VFTS 682, a Wolf-Rayet star that is discussed in further detail by Bestenlehner et al. (2011), is shown in the K_s band (main) marked by a red circle and Hα/Hβ derived map as a red dot (subset). The red box in the K_s image represents the subset image’s field-of-view. The candidate is located in a relatively sparse field of stars and the subset shows that’s located in a region of relatively high A_V. VFTS 682 is the most massive candidate presented in this paper.