178 evolution-"https:"-"https:"-"https:"-"https:"-"University-of-Liverpool" Fellowship positions in Norway
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development (R&D) activities within technical subjects, arts and design. The Faculty has approximately 4.000 students and 400 staff members and is situated at Pilestredet Campus in downtown Oslo and at Kjeller
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development (R&D) activities within technical subjects, arts and design. The Faculty has approximately 4.000 students and 400 staff members and is situated at Pilestredet Campus in downtown Oslo and at Kjeller
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development (R&D) activities within technical subjects, arts and design. The Faculty has approximately 4.000 students and 400 staff members and is situated at Pilestredet Campus in downtown Oslo and at Kjeller
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disciplines. The candidate will participate in the development of methodologies for repatriation and post-repatriation work. Knowledge of cultural heritage, museums, provenance, material culture and
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development and evidence-to-practice initiatives. The fellow will work within an international network of leading researchers, clinicians, journals, and policy organisations and will have opportunities for high
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. October 2026. This is a trainee position that will give promising researchers an opportunity for academic development through a PhD education leading to a doctoral degree. The hired candidate will be
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development (R&D) activities within technical subjects, arts and design. The Faculty has approximately 4.000 students and 400 staff members and is situated at Pilestredet Campus in downtown Oslo and at Kjeller
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development (R&D) activities within technical subjects, arts and design. The Faculty has approximately 4.000 students and 400 staff members and is situated at Pilestredet Campus in downtown Oslo and at Kjeller
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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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the Team, and from those outcomes, run dynamical evolution models (N-body) to investigate the occurrences of subsequent collisions, using a surrogate model for giant impacts trained on SPH simulations