Fig. 2
2.5 × 2.5 parsec (10′′ × 10′′) logarithmically stretched grey scale images of each of the stars. All of the candidates were observed in the F814W band except for VFTS 682 and VFTS 849, which are observed in the F673N and F606W bands, respectively. Additionally, all of the candidates were observed with the WFPC2, except for VFTS 123, 208 and 216 which were observed with ACS.
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