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Published online by Cambridge University Press: 25 April 2016
Developments in the measurements of oscillator strengths, that are of current and future interest to astrophysics, have taken place in the past few years:
– there is increased emphasis on methods which are independent of level populations (i.e., of number densities and thus equilibrium in the vapour or plasma under investigation),
– clear progress has been made towards higher precision (and accuracy) and
– the dynamic range of astrophysically relevant oscillator strengths was further extended towards weaker lines.