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Field
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actor analysis, implemented through case studies. These include youth surveys, an examination of local governance mechanisms, the provision of local infrastructure, and the organisation of actors and
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development of numerical algorithms and analysis necessary for simulating and understanding complex, multi-scale systems. The group is part of the Mathematics in Computation (MiC) Section
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specialist in high-resolution spectroscopy Have a good knowledge of methods for extracting stellar radial velocity A good knowledge of the processes occurring in the photosphere of active stars and numerical
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travel allowance and access to advanced computing resources. The MMD group is responsible for the design and development of numerical algorithms and analysis necessary for simulating and understanding
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uncertainty quantification. The position comes with a travel allowance and access to advanced computing resources. The MMD group is responsible for the design and development of numerical algorithms and
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compare the simulated galaxies to JWST observations (in particular COSMOS-Web). - Creation of synthetic observations from the numerical simulations; - Scientific exploitation and interpretation
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with the main field of application being topological photonics based on microcavities. Analytical calculations Numerical calculations Analysis of experimental data The work will be carried out
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the research and education has a unique breadth, with large activities in classical scientific computing areas such as mathematical modeling, development and analysis of algorithms, scientific software
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in drawing styles, the numerous elements and their complex relationships, and the implicit meanings of specific symbols. By accelerating RP analysis with AI, RPs can also be used as a measurement tool
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modelling; perform rigorous statistical analysis and ensure reproducible workflows (well‑documented code/analysis) Report and disseminate results (manuscripts, conference talks), contribute to grant writing