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engineering. Experience with experimental measurements, image-based diagnostics, laboratory testing or quantitative data analysis. Coding and analysis capability in Python and/or Julia, preferably with
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while working effectively within a multidisciplinary team. Candidates who are in the process of completing their H1 degree will be considered. Applicants who already hold a PhD degree will not be
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. Analysis of this data will employ both qualitative and quantitative methods. Work on WP-2 will suit someone with an interest and aptitude for coding administrative data using large language models. It will
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group’s projects often combine astronomy, coding, visualisation, and data science, and work well for students who enjoy either astrophysics, machine learning/coding, or both. The multidimensional structure
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nucleosynthesis in violent episodes suffered by ancient stars" (with Dr Carolyn Doherty) "Applying 3D stellar hydrodynamics findings to 1D stellar codes: Improving the modelling of convection in stars" web page
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submitting an EOI: A cover letter not exceeding 500 words stating your suitability and research interest. A curriculum vitae including peer-reviewed publications, conference presentations, and relevant
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spectroscopy" "Chemical abundances in star clusters using Korg, the first spectral synthesis code developed in two decades" web page For further details or alternative project arrangements, please contact
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these requirements before deciding whether they should apply. Scholarship holders must be enrolled full-time and on campus. Please note: applicants who already hold a PhD will not be considered. The successful
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not exceeding 500 words stating your suitability and research interest. A curriculum vitae including peer-reviewed publications, conference presentations, and relevant research/work experience. Scanned
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they familiarise themselves with these requirements before deciding whether they should apply. Scholarship holders must be enrolled full-time and on campus. Please note: applicants who already hold a PhD will not be