Oxygen lines in solar granulation - II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance

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Table 4:

Ni I isotopes used and scaled $\log gf$ values.
Ni isotope	%^a	Wavelength [nm]^b	$\log gf$
⁵⁸Ni	68.27	630.0335	-2.2757
⁶⁰Ni	26.10	630.0355	-2.6933
⁶¹Ni	1.13	630.0365	-4.0569
⁶²Ni	3.59	630.0375	-3.5549
⁶⁴Ni	0.91	630.0395	-4.1509

^a Isotopic fractions from Rosman & Taylor (1998). ^b Wavelength of main
component and isotopic splitting from Johansson et al. (2003).

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