Chemical abundance analysis of Tucana III, the second r-process enhanced ultra-faint dwarf galaxy

DES Collaboration, J. L. Marshall*, T. Hansen, J. D. Simon, T. S. Li, R. A. Bernstein, K. Kuehn, A. B. Pace, D. L. Depoy, A. Palmese, A. Pieres, L. Strigari, A. Drlica-Wagner, K. Bechtol, C. Lidman, D. Q. Nagasawa, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. BurkeA. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. E. Cunha, C. B. D'Andrea, L. N.Da Costa, J. De Vicente, S. Desai, P. Doel, T. F. Eifler, B. Flaugher, P. Fosalba, J. Frieman, J. Garciá-Bellido, E. Gaztanaga, D. W. Gerdes, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, D. L. Hollowood, K. Honscheid, B. Hoyle, D. J. James, N. Kuropatkin, M. A.G. Maia, F. Menanteau, C. J. Miller, R. Miquel, A. A. Plazas, E. Sanchez, B. Santiago, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, M. Smith, M. Soares-Santos, E. Suchyta, M. E.C. Swanson, G. Tarle, W. Wester

*Corresponding author for this work

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