41 coding-"Prof"-"Foundation-for-Research-and-Technology-Hellas"-"Prof" positions at CNRS in France
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beamline at the ESRF. The analysis and interpretation of the acquired data will require solid proficiency with the various code bases developed on the beamline. The candidate will be trained in the use
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Code34094Street141 rue de la CardonilleGeofield Contact City Montpellier Website http://www.igf.cnrs.fr/index.php/en/ Street 141 rue de la Cardonille Postal Code 34094 E-Mail cedric.leyrat@igf.cnrs.fr STATUS: EXPIRED
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proteins in lipid droplets; (2) development and maintenance of the POP_MD code for non-equilibrium molecular dynamics simulations of biological systems. The successful candidate will be responsible
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geodetic observations. * Writing and documenting simulation codes for for open distribution. * Communicating the results at international conferences and publishing them in international, open-access
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. An in-depth study conducted by the SFDE in conjunction with the Health and Biodiversity Alliance shows the need for legislation to transform codes and introduce a One Health principle. Recently, the
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. Their results will be convolved with advanced radiative codes to calculate fluxes and multi-messenger spectra. These simulations will also be supplemented by kinetic simulations of particle acceleration in
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environments. • Write and execute code in R, Python, GitHub etc., high-performance computing. • Evidence of ability to publish research results in international peer-reviewed journals. • Ability to organize and
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including sequencing data. • Analysis skills: write and execute code in R, Python, GitHub etc., high-performance computing. • Strong oral and written communication skills in English. • Ability to work
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Lyon Website https://www.cnrs.fr/fr https://lbti.ibcp.fr/ Street 7, Passage du Vercors Postal Code 69007 E-Mail catherine.moali@cnrs.fr STATUS: EXPIRED X (formerly Twitter) Facebook LinkedIn Whatsapp
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" (ARMS) code, running on high-performance computing centers. The simulation domain will consist of a restricted portion of the solar atmosphere. The doctoral student will have to explore the simulation