Curves of growth for transiting exocomets: Application to Fe II lines in the β Pictoris system

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Table A.2

Same parameters for the faint Fe II lines rising from highly excited levels, used in Sect. 5.2.

λ_lu (Å)	E_l (cm⁻¹)	E_l/k_B (K)	A_ul^a (10⁷ s⁻¹)	𝑔l f_lu^a
2424.88	22637	32578	22.1	2.34
2430.82	22810	32827	19.1	1.70
2445.26	20830	29977	27.8	2.00
2446.31	21812	31390	20.7	1.12
2471.42	22810	32827	15.4	0.85
2499.65	21581	31058	21.2	2.39
2512.52	21712	31246	23.0	2.18
2526.15	21251	30583	19.1	2.56
2527.05	20830	29977	24.7	1.42
2530.31	22637	32578	22.0	2.12
2530.32	21812	31390	20.2	0.78
2534.39	21430	30841	19.2	2.22
2535.18	21711	31245	18.3	1.41
2667.43	27620	39748	18.7	1.60
2685.55	30764	44273	15.7	1.70
2693.40	30388	43732	14.0	1.83
2704.79	27314	39308	13.8	1.21
2712.65	25428	36594	4.3	0.68
2717.02	27620	39748	11.5	0.77
2754.10	26352	37923	18.9	2.58
2768.32	26170	37662	15.8	2.55
2780.12	26352	37923	10.0	0.93
2784.51	26170	37662	10.6	1.23
2832.39	25787	37110	7.6	0.55
2841.48	26932	38758	7.6	0.37
2859.18	30388	43732	4.8	0.71

^a Parameters obtained from the NIST database. The uncertainties on A_ul and f_lu are typically of the order of 10 to 15%.

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