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Fig. 1
Suzaku images (in counts) of the SNR 1E 0102-72.3 (obsID: 101005050), in the full energy band (top) where the pulsar and the SNR are confused, and in the 2.5−10 keV band (bottom) where the contribution of the SNR is negligible.
This figure is made of several images, please see below:
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