\begin{table}%t1
\caption{\label{targets}Overview of the 37 targets discussed in this paper. 
For each object, we give: the HD number (1), the \hipparcos\ number (2), the Johnson $V$ magnitude (3) and the spectral classification (4) as found in the {\sc simbad} astronomical database; the number of \coralie\ spectra~(5) and their total time span expressed in days (6);  the main \hipparcos\ period in days (7); the orbital classification (8); an indication of the observation of cross-correlation profile variations (9); the variability classification (10); and the mean \vsini\ values obtained by least-square fitting with synthetic profiles for the primary (11) and secondary (12) components. 
The errors are given between brackets in units of the last decimal.
The targets that are in common with those of the Eyer et al. sample (in preparation) are indicated by $\ast$ in Col.~(1). 
The stars that were already classified as confirmed or suspected binaries are indicated by $^+$ in Col.~(8).
The stars already classified as bf \gdor\ stars are indicated by $\degree$ in Col.~(10). 
}
%\begin{center}
{\begin{tabular}{llclrrlllllcc} \hline \hline 
HD        & HIP     & $m_V$ & $SpT$    & $\#$ & \multicolumn{1}{c}{$\Delta T$} & \multicolumn{1}{c}{\phipp} && binarity & CPVs & variability  &\multicolumn{2}{c}{$v\sin i$} \\ %\multicolumn{1}{c}{$\Delta\nu$} &
&& \multicolumn{1}{c}{\tiny(mag)} &&& \multicolumn{1}{c}{\tiny(days)} & \multicolumn{1}{c}{\tiny(days)} &&&&& \multicolumn{2}{c}{\tiny(\kms)}  \\ %\multicolumn{1}{c}{\tiny(\cd)} &      
\multicolumn{1}{c}{(1)}&\multicolumn{1}{c}{(2)}&(3)&\multicolumn{1}{l}{(4)}&(5)&\multicolumn{1}{c}{(6)}&\multicolumn{1}{c}{(7)}&&(8)&(9)&(10) & \multicolumn{1}{c}{(11)} & \multicolumn{1}{c}{(12)} \\  \hline 
  5590      &   4481  &  9.21 & F2~V    &  16  &  1355      &          &            & SB2    &     & constant                  & 103(3)   & 3.4(0.3) \\%  0.0003 &
  7455      &   5745  &  8.47 & G3~V    &  19  &  1723      &          &            &        & no  & constant                  &   3.3(3) &          \\%  0.0002 &
  8393      &   6387  &  9.49 & F7w      &  14  &  1136      &          &            & SB2    &     & constant                  &   4.1(3) &   3.7(2) \\%  0.0003 &
 10167$\ast$&   7649  &  6.67 & F0~V    &  15  &  1721      &          &            & SB2$^+$&     & cand \gdor                &   4.5(5) &   4.9(6) \\%  0.0002 & 
 12901$\ast$&   9807  &  6.74 & F0       &  50  &  1721      & 2.18:    &{\tiny [2]} &        & yes & bf \gdor$\degree$         &  64(3)   &          \\%  0.0004 &
 14940$\ast$&  11192  &  6.68 & F0~IV/V &  63  &   685      & 0.50038  &{\tiny [1]} &        & yes & bf \gdor                  &  39(4)   &          \\%  0.02   & 
 22001      &  16245  &  4.71 & F5~IV/V &  18  &  1719      &          &            &        & no  & constant                  &  12(2)   &          \\%  0.0003 &
 26298$\ast$&  19383  &  8.16 & F0/F2~V &   9  &   332      &          &            & SB1?   &     & cand \gdor?               &  50.9(5) &          \\%  0.0010 &
 27290      &  19893  &  4.26 & F4~III  &  19  &  1395      & 0.757031 &{\tiny [1]} &        & yes & bf \gdor$\degree$(/\dsct?)&  55(2)   &          \\%  0.0003 &
 27377$\ast$&  20036  &  7.4  & F0~V    &   3  &    13      & 2.8482   &{\tiny [3]} & SB2    &     & cand \gdor?               &   5.5(4) &   5.2(6) \\%  0.03   & 
 27604      &  20109  &  6.08 & F7~IV/V &   3  &     6      &          &            & VB?    &     & constant                  &  67.5(4) &   4.3(3) \\%  0.07   & 
 33262      &  23693  &  4.71 & F7~V    &  19  &  1722      & 0.28603  &{\tiny [3]} &        & no  & constant                  &  10.1(10)&          \\%  0.0003 &
 34025$\ast$&  24215  &  7.87 & F2~IV   &   8  &   302      & 0.62221  &{\tiny [1]} & SB2    & yes & bf \gdor                  &  62.8(11)&  39(2)   \\%  0.0012 & 
 35416$\ast$&  25183  &  7.53 & F3~V    &  11  &   625      &          &            & SB2    &     & cand \gdor?               &  6.6(?)  &  6.0(?)  \\%  0.0014 & 
 40745$\ast$&  28434  &  6.21 & F2~IV   &   8  &   334      & 0.82415  &{\tiny [1]} &        & yes & bf \gdor                  &  39(2)   &          \\%  0.0011 & 
 41448$\ast$&  28778  &  7.60 & A9~V    &  12  &    10      & 0.419912 &{\tiny [1]} &        & yes & bf \gdor                  & 106(3)   &          \\%  0.05   & 
 48501$\ast$&  32144  &  6.26 & F2~V    &  34  &  1493      &          &            &        & yes & bf \gdor$\degree$         &  44(4)   &          \\%  0.0003 &
 65526$\ast$&  39017  &  6.98 & A3       &   2  &     1      & 1.28798  &{\tiny [1]} &        & yes & bf \gdor$\degree$         &  56(4)   &          \\%  0.3    &
 81421$\ast$&  46223  &  7.01 & A3       &  63  &   384      & 0.489724 &{\tiny [1]} & SB2$^+$&     & constant                  &  62.0(4) &  42(4)   \\%  0.03   & 
 85964$\ast$&  48580  &  7.52 & F3~IV/V &  11  &   381      & 0.62425  &{\tiny [1]} & SB1    &     & constant                  &  65(2)   &          \\%  0.0012 & 
110379      &         &  3.65 & F0~V    &   8  &    15      &          &            &        &     & cand \gdor                &  23.9(6) &          \\%  0.03   & 
110606$\ast$&  62105  &  7.8  & F2~V    &   7  &    75      & 0.977    &{\tiny [2]} & SB2$^+$&     & cand \gdor                &   5.8(4) &  10(2)   \\%  0.005  & 
111709$\ast$&  62774  &  9.27 & A3:m...  &   5  &    78      & 1.18567  &{\tiny [1]} & SB2    & yes & cand \gdor/CP star?       &  61(1)   &  25(4)   \\%  0.005  & 
111829$\ast$&         &  9.49 & A1~IV/V &   2  &     0      &          &            & SB2?   &     & cand \gdor?               &  47(2)   &   ?      \\%         & 
112685$\ast$&  63372  &  7.85 & F0~V    &  24  &   385      & 0.61645  &{\tiny [1]} &        & yes & bf \gdor                  &  70(3)   &          \\%  0.004  & 
112934$\ast$&  63491  &  6.6  & A9~V    &   5  &    79      & 0.8:     &{\tiny [2]} &        &     & cand \gdor                &  70.5(7) &          \\%  0.005  & 
125081$\ast$&  69848  &  7.35 & F2~II   &   7  &    77      & 0.153981 &{\tiny [1]} &        & yes & bf \dsct                  &   5.6(5) &          \\%  0.005  & 
126516$\ast$&  70566  &  8.2  & F3~V    &   9  &    76      & 0.493    &{\tiny [2]} & SB1$^+$&     & cand \gdor                &   3.8(3) &          \\%  0.02   & 
135825$\ast$&  74825  &  7.31 & F0       &  17  &   450      & 0.76053  &{\tiny [1]} &        & yes & bf \gdor                  &  38(5)   &          \\%  0.0009 & 
147787$\ast$&  80645  &  5.28 & F4~IV   &  10  &   377      & 1.45557  &{\tiny [1]} & SB2$^+$&     & cand \gdor                &  7.6(?)  & 25(?)    \\%  0.0010 & 
149989$\ast$&  81650  &  6.30 & A9~V    &  10  &   379      & 0.42658  &{\tiny [1]} &        & yes & bf \gdor                  & 134(3)   &          \\%  0.0012 & 
167858$\ast$&  89601  &  6.62 & F2~V    &   7  &     3      & 1.30700  &{\tiny [1]} & SB1$^+$&     & bf \gdor$\degree$         &   5.0(2) &          \\%  0.16   &
187028$\ast$&  97590  &  7.60 & F0~V    &  21  &   179      & 0.69532  &{\tiny [1]} &        & yes & bf \gdor                  &  85(3)   &          \\%  0.03   & 
209295$\ast$& 108976  &  7.5  & A9/F0~V &  61  &  1399      & 0.885274 &{\tiny [1]} & SB1$^+$& yes & bf \gdor/\dsct$\degree$   &  86(3)   &          \\%  0.0012 &
214291      & 111718  &  6.54 & F7~V    &   5  &  1329      & 0.87125  &{\tiny [1]} & SB2$^+$&     & cand \gdor?               &  67.6(8) &  64.7(7) \\%  0.0005 & 
216910$\ast$& 113402  &  6.70 & F2~IV   &  11  &  1718      & 0.69349  &{\tiny [1]} &        & yes & bf \gdor                  &  92(3)   &          \\%  0.0002 & 
218225$\ast$& 114127  &  8.72 & F3~IV   &  14  &  1327      & 0.86679  &{\tiny [1]} &        & yes & bf \gdor                  &  59(3)   &          \\%  0.007  & 
 \hline
\end{tabular}}
\parbox{17cm}{
{[1] \citet{ESA1997}; [2] \citet{Handler1999MNRAS.309L..19H}; [3] \citet{Koen2002MNRAS.331...45K}}.}
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\end{table}