Determination of RV for 30 Dor. In the R136 region a): the MV of single O-type stars derived from HST/WFC3 photometry is plotted against the expected MV derived from VLT-MAD K-band photometry after applying the Martins & Plez (2006) calibration. In the MEDUSA region b): the MV derived from VFTS photometry is plotted against the expected MV derived from IRSF K-band photometry after applying the Martins & Plez (2006) calibration. Solid lines indicate the 1:1 relations.
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