Topic: astrophysical models

The FICOSS-AI project will develop an open-source pipeline integrating astrophysical models, spectral diagnostics and AI to study stellar populations and galaxy evolution. The fellow will combine machine learning, population-synthesis models and spectral-analysis tools, contribute to publications and mentor students technically. The expected start is 1 February 2027, or earlier if needed. Apply by 2 November 2026 with a CV, publication list and research-interest statement; two recommendation letters must be sent directly by referees as described on the official advertisement.

Observations with instruments including JWST and SKA motivate simulations of the first cosmic structures and the epoch of reionization. This seminar explains why the physics and observability of these early objects strain conventional astrophysical models, and describes the alternative tools and numerical methods being developed to interpret forthcoming data.