Chemical Abundance Analysis of Tucana III, the Second r-process Enhanced Ultra-faint Dwarf Galaxy This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.

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. Burke, A. Carnero RosellM. 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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