345 coding-"https:"-"Prof"-"FEMTO-ST" "https:" "https:" "https:" "https:" "https:" "U.S" "St" research jobs at CNRS
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of the project. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre/UMR7587-PEDBAR-007/Candidater.aspx Requirements Research FieldEngineeringEducation LevelPhD or equivalent Research FieldPhysicsEducation
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Website https://emploi.cnrs.fr/Candidat/Offre/UMR9002-ANNRAM-002/Candidater.aspx Requirements Research FieldBiological sciencesEducation LevelPhD or equivalent Research FieldBiological sciencesEducation
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of the ANR Lamorsim project (https://anr.fr/Project-ANR-23-CE08-0029 ). The main objective of this project is to develop methodologies for achieving controlled laser-induced amorphization of silicon. In this
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. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre/UMR8243-TIFKON-004/Candidater.aspx Requirements Research FieldComputer scienceEducation LevelPhD or equivalent Research
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to the main plasma physics conferences. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre/UMR7345-YANCAM-002/Candidater.aspx Requirements Research FieldPhysicsEducation LevelPhD or equivalent
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postdoc will: ● Start by familiarizing with existing research and methods for genome interpretation, such as the AI4GI lab previous publications (https://academic.oup.com/nar/article/50/3/e16/6430850?login
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in project meetings and team and lab meetings in Villefranche. The Laboratoire d'Océanographie de Villefranche (LOV ; http://lov.obs-vlfr.fr/ ) is located close to Nice, on the French Riviera. It
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(UCBL/CNRS/CNES/ArianeGroup). The laboratory has internationally recognized expertise (NASA, U.S. Defense Energy Center Support / DESC, etc.) in the fundamental chemistry of N-N interactions, including
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aérothermochimieCountryFranceCityST ETIENNE DU ROUVRAYGeofield Contact City ST ETIENNE DU ROUVRAY Website http://www.coria.fr STATUS: EXPIRED X (formerly Twitter) Facebook LinkedIn Whatsapp More share options E-mail Pocket Viadeo
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of very-high-energy gamma-ray sources, in the context of study of magnetic fields in the Milky Way galaxy and in the intergalactic medium. The work will include development of numerical code for modelling