Comparative modelling of the spectra of cool giants

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Table 9

Lines used by the A2 participants (Sect. 3.2.2).

Ion	λ	log (gf)	Source	EW Star 1	EW star 2	Ion	λ	log (gf)	Source	EW star 1	EW star 2
	(nm)			(mA)	(mA)		(nm)			(mA)	(mA)

26.00^⋆	490.514	–2.050	FMW	73.63	30.33	26.00	536.162	–1.430	FMW	269.68	225.63
26.01	492.393	–1.320	FMW	–	–	26.00^⋆	537.371	–0.860	FMW	82.82	97.37
26.00	492.477	–2.220	FMW	107.96	183.82	26.00	537.958	–1.480	FMW	102.03	113.47
24.00	493.634	–0.340	MFW	110.10	82.99	26.00	538.634	–1.770	FMW	–	–
26.00^⋆	496.258	–1.290	FMW	52.201	–	26.00^⋆	538.948	–0.410	FMW	20.50	85.97
28.00	501.094	–0.870	FMW	–	–	28.00	539.233	–1.320	FMW	–	4.94
26.00	504.422	–2.150	FMW	169.70	181.76	26.00	612.025	–5.950	FMW	112.24	113.17
26.00	504.982	–1.420	FMW	–	–	26.00^⋆	615.938	–1.970	FMW	26.72	40.58
26.00^⋆	505.465	–2.140	FMW	25.21	25.79	26.00	622.674	–2.220	FMW	23.82	6.31
22.00^⋆	506.406	–0.270	MFW	2.45	2.50	26.01^⋆	636.946	–4.253	K88	–	–
26.00^⋆	508.334	–2.958	FMW	1.16	11.24	26.00^⋆	639.254	–4.030	FMW	64.58	67.31
26.00	509.078	–0.400	FMW	–	4.39	21.01	660.460	–1.480	MFW	142.65	127.39
28.00^⋆	509.441	–1.080	FMW	23.30	22.79	26.00^⋆	672.536	–2.300	FMW	61.93	8.42
26.00^⋆	512.735	–3.307	FMW	72.89	74.44	26.00^⋆	848.198	–1.647	K94	39.32	30.20
26.00^⋆	514.174	–2.150	FMW	73.17	91.99	14.00^⋆	850.222	–1.260	KP	14.75	1.58
26.00^⋆	514.373	–3.790	FMW	27.32	28.61	26.00	851.510	–2.073	O	152.76	132.81
22.00^⋆	514.547	–0.574	MFW	–	–	26.00	858.225	–2.133	O	146.53	141.05
26.00^⋆	515.191	–3.322	FMW	83.65	104.74	26.00^⋆	859.295	–1.083	K94	83.14	81.46
26.00^⋆	515.906	–0.820	FMW	74.80	80.40	14.00^⋆	859.596	–1.040	KP	42.03	38.56
26.00	518.006	–1.260	FMW	–	–	14.00^⋆	859.706	–1.370	KP	60.52	47.79
26.00^⋆	518.791	–1.260	FMW	56.57	37.12	26.00^⋆	859.882	–1.088	O	71.36	59.76
26.00	519.495	–2.090	FMW	73.31	113.68	26.00^⋆	860.707	–1.463	K94	48.49	49.34
26.00^⋆	519.547	0.018	K94	85.83	21.61	26.00	861.180	–1.900	FMW	217.20	226.04
22.01	521.154	–1.356	K88	–	–	26.00	862.160	–2.321	O	128.62	135.64
22.00^⋆	521.970	–2.292	MFW	174.09	173.95	26.00^⋆	867.474	–1.850	FMW	46.99	25.25
26.00	522.985	–0.241	K94	–	26.94	14.00	868.635	–1.200	KP	–	4.67
26.01	523.463	–2.050	FMW	–	–	26.00	868.862	–1.212	FMW	351.04	340.18
26.00	524.250	–0.840	FMW	114.71	172.90	26.00^⋆	869.870	–3.433	K94	86.81	87.78
26.01^⋆	525.693	–4.250	K88	57.75	–	26.00^⋆	869.945	–0.380	O	77.67	69.31
26.00	526.331	–0.970	FMW	129.66	135.07	26.00^⋆	871.039	–0.555	K94	87.34	86.76
24.00^⋆	528.718	–0.907	MFW	61.55	19.62	14.00^⋆	872.801	–0.610	KP	24.91	22.03
24.00	529.670	–1.400	MFW	214.13	203.87	26.00^⋆	872.914	–2.951	K94	91.38	96.13
27.00^⋆	535.205	0.060	FMW	62.30	50.28

Notes. For each line, the species code, the wavelength λ and the gf value are given (taken from the line lists of Kurucz). Lines included in the final fit have been marked with the symbol ^⋆. The species code follows Kurucz’s notation, e.g. for iron lines (atomic number 26): 26.00 = Fe I, 26.01 = Fe II, etc. References as listed in Kurucz & Bell (1995)^a. Furthermore, the table gives the measured equivalent widths of the lines in the two benchmark stars. The full table is available at the CDS.

^(a)

http://kurucz.harvard.edu/LINELISTS/LINES/gfall.ref.

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