Postdoc in modeling of star-disk formation
Role highlights
39,200–39,200 DKK
Full Time
Permanent
Independent
On-site
This postdoctoral position focuses on advanced computational modeling of star and disk formation within the astrophysics domain, specifically targeting the processes involved in young star and planet systems. Candidates must possess a PhD obtained on or after October 10, 2020, demonstrating recent and relevant academic expertise. Core competencies include expertise in computational astrophysics, high-performance computing (HPC), and synthetic observations, with a strong emphasis on comparing simulation outputs to observational data, particularly from (sub)millimeter wavelengths such as ALMA. Experience in handling and interpreting complex observational datasets to validate theoretical models is essential. Additional desirable skills include familiarity with machine learning techniques applicable to astrophysical data analysis and observational astronomy experience, which would complement the modeling efforts. The role involves conducting cutting-edge research funded by a competitive grant, requiring proficiency in scientific programming, numerical simulations, and data analysis within a collaborative academic environment. Teaching opportunities may be available, indicating a potential for academic communication and mentoring skills. The position is embedded in an inclusive, diverse research group at the Niels Bohr Institute, offering exposure to interdisciplinary scientific challenges in star-disk system evolution. Candidates should be prepared to produce high-quality research outputs, including publications and presentations, and contribute to the broader scientific community through innovative computational approaches and synthetic observational methods.
About the role
- Postdoc position in modeling of star-disk formation
- Part of the "Young Stars and Planets" research group at the Niels Bohr Institute
- Funded by the DFF Sapere Aude grant “DSTREAM: Disk Systems That are Replenished and Evolve through Accretion of Material”
- Focus on computational modeling, synthetic observations, and high-performance computing
- Position open from 01/10/2026 (earlier or later start possible)
- Duration: 2 years
Responsibilities
- Conduct research in star and disk formation modeling
- Opportunities for teaching (not mandatory)
Requirements
- PhD degree obtained on or after October 10th, 2020 (leave periods accepted per DFF regulations)
- Expertise in computational modeling of star and disk formation
- Experience with synthetic observations and high-performance computing
- Ability to compare computational results with (sub)mm observational data, especially ALMA
Nice to Have
- Experience with machine-learning techniques
- Observational expertise
Benefits
- Covered by the Memorandum on Job Structure for Academic Staff
- Salary starts at 39,200 DKK/month (approx. 5,200 EUR, November 2025 level)
- Supplement possible depending on qualifications
- Employer pays additional 18.07% to pension fund
- Possible tax reductions for foreign and Danish applicants who have not lived in Denmark in the last 10 years
- Inclusive and diverse work environment
How to Apply
- Application must be in English and submitted electronically
- Include:
- Curriculum vitae (2 pages)
- Diplomas (Master and PhD or equivalent)
- Research plan (~3 pages)
- Complete publication list
- Separate reprints of 3 relevant papers
- Deadline: 15th January 2026, 23:59 GMT +1
- For questions, contact Dr. Michael Küffmeier
- More information: Niels Bohr Institute
- Read about the recruitment process: http://employment.ku.dk/faculty/recruitment-process/
- Please mention in your application that you found the job at Jobindex
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