Fig. 6
Examples of some follow-up images used to confirm stellar tidal stream candidates in our sample. The top row shows the SDSS g–r–i stacked images for NGC 7743, NGC 5750, and NGC 3041 (see Sect. 3) processed as described in Sect. 2, and kindly provided by A. Miskolczi. The bottom row shows the deep images obtained by the STSS (Martínez-Delgado et al., in prep.) for the same objects, but with a luminance filter. In all cases, the deeper images detect additional features or reveal a more detailed morphology of the features detected in the SDSS images.
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