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Inria, the French national research institute for the digital sciences | Villeneuve la Garenne, le de France | France | about 1 month ago
algorithms, and to publish these results in research papers. bibliographic work algorithm design and their theoretical analysis numerical simulations writing scientific papers Where to apply Website https
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, with a strong background in one or more of the following areas: ice dynamics, numerical modelling, subglacial processes, geophysical data analysis, the use of remote sensing in geoscience. Experience
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computing resources. The MMD group is responsible for the design and development of numerical algorithms and analysis necessary for simulating and understanding complex, multi-scale systems. The group is part
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of 15 minutes, will be classified on a numerical scale from 0 to 100 points, applying the following parameters and criteria evaluation: a) attitude and critical sense (ACS) b) motivation of the candidate
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+ 0.2 EMA. 9.4. The Interview (INT), with the duration of 15 minutes, will be classified on a numerical scale from 0 to 100 points, applying the following parameters and criteria evaluation: a) attitude
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high-performance classical simulations, working at the interface between quantum theory, numerical methods, and large-scale scientific data analysis. The position is not limited to quantum computing and
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About the Opportunity JOB SUMMARY The Blazek group performs research in cosmology, including both theoretical, observational, and numerical methods. We are involved in analysis of DES data and
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within various scientific and engineering disciplines, including ground-based, airborne, and satellite measurements, numerical modelling, and data analysis. The division's goals are to enhance
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of Integrative Physiology focuses on inherited and acquired arrhythmias and cardiomyopathies. The lab utilizes numerous techniques from cloning and in vitro cell work, to the generation of mutant mice and surgical
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numerical cosmology. The successful candidate will lead the develop of realistic simulations of a galaxy, lensing, X-ray and CMB secondary observables. This will be built on the backlight simulations, a new