Example of a dwarf galaxy successfully detected in the VIS BGSUB mosaic (left panel). The second background subtraction affects its appearance (along with the square-shaped background mesh used in the process) and consequently its structural parameters in the final MER mosaic (right panel). Both images use the same scale. It is worth noting that this is the brightest (I_E = 18) and most extended galaxy in our sample at 10 Mpc and that such objects are statistically rare in the Local Universe.