doi.eso.org

• Cioni, M.- R. L. [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Storm, Jesper [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Bell, Cameron P. M. [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Lemasle, Bertrand [Zentrum für Astronomie der Universität Heidelberg/Astronomisches Rechen-Institut, Germany]
• Niederhofer, Florian [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Bestenlehner, Joachim M. [Physics and Astronomy, University of Sheffield, UK]
• Youssoufi, Dalal El [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Feltzing, Sofia [Lund Observatory, Lund University, Sweden]
• González-Fernández, Carlos [Institute of Astronomy, University of Cambridge, UK]
• Grebel, Eva K. [Zentrum für Astronomie der Universität Heidelberg/Astronomisches Rechen-Institut, Germany]
• Hobbs, David [Lund Observatory, Lund University, Sweden]
• Irwin, Mike [Institute of Astronomy, University of Cambridge, UK]
• Jablonka, Pascale [Laboratoire d’astrophysique, École Polytechnique Fédérale de Lausanne, Switzerland]
• Koch, Andreas [Zentrum für Astronomie der Universität Heidelberg/Astronomisches Rechen-Institut, Germany]
• Schnurr, Olivier [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany; Cherenkov Telescope Array Observatory, Bologna, Italy]
• Schmidt, Thomas [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Steinmetz, Matthias [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]

The One Thousand and One Magellanic Fields (1001MC) survey aims to measure the kinematics and elemental abundances of many different stellar populations that sample the history of formation and interaction of the Magellanic Clouds. The survey will collect spectra of about half a million stars with G < 19.5 magnitudes (Vega) distributed over an area of about 1000 square degrees and will provide an invaluable dataset for a wide range of scientific applications.