102 cloud-computing-"https:" "https:" "https:" "https:" "https:" "St" "St" positions at University of Leeds
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consider eligibility under the Global Talent visa. For more information please visit: https://www.gov.uk/global-talent To explore the post further or for any queries you may have, please contact: Dr Steve
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preparedness and refining projections of glacier evolution across High-Mountain Asia. You will contribute to creating systematic and open access glacial lake monitoring through our Glacial Lake Observatory (http
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Design or Human-Computer Interaction, and a developing record of either research, pedagogy, or commercial and industrial collaboration commensurate with the level of the post. You will have an in depth
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. Information on other visa options is available at: https://www.gov.uk/browse/visas-immigration/work-visas  ; What we offer in return Generous pension scheme options plus life assurance Health and Wellbeing
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and increase access in the Oxford Common File Layout (OCFL) standard; A foundational cloud infrastructure for digital humanities research and teaching. You will utilise your skills, knowledge and
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Layout (OCFL) standard; A foundational cloud infrastructure for digital humanities research and teaching. You will utilise your skills, knowledge and experience to provide high quality and proactive
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programme grant “Total Body Nuclear Imaging for the Development of Nanotheranostics”. This Programme involves 15 co-investigators in a range of disciplines related to PET imaging strategies
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Project Link: Image guided intervention supported with mixed reality | Project Opportunities | PhD | University of Leeds Eligibility: UK and International Funding: School of Computer
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contribute to teaching students in the School’s undergraduate programme in Paediatric Dentistry. You will participate in the maintenance and further development of excellence in the quality of education within
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School of Physics and Astronomy. You will carry out a research programme analysing stellar populations and chemical enrichment processes in galaxies using large galaxy surveys such as SDSS and DESI, as