Significance map centered on PSR B1706-44. The cross marks the pulsar position. The contour lines correspond to the 2.2 GHz image of G 343-2.3 (Duncan et al. 1995). The solid circle indicates the integration region of the Standard cuts, the dashed circle the CANGAROO cuts and the dot-dashed circle the Radio arc cuts. The significance distribution for the entire HESS field of view is compatible with a Gaussian of mean -0.06 and of sigma 1.09. |
| Open with DEXTER | |
![]() |
Figure 3: Integral upper limits at 99% CL for the flux from the PWN position (solid, dotted and dot-dashed line). The filled circle corresponds to the CANGAROO detection of Kifune et al. (1995) and the CANGAROO integrated flux (grey area) is calculated from the result of a broken power law fit to the 2000 and 2001 differential spectrum (Kushida et al. 2003). The open diamond and the triangle are from Rowell et al. (1998) and Chadwick et al. (1998), respectively. |
| Open with DEXTER | |