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to work in the Galactic Archeaology group led by Prof. Sofia Feltzing. The main topic of research is foreseen to be the formation and evolution of the Milky Way thick disk. The primary aim of the project is
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Science, with around 80 employees, out of which about 25 are PhD students. The main research areas are Galaxies, Supernovae, Computational astrophysics, Solar Physics and Planet and star formation. Project
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simulations to have the full characterization of the structure of micorgels under flow at interfaces. The main objectives of this project are: (i) Probe the shape and architecture of individual microgels under
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cyber-physical systems. Its research spans from formal specification, verification, and synthesis, to runtime verification. Currently, the main focus is on developing methods and tools for: runtime
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) on virtually all fields related to solution NMR spectroscopy. The current chief expertise of NMR Uppsala is small molecule NMR spectroscopy, integrating applications from organic, natural product and medicinal
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. The main objectives of this project are: (i) Probe the shape and architecture of individual microgels under flow; (ii) characterize the structure of the microgels solutions under flow; (iii) probe
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northern Sweden, Finland, and Norway, is one of the primary sources. EISCAT uses radar technology to gather data on processes occurring in the atmosphere and ionosphere. Other data sources include
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, and synthesis, to runtime verification. Currently, the main focus is on developing methods and tools for: runtime assurance, the development of runtime monitoring approaches for the safe operation of