411 master-"https:" "https:" "https:" "https:" "Robert Gordon University" Fellowship positions in Norway
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other relevant activities. Copies of diplomas with all grades included in the degree and certificates (if the original language of diplomas/certificates is not English or a Scandinavian language, an
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required documents. The letter should schematically include: Master thesis topic and a brief description of its original content (e.g., new results, new codes, innovative methodology). Links to any public
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across a range of stellar masses and ages, with direct applicability to studies of planetary atmospheric evolution. Starting from the most active pre-main-sequence end of the cool star sequence, where
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for three years. About the project/work tasks: We invite original and ambitious project proposals within the fields of art history, social anthropology, ethnology, and archaeology. Proposals that cross
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. The research fellow must take part in the Faculty’s approved PhD program (TIK track) and is expected to complete the project within the set fellowship period. The main purpose of the fellowship is research
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founder and now chief scientist) and leading research groups in Europe (LSE, Oxford, KU Leuven) and North America (Harvard, Dartmouth). The Postdoctoral Fellow will be part of the Department of Behavioural
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comprises more than 200 faculty members from many higher education institutions in Norway, in collaboration with numerous public and private sector partners. The primary objective of MishMash is to create
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of employment is Oslo. More about the position and what your main tasks will be The postdoctoral fellow will conduct research on transnational waste trafficking (such as electronic waste, scrap cars, paper and
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, thereby testing currently competing planet formation models against observations. The primary responsibilities of this position involve the implementation of chemical compositions for forming exoplanets
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. The Moon-forming collision might have been a "hit-and-run-return’’ where accretion happened only on the second try. The main work is to model giant impacts using a high-heritage SPH model supported by