**Table 1:** Fundamental parameters of the program stars.
HD	JD-2 450 000	$T_{\rm eff}$	$\log g$	$v_{\rm e}\sin i$	$\langle B_{\rm s}\rangle$	$B_{\rm r}/B_{\rm a}$	Reference
number		(K)		(km s^-1)	(kG)
Magnetic chemically peculiar stars
965	2190.632-2190.646	7500	4.00	3.0	4.4	3.2/3.2	RKP
24712^*	1982.545-1982.561	7250	4.30	5.6	2.3	2.3/0.0	RLG97
29578	2213.805-2213.819	7800	4.20	2.5	5.6	4.5/3.4	RNW04
47103	2286.690-2286.719	8180	3.50	0.0	16.3	0.0/16.3	RKP
66318	2413.467-2413.477	9200	4.25	0.0	15.5	10.2/11.7	BLL03
75445	2236.837-2236.846	7650	4.00	3.0	3.0	2.8/1.0	RNW04
101065^*	2280.849-2280.863	6600	4.20	3.5	2.3	2.3/0.0	CRK00
111133	2294.861-2294.866	9930	3.65	5.0	4.0	4.0/0.0	RKP
116114^*	2296.864-2296.871	8000	4.10	2.5	6.2	4.6/3.9	RNW04
118022	2298.861-2298.865	9500	4.00	10.0	3.0	3.0/0.0	RKP
122970^*	2295.862-2295.875	6930	4.10	5.5	2.5	2.5/0.0	RSH00
128898^*	2320.870-2320.873	7900	4.20	12.5	1.5	1.5/0.0	KRW96
133792	2331.791-2331.797	9400	3.70	0.0	1.1	1.1/0.0	KTR06
134214^*	2331.816-2331.826	7315	4.45	2.0	3.1	2.5/1.7	RKP
137909^*	2331.892-2331.895	8000	4.30	2.5	5.4	5.0/2.0	RNW04
137949^*	2331.803-2331.810	7550	4.30	1.0	5.0	2.2/4.5	RNW04
144897	2331.834-2331.851	11 250	3.70	3.0	8.8	6.3/6.2	RRK06
166473^*	2189.508-2189.517	7700	4.20	0.0	8.6	5.0/7.0	GRW00
170973	2190.511-2190.518	10 750	3.50	8.0	0.0		K03
176232^*	2190.522-2190.528	7650	4.00	2.0	1.5	1.5/0.0	RSH00
188041	2190.599-2190.605	8800	4.00	0.0	3.6	3.4/1.0	RLK04
203932^*	2189.540-2189.557	7550	4.34	5.3	$\le$ 1		GKW97
217522^*	2189.567-2189.577	6750	4.30	2.5	$\le$ 1.5	1.5/0.0	G98
Comparison stars
27411	2501.937-2501.946	7650	4.00	18.5	0.0		RKP
61421	2555.906-2555.909	6510	3.96	3.5	0.0		AAG02
73666	3745.063-3745.082	9382	3.78	10.0	0.0		FBM07

The columns give the target HD number, range of Julian dates of its observation with UVES, effective temperature, surface gravity, projected rotational velocity, estimate of the mean magnetic field modulus and the ratio of radial to azimuthal field strength adopted in spectrum synthesis. Rapidly oscillating Ap (roAp) stars are identified by asterisk.

References. RKP - this paper; RLG97 - Ryabchikova et al. (1997); RNW04 - Ryabchikova et al. (2004b); BLL03 - Bagnulo et al. (2003b); CRK00 - Cowley et al. (2000); RSH00 - Ryabchikova et al. (2000); KRW96 - Kupka et al. (1996); KTR06 - Kochukhov et al. (2006a); RRK06 - Ryabchikova et al. (2006); GRW00 - Gelbmann et al. (2000); K03 - Kato (2003); RLK04 - Ryabchikova et al. (2004a); GKW97 - Gelbmann et al. (1997); G98 - Gelbmann (1998); AAG02 - Allende Prieto et al. (2002); FBM07 - Fossati et al. (2007).