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Fig. 8.

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Three newly identified TDG candidates. (a) MATLAS-1180 (center), connected to a tidal tail extending from an interacting galaxy visible in the top-left corner; (b) MATLAS-947 (top-left corner), tidally connected to the ETG NGC 3610 (bottom-right corner) showing shell features; (c) MATLAS-1322 (center), with extended isophotes toward interacting galaxies on the bottom-left and top-right corners. The images are 7′ × 7′ for (a) and (c), and 20′ × 20′ for (b), with north up and east left. RGB images were produced with the help of the ASTROPY package, based on the method from Lupton et al. (2004).

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