Fig. B.3
Line-by-line Si I abundances determined for four benchmark stars for two groups of lines with different quality assessment of their transition probabilities, as a function of equivalent width and lower level energy. Abundances are given as log (εSi) + 12, where εSi = NSi∕NH. Only lines with synflag = Y or U and with equivalent widths >5 mÅ are included.
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