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Fig. 4.


Left column: original HFF images in the four filters after PSF deconvolution and masking of star residuals and of the large foreground galaxy. Right column: stacked images of objects detected and reconstructed by three runs of DAWIS. The F105W residual map is smaller as a result of the WFC3 FoV being smaller than the ACS one, and has therefore been scaled to the other ones.

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