Table 13: (Continued) Preliminary set of O II lines selected for the analysis, divided by multiplets. The spectrum of the low v sin i star $\tau$ Sco was used to identify the lines. The log gf values are from the NIST database.
Label $\lambda$ ( Å) log gf Notes

2s² 2p² (1D) 3s-2s² 2p² (1D) 3p

NIST 99 (2D-2F₀)

O II 4590 4590.974 0.350

O II 4596 4595.957 -1.032

4596.177 0.200

2s² 2p² (1D) 3p-2s² 2p² (1D) 3d

NIST 161 (2F₀-2G)

O II 4185 4185.440 0.604 + C III

O II 4189 4189.788 0.716

4189.581 -0.828

NIST 188 (2P₀-2P)

O II 4691 4690.888 -0.610

4691.419 -0.309

O II 4701 4701.179 0.088

4701.712 -0.611

4700.441 -3.298

NIST 172 (2D₀-2F)

O II 4703 4703.161 0.263

**Table 13:** (Continued) Preliminary set of O II lines selected for the analysis, divided by multiplets. The spectrum of the low v sin i star $\tau$ Sco was used to identify the lines. The log gf values are from the NIST database.
Label	$\lambda$ ( Å)	log gf	Notes
2s² 2p² (1D) 3s-2s² 2p² (1D) 3p
		NIST 99 (2D-2F₀)
O II 4590	4590.974	0.350
O II 4596	4595.957	-1.032
	4596.177	0.200
2s² 2p² (1D) 3p-2s² 2p² (1D) 3d
		NIST 161 (2F₀-2G)
O II 4185	4185.440	0.604	+ C III
O II 4189	4189.788	0.716
	4189.581	-0.828
		NIST 188 (2P₀-2P)
O II 4691	4690.888	-0.610
	4691.419	-0.309
O II 4701	4701.179	0.088
	4701.712	-0.611
	4700.441	-3.298
		NIST 172 (2D₀-2F)
O II 4703	4703.161	0.263

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