Similar to Fig. 11 but for dwarf galaxies with stellar mass M_* < 10⁷ M_⊙ (see all 16 dwarf galaxies in this stellar mass range in Fig. C.2). On average, the galaxies in this stellar mass range do not host GCs; however, there are a few exceptions with GC number counts greater than zero. Considering the detections and possible contaminants, statistically one expects the dwarf galaxies FDSLSB45 (with M_* = 5.89 × 10⁵ M_⊙), FDSLSB43 (with M_* = 5.83 × 10⁵ M_⊙), FDS16_DWARF227 (with M_* = 5.78 × 10⁵ M_⊙), and FDSLSB36 (with M_* = 5.76 × 105 Mo) with 1.0, 0.7, 0.9, and 0.7 GCs, respectively (see Fig. C.2).