Derived solar abundances (log ϵX ⊙), with their corresponding line-to-line scatter error (), and number of lines (N).
|Ion||log ϵX ⊙||Error||N|
|O I (nLTE)||8.79||0.04||3|
|V I (HFS)||3.91||0.03||14|
|Co I (HFS)||4.95||0.03||4|
|Cu I (HFS)||4.29||0.07||2|
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