Images of the SXS showing individual counts as a pixels on the sky. Blue boxes are counts included after relaxing the angular distance criterion. The red contours trace the Chandra emission, and the green circles show radii of 1|$ {^{\prime}_{.}} $|5 and 2|$ {^{\prime}_{.}} $|0 from the Chandra peak. The counts in Fe K (right) correspond well to the remnant extent, while some of the counts in the other bands are outside the bounds of the remnant.