Improved oscillator strengths and wavelengths for Os I and Ir I, and new results on early r-process nucleosynthesis
The radioactive decay of 238U and 232Th has recently been used to determine ages for some of the oldest stars in the Universe. This has highlighted the need for accurate observational constraints on production models for the heaviest r-process elements which might serve as stable references, notably osmium and iridium. In order to provide a firmer basis for the observed abund
