Carbon and oxygen abundances in stellar populations

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Volume 568 (August 2014)

A&A, 568 (2014) A25

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Table 1

Line data and derived solar abundances.

ID	Wavelength	χ_exc	log(gf)	E W_⊙	A(X)_⊙ ^a	A(X)_⊙
	(Å)	(eV)		(mÅ)	LTE	non-LTE


C i	5052.17	7.685	−1.301	35.9	8.44	8.43
C i	5380.34	7.685	−1.616	21.5	8.44	8.43
[O i]	6300.31	0.000	−9.720	3.7^b	8.68
O i	7771.94	9.146	0.369	71.8	8.88	8.66
O i	7774.17	9.146	0.223	61.8	8.86	8.66
O i	7775.39	9.146	0.002	48.6	8.84	8.67
Fe ii	5414.08	3.22	−3.580	28.1	7.47
Fe ii	5425.26	3.20	−3.220	42.0	7.43
Fe ii	5991.38	3.15	−3.540	31.2	7.43
Fe ii	6084.11	3.20	−3.790	21.0	7.45
Fe ii	6113.33	3.22	−4.140	11.6	7.47
Fe ii	6149.25	3.89	−2.690	36.3	7.40
Fe ii	6238.39	3.89	−2.600	44.3	7.51
Fe ii	6239.95	3.89	−3.410	12.7	7.41
Fe ii	6247.56	3.89	−2.300	52.7	7.40
Fe ii	6369.46	2.89	−4.110	19.8	7.43
Fe ii	6432.68	2.89	−3.570	41.3	7.45
Fe ii	6456.39	3.90	−2.050	63.2	7.39

Notes.

^(a)

For an element X, A(X) ≡ log (N_X/N_H) + 12.0.

^(b)

This value refers to the EW of the [O i] line after correction for the Ni i contribution to the [O i]–Ni iλ6300 blend. The total EW of the blend is 5.4 mÅ.

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