\begin{table}%t1
\caption{Fundamental parameters of the program stars. }\label{tbl1}
%\centerline
{\small 
\begin{tabular}{rclccccl}
\hline
\hline
HD~~~~  & JD$-$2~450~000 &~~\teff     & \lgg & \vs~~     & \bs & $B_{\rm r}/B_{\rm a}$ & ~~Reference  \\
number~ &              &~~(K)	 &	& (\kms)    & (kG)&		\\
\hline
\multicolumn{7}{c}{\it Magnetic chemically peculiar stars} \\
   965\noap &2190.632--2190.646&~~7500& 4.00 & ~3.0   & 4.4 & 3.2/3.2   &RKP   \\
 24712\roap &1982.545--1982.561&~~7250& 4.30 & ~5.6   & 2.3 & 2.3/0.0   &RLG97 \\  
 29578\noap &2213.805--2213.819&~~7800& 4.20 & ~2.5   & 5.6 & 4.5/3.4   &RNW04 \\  
 47103\noap &2286.690--2286.719&~~8180& 3.50 & ~0.0   &16.3 & 0.0/16.3  &RKP   \\                         
 66318\noap &2413.467--2413.477&~~9200& 4.25 & ~0.0   &15.5 & 10.2/11.7 &BLL03 \\    
 75445\noap &2236.837--2236.846&~~7650& 4.00 & ~3.0   & 3.0 & 2.8/1.0   &RNW04 \\                         
101065\roap &2280.849--2280.863&~~6600& 4.20 & ~3.5   & 2.3 & 2.3/0.0   &CRK00 \\
111133\noap &2294.861--2294.866&~~9930& 3.65 & ~5.0   & 4.0 & 4.0/0.0   &RKP   \\
116114\roap &2296.864--2296.871&~~8000& 4.10 & ~2.5   & 6.2 & 4.6/3.9   &RNW04 \\  
118022\noap &2298.861--2298.865&~~9500& 4.00 & 10.0   & 3.0 & 3.0/0.0   &RKP   \\                        
122970\roap &2295.862--2295.875&~~6930& 4.10 & ~5.5   & 2.5 & 2.5/0.0   &RSH00 \\  
128898\roap &2320.870--2320.873&~~7900& 4.20 & 12.5   & 1.5 & 1.5/0.0   &KRW96 \\        
133792\noap &2331.791--2331.797&~~9400& 3.70 & ~0.0   & 1.1 & 1.1/0.0   &KTR06 \\  
134214\roap &2331.816--2331.826&~~7315& 4.45 & ~2.0   & 3.1 & 2.5/1.7   &RKP   \\                        
137909\roap &2331.892--2331.895&~~8000& 4.30 & ~2.5   & 5.4 & 5.0/2.0   &RNW04 \\  
137949\roap &2331.803--2331.810&~~7550& 4.30 & ~1.0   & 5.0 & 2.2/4.5   &RNW04 \\  
144897\noap &2331.834--2331.851& 11~250& 3.70 & ~3.0   & 8.8 & 6.3/6.2   &RRK06 \\ 
166473\roap &2189.508--2189.517&~~7700& 4.20 & ~0.0   & 8.6 & 5.0/7.0   &GRW00 \\   
170973\noap &2190.511--2190.518& 10~750& 3.50 & ~8.0   & 0.0 &           &K03   \\             
176232\roap &2190.522--2190.528&~~7650& 4.00 & ~2.0   & 1.5 & 1.5/0.0   &RSH00 \\               
188041\noap &2190.599--2190.605&~~8800& 4.00 & ~0.0   & 3.6 & 3.4/1.0   &RLK04 \\ 
203932\roap &2189.540--2189.557&~~7550& 4.34 & ~5.3   &$\le$1&          &GKW97 \\
217522\roap &2189.567--2189.577&~~6750& 4.30 & ~2.5   &$\le$1.5&1.5/0.0 &G98   \\
\multicolumn{7}{c}{\it Comparison stars} \\
 27411\noap &2501.937--2501.946&~~7650& 4.00 & 18.5   & 0.0 & &RKP  \\
 61421\noap &2555.906--2555.909&~~6510& 3.96 & ~3.5   & 0.0 & &AAG02\\
 73666\noap &3745.063--3745.082&~~9382& 3.78 & 10.0   & 0.0 & &FBM07  \\
\hline
\end{tabular}}
 \smallskip
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. 
\par
References. RKP -- this paper; RLG97 -- Ryabchikova et~al. (\cite{RLG97}); 
RNW04 -- Ryabchikova et~al. (\cite{RNW04}); BLL03 -- Bagnulo et~al. (\cite{bagn03});
CRK00 -- Cowley et~al. (\cite{CRK00}); RSH00 -- Ryabchikova et~al. (\cite{RSH00});
KRW96 -- Kupka et~al. (\cite{KRW96}); KTR06 -- Kochukhov et~al. (\cite{KTRM06});
RRK06 -- Ryabchikova et~al. (\cite{RRKB06}); GRW00 -- Gelbmann et~al. (\cite{GRW00});
K03 -- Kato (\cite{Kato03}); RLK04 -- Ryabchikova et~al. (\cite{RLKB04});
GKW97 -- Gelbmann et~al. (\cite{GKWM97}); G98 -- Gelbmann (\cite{G98});
AAG02 -- Allende Prieto et~al. (\cite{Procyon}); FBM07 -- Fossati et~al. (\cite{fossati}).\end{table}