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Table 1

Atomic parameters of the spectral lines together with our measurements of EW and abundance in the Sun.

λ log(gf) χlo Ref. EW logϵ(X)
( Å) (eV) (mÅ)

OI 6158.171 –0.296 10.74 1 3.7 8.71
[OI] 6300.304 –9.717 0.00 1 3.4 8.65
NiI 6300.336 –2.110 4.27 2 2.0 6.25

Notes. This solar value will be used as reference in the present analysis.

Reference. (1) Caffau et al. (2008); (2) Johansson et al. (2003).

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