Table 5:

Stellar parameters of the 18 Sun-like stars.

Object			[Fe/H]	[Mg/Fe]				ref.	M	R	B.C.V
	[K]	[cm/s2]			[km s-1]	[km s-1]	[km s-1]		[]	[]			[pc]	[%]
M01k
HD 11131	5796	4.43	-0.10	0.00	0.97	3.70	1.5	2	1.00	1.01	-0.13	4.73	23.8	0.6
	70	0.10	0.07	0.05	0.20		1.0		0.05	0.04		0.07	3.3
HD 24916 A	4600	4.60	-0.03	-	-	-	2.1	3	0.70	0.69	-0.57	6.48	15.4	-2.4
	100	0.20	0.15	-	-		2.0		0.05	0.03		0.09	3.7
HD 26923	5975	4.41	-0.06	-0.01	0.99	4.40	<1.0	2	1.07	1.01	-0.11	4.57	22.4	5.5
	70	0.10	0.07	0.05	0.20		-		0.05	0.04		0.07	3.0
HD 38393	6310	4.281	-0.05	0.01	1.30	5.70	8.1	1	1.23	1.33	-0.08	3.74	-	-
	60	0.03	0.05	0.06	0.20		1.0		0.05	0.04		0.05	-
HD 41593	5278	4.54	0.02	-0.01	1.12	1.70	4.3	2	0.89	0.82	-0.24	5.57	15.8	2.5
	80	0.10	0.07	0.05	0.20		1.0		0.05	0.03		0.06	2.2
HD 112196	6110	4.391	0.01	0.02	1.31	4.90	12.0	1	1.15	1.14	-0.09	4.22	-	-
	60	0.06	0.05	0.05	0.20		1.0		0.05	0.08		0.14	-
HD 167389	5895	4.37	-0.02	-0.03	0.99	4.00	3.3	1	1.05	1.01	-0.12	4.64	36.8	10.0
	80	0.15	0.07	0.05	0.20		1.0		0.05	0.04		0.07	6.5
HD 184960	6310	4.22	-0.08	-0.01	1.55	5.70	8.0	1	1.23	1.43	-0.08	3.59	25.6	0.0
	80	0.10	0.05	0.05	0.20		1.0		0.05	0.05		0.06	3.1
M01k, K03k, K03f
HD 59747	5094	4.55	-0.03	-0.01	1.00	0.90	1.5	2	0.83	0.76	-0.31	5.90	20.8	5.8
	90	0.10	0.07	0.05	0.20		1.0		0.05	0.04		0.08	2.9
HD 109647	4980	4.70	0.05	-0.07	0.80	0.40	3.1	1	0.83	0.74	-0.36	6.05	24.0	-8.8
	60	0.15	0.15	0.15	0.20		1.0		0.05	0.03		0.08	4.3
HD 110463	4940	4.68	0.00	-0.02	0.86	0.40	3.1	1	0.80	0.75	-0.38	6.05	20.9	-9.8
	80	0.18	0.10	0.10	0.20		1.0		0.05	0.03		0.07	4.5
HD 115043	5850	4.36	-0.10	0.05	1.26	3.90	7.5	1	1.05	1.03	-0.13	4.64	28.3	9.3
	70	0.13	0.07	0.05	0.20		1.0		0.05	0.04		0.06	4.4
K03k, K03f
HD 28495	5465	4.45	-0.05	0.00	0.93	2.34	4.5	1	0.95	0.85	-0.19	5.35	31.3	13.8
	90	0.12	0.05	0.05	0.20		1.0		0.10	0.04		0.08	4.8
HD 39587	5920	4.39	-0.07	-0.01	0.95	4.20	8.7	2	1.04	1.03	-0.12	4.59	9.1	5.3
	70	0.10	0.07	0.05	0.20		0.8		0.05	0.04		0.05	1.3
HD 71974 A2	5570	4.49	-	-	-	2.8	3.2	1	-	-	-	-	-	-
	100	0.19	-	-	-		1.0		-	-		-	-
HD 109011	5000	4.60	-0.12	-0.03	0.52	0.50	5.0	1	0.83	0.81	-0.34	5.85	22.3	-6.0
	100	0.20	0.07	0.07	-		1.0		0.05	0.07		0.17	5.3
HD 171746 A	6100	4.361	-0.04	0.03	1.50	4.80	8.3	1	1.15	1.18	-0.10	4.16	-	-
	80	0.06	0.06	0.05	0.20		1.0		0.05	0.08		0.14	-
HD 171746 B	6040	4.371	0.02	-0.04	1.51	4.60	7.3	1	1.10	1.16	-0.10	4.24	-	-
	80	0.06	0.05	0.05	0.20		1.0		0.05	0.08		0.14	-

The stellar parameters of the sample stars which were studied following the methods of Fuhrmann (1998). The stars are grouped according to the samples they form part of (Table 3). The following quantities are listed with the second line providing the errors bars: (2) effective temperature, (3) surface gravity, (4) iron abundance, (5) magnesium abundance relative to iron, (6) microturbulence parameter, (7) macroturbulence parameter, (8) projected rotational velocity, (9) source of the values: 1 = this work, 2 = Fuhrmann04, 3 = König et al. (2006), (10) mass, (11) radius, (12) bolometric correction based on Alonso et al. (1995), (13) absolute bolometric magnitude (from Hipparcos distance), (14) spectroscopic distance, and (15) relative offset from Hipparcos distance.
¹ Surface gravity derived from Hipparcos parallax as described in Sect. 3.1.4. The comparison of spectroscopic distance with Hipparcos distance cannot be done.
² The stellar parameters are preliminary because HD 71974 is a spectroscopically unresolved binary (see discussion of individual objects in Sect. 3.3). Abundances could not be derived.