Detection rates of WD-fTDEs from dwarf galaxies (left panel) and from GCs (right panel) plotted for different S/N thresholds. The blue curve was calculated considering LISA as the detector, while the orange curve was obtained considering DO. The observation time for both instruments is assumed to be 10 years. The dashed black line is one event over 10 years. The occupation fraction is 1 for both scenarios.