Modelling the Tucana III stream - a close passage with the LMC
D. Erkal*, T. S. Li, S. E. Koposov, V. Belokurov, E. Balbinot, K. Bechtol, B. Buncher, A. Drlica-Wagner, K. Kuehn, J. L. Marshall, C. E. Martínez-Vázquez, A. B. Pace, N. Shipp, J. D. Simon, K. M. Stringer, A. K. Vivas, R. H. Wechsler, B. Yanny, F. B. Abdalla, S. Allam
*Corresponding author for this work
- University of Surrey
- University of Cambridge
- Fermi National Accelerator Laboratory
- The University of Chicago
- Carnegie Mellon University
- Flatiron Institute
- LSST Corporation
- University of Illinois at Urbana-Champaign
- Australian Astronomical Observatory
- Texas A&M University
- National Optical Astronomy Observatory
- Carnegie Institution of Washington
- Stanford University
- University College London
- Rhodes University
- Institut d 'Astrophysique de Paris
- Laboratório Interinstitucional de e-Astronomia
- Observatório Nacional
- Autonomous University of Barcelona
- University of Wyoming
- University of Pennsylvania
- CIEMAT
- University of Arizona
- Jet Propulsion Laboratory, California Institute of Technology
- University of Michigan, Ann Arbor
- Universidad Autónoma de Madrid
- Institute of Space Studies of Catalonia
- Swiss Federal Institute of Technology Zurich
- University of California at Santa Cruz
- University of Southampton
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