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Sanchez, E. Suchyta, F. Sobreira, G. Gutierrez, G. Tarle, H. T.Diehl, I. Sevilla-Noarbe, J. Carretero, J. Frieman, J. L. Marshall, J. Thaler, K. Honscheid, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Carrasco Kind, M. E. C. Swanson, M. Schubnell, M. Soares-Santos, N. Kuropatkin, O. Lahav, P. Fosalba, P. Martini, R. A. Gruendl, R. C. Nichol, R. C. Smith, R. Miquel, R. Ogando, S. Allam, S. Desai, T. F. Eifler, T. S. Li, V. Scarpine","submitted_at":"2015-12-03T11:00:09Z","abstract_excerpt":"The Large Magellanic Cloud (LMC) harbors a rich and diverse system of star clusters, whose ages, chemical abundances, and positions provide information about the LMC history of star formation. We use Science Verification imaging data from the Dark Energy Survey to increase the census of known star clusters in the outer LMC and to derive physical parameters for a large sample of such objects using a spatially and photometrically homogeneous data set. 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