doi.eso.org

• Chiappini, Cristina [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Minchev, Ivan [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Starkenburg, Else [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Anders, Friedrich [Departament de Física Quàntica i Astrofísica, Universitat de Barcelona, Spain]
• Fusillo, Nicola Gentile [Department of Physics, University of Warwick, UK]
• Gerhard, Ortwin [Max-Planck-Institut für extraterrestrische Physik, Garching, Germany]
• Guiglion, Guillaume [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Khalatyan, Arman [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Kordopatis, Georges [Observatoire de la Côte d’Azur, Nice, France]
• Lemasle, Bertrand [Zentrum für Astronomie der Universität Heidelberg / Astronomisches Rechen- Institut, Germany]
• Matijevic, Gal [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Queiroz, Anna Barbara de Andrade [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Schwope, Axel [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Steinmetz, Matthias [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Storm, Jesper [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Traven, Gregor [Lund Observatory, Lund University, Sweden]
• Tremblay, Pier-Emmanuel [Department of Physics, University of Warwick, UK]
• Valentini, Marica [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Andrae, Rene [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Arentsen, Anke [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Asplund, Martin [Research School of Astronomy & Astrophysics, Australian National University, Canberra, Australia]
• Bensby, Thomas [Lund Observatory, Lund University, Sweden]
• Bergemann, Maria [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Casagrande, Luca [Research School of Astronomy & Astrophysics, Australian National University, Canberra, Australia]
• Church, Ross [Lund Observatory, Lund University, Sweden]
• Cescutti, Gabriele [Osservatorio Astronomico di Trieste, INAF, Italy]
• Feltzing, Sofia [Lund Observatory, Lund University, Sweden]
• Fouesneau, Morgan [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Grebel, Eva K. [Zentrum für Astronomie der Universität Heidelberg / Astronomisches Rechen- Institut, Germany]
• Kovalev, Mikhail [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• McMillan, Paul [Lund Observatory, Lund University, Sweden]
• Monari, Giacomo [Leibniz-Institut für Astrophysik Potsdam (AIP), Germany]
• Rybizki, Jan [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Ryde, Nils [Lund Observatory, Lund University, Sweden]
• Rix, Hans-Walter [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Walton, Nicholas [Institute of Astronomy, University of Cambridge, UK]
• Xiang, Maosheng [Max-Planck-Institut für Astronomie, Heidelberg, Germany]
• Zucker, Daniel [Department of Physics and Astronomy, Macquarie University, Sydney, Australia]
• The 4MIDABLE-LR Team

The mechanisms of the formation and evolution of the Milky Way are encoded in the orbits, chemistry and ages of its stars. With the 4MOST MIlky way Disk And BuLgE Low-Resolution Survey (4MIDABLE-LR) we aim to study kinematic and chemical substructures in the Milky Way disc and bulge region with samples of unprecedented size out to larger distances and greater precision than conceivable with Gaia alone or any other ongoing or planned survey. Gaia gives us the unique opportunity for target selection based almost entirely on parallax and magnitude range, hence increasing the efficiency in sampling larger Milky Way volumes with well-defined and effective selection functions.