Close-up view of the t-SNE embeddings for HSD (left panel) and CV (right panel) clusters. Left panel: HSD sub-clusters 0 and 1 represent the cluster HSD in Fig. 2c, where p-mode hot subdwarfs were identified from Baran et al. (2024), while the other modes (g, p+g, g mode + binary) were taken from (Krzesinski & Balona 2022). Right panel: Magnetic CVs (mCVs), non-magnetic CVs (non-mCVs), and dwarf novae (DNs) from Canbay et al. (2023) are shown.