Supernova remnants in the SMC as seen by EPIC. Colours represent the same energy bands as in Fig. 5 and the panels are numbered according to Fig. 5. To more clearly reveal faint diffuse emission, all images were detector background-subtracted and both exposure- and vignetting-corrected and are shown with the scale indicated in the upper right. For a description of the markings see Sects. 2.1 (SNRs) and 2.2 (galaxy clusters). The bottom right panel shows the only known SMC SNR (Haberl et al. 2012) not covered by our survey.
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