Location of the candidate WR stars we found in the Dragonfish complex (orange circles) together with Wolf-Rayet stars from the literature (red crosses) and the same clusters that are highlighted in Fig. 12 (green/blue squares; the blue ones host confirmed WR stars). 32% of clusters and 38% of WR candidates, as well as the bulk of confirmed WR stars, are located within the dotted rectangle. The dashed circumference shows the position and size of the overdensity of 2MASS sources found by Rahman et al. (2011a).