Examples of FP cases in SAD-CNN. The first row illustrates various luminous structures such as satellite accretion or merging satellites that are misclassified as LSBFs taken from different Auriga halos at different snapshot lookback times. The second row displays FPs for halos at a 45° inclination. These models present prominent disc features, such as spiral arms, which were mistakenly classified as stellar streams. All models present the ${\mu }_{lim}^r$ in mag arcsec⁻² of different Auriga Halos. The box has a side of 300 kpc.