Table 2: The predicted line strengths in pm for the OH A-X and Be lines using a 3D hydrodynamical solar model atmosphere. The OH lines are computed for log $~\epsilon_{\rm O}=8.66$ and the Be line for log $~\epsilon_{\rm Be}=1.38$ .
line $\chi_{\rm exc}$ log gf $W_\lambda$ $W_\lambda$

[nm] [eV] $\Delta \kappa _\nu ^{\rm cont}/\kappa _\nu ^{\rm cont}$ $\Delta \kappa _\nu ^{\rm cont}/\kappa _\nu ^{\rm cont}$

=0.00 =0.50

OH 312.80 0.102 -2.425 6.38 5.90

OH 312.82 0.209 -2.074 7.42 6.91

OH 313.91 0.760 -1.563 7.29 6.75

OH 316.71 1.108 -1.544 5.87 5.34

Be II 313.10 0.000 -0.468 8.62 7.65

**Table 2:** The predicted line strengths in pm for the OH A-X and Be lines using a 3D hydrodynamical solar model atmosphere. The OH lines are computed for log $~\epsilon_{\rm O}=8.66$ and the Be line for log $~\epsilon_{\rm Be}=1.38$ .
line	$\chi_{\rm exc}$	log gf	$W_\lambda$	$W_\lambda$
[nm]	[eV]		$\Delta \kappa _\nu ^{\rm cont}/\kappa _\nu ^{\rm cont}$	$\Delta \kappa _\nu ^{\rm cont}/\kappa _\nu ^{\rm cont}$
			=0.00	=0.50
OH 312.80	0.102	-2.425	6.38	5.90
OH 312.82	0.209	-2.074	7.42	6.91
OH 313.91	0.760	-1.563	7.29	6.75
OH 316.71	1.108	-1.544	5.87	5.34
Be II 313.10	0.000	-0.468	8.62	7.65

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