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When measuring star formation rates using ultraviolet light, correcting fordust extinction is a critical step. However, with the variety of dustextinction curves to choose from, the extinction correction is quite uncertain.Here, we use Swift/UVOT to measure the extinction curve for star-formingregions in the SMC and M33. We find that both the slope of the curve and thestrength of the 2175 Angstrom bump vary across both galaxies. In addition, aspart of our modeling, we derive a detailed recent star formation history foreach galaxy.

UVOT Measurements of Dust and Star Formation in the SMC and M33