Fig. A.3
Emission line HST/WFC3 images of the region surrounding source No. 116. Left panel: WFC3 image with the narrowband filter F657N, corresponding to Hα line emission. Right panel: WFC3 image with the narrowband filter F673N, corresponding to SII line emission. The radii of the circles of Chandra (SW105) and XMM-Newton (116) sources give the 3σ accuracy of the position of the sources. The circle labelled BL53 gives the position of the opitcal SNR candidate.
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