MCDHF calculations with tested correlation models deliver a benchmark E1 line strength for the specified transition in C III with uncertainty estimated from model differences.
Chang, The Astrophysical Journal 211, 300 (1977)
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High-precision calculations of the $1s^{2} 2s 2p$ $^1P_{1} \to 1s^{2} 2s^{2}$ $^1S_{0}$ spin-allowed $E1$ transition in C {\small III}
MCDHF calculations with tested correlation models deliver a benchmark E1 line strength for the specified transition in C III with uncertainty estimated from model differences.