\begin{table}%t1
\caption{The galaxy sample.} \label{tgalaxies}
%\centerline
{\begin{tabular}{llrrccccrrrrr} \hline \hline
 & Type  &  \multicolumn{1}{c}{$T$}  & \multicolumn{1}{c}{$B_{\rm T}$} &  $i$
& Bulge type$^{a}$ & Environment & Run$^{b}$ &  PA$^{c}$ & \multicolumn{1}{c}{Exp.$^{d}$} &
\multicolumn{1}{c}{$r_{\rm eff}^{e}$} &
\multicolumn{1}{c}{$\Delta r_{\rm eff}$} &
\multicolumn{1}{c}{$V_{\rm max}^{f}$} \\
\hline
NGC  522     &  Sc &   4.1 &    13.98   &  90& box         &             &2    &  123 &   8200 &3.5&0.7&196.1\\
NGC  585     &  Sa  &   1.0 &    14.06   &  90& close to box&             &4,5  &   86 &   7200 &2.4&0.7&246.6\\
NGC  678     &  SBb &   3.0 &    13.31   &  90& box         & cluster     &1    &  168 &  12~000 &23.3&1.4&169.0\\
NGC  891     &  SAb  &   3.0 &    10.83   &  88& box         &             &1    &  112 &  10~500 &13.2&0.7&212.0\\
NGC  973     &  Sbc  &   3.2 &    14.17   &  90& box         &             &2    &  138 &  13~800 &3.4&0.4&270.0\\
NGC 1032     &  S0-a&   0.4 &    12.74   &  90& elliptical  & companions? &1    &  158 &   9000 &11.4&1.1&283.9\\
NGC 1184     &  S0-a&   0.0 &    12.95   &  90& close to box&             &2    &   79 &   8200 &11.3&1.9&\\
NGC 1351A    &  SBbc&   4.5 &    14.16   &  80& elliptical   & cluster     &5    &  132 &   5400 &5.8&0.8&90.7\\
NGC 1886     &  Sab &   3.9 &    13.80   &  90& peanut      & isolated    &3    &   60 &  10~800 &1.6&0.3&154.6\\
NGC 3957     &  SA0 &  $-1.0$ &  13.03   &  90& close to box& cluster     &3    &  173 &   7200 &4.0&0.8& \\
NGC 5084     &  S0  &  $-1.8$ &  11.55   &  90& elliptical  & cluster     &3    &   80 &   7200 &38.1&11.6&310.3\\
NGC 6010     &  S0-a&   0.4 &    12.95   &  90&             &             &1    &   15 &  13~800 &4.2&0.9&148.8\\
NGC 6829     &  Sb  &   3.0 &    15.09   &  90&             &             &2    &  121 &  12~800 &7.1&1.4&211.9\\
NGC 7183     &  S0 &  $-0.7$ &  13.14   &  90& close to box&             &5    &   77 &   7200 &2.5&0.5&209.9\\
NGC 7264     &  Sb  &   3.1 &    14.58   &  90& elliptical  &             &2    &  147 &  13~000 &1.2&0.4&248.0\\
NGC 7332     &  S0  &  $-2.0$ &  12.56   &  90& close to box&             &1    &   65 &  15~000 &7.5&1.1&121.3\\
NGC 7396     &  Sa  &   1.0 &    13.85   &  60& elliptical  &             &2    &   13 &  13~000 &25.2&1.6&360.7\\
NGC 7703     &  S0  &  $-2.0$ &  14.41   &  90& elliptical  & cluster     &2    &   57 &   6400 &4.8&2.0&159.5\\
NGC 7814     &  SAab &   2.0 &    11.68   &  67& elliptical  &             &1    &   45 &  18~400 &33.5&2.0&231.0\\
IC 1711      &  Sb  &   3.0 &    14.53   &  90& elliptical  &             &2    &  133 &   6200 &2.1&0.5&173.4\\
IC 1970      &  SAb  &   3.1 &    13.36   &  88& elliptical  &             &4    &   75 &   7200 &8.1&1.0&118.9\\
IC 2531      &  Sb  &   4.9 &    12.88   &  90& peanut      & cluster     &3    &   75 &   7200 &2.3&0.3&228.1\\
IC 5176      &  SABbc&   4.4 &    13.02   &  90& elliptical  & companions? &5    &  151 &   7200 &4.6&0.3&164.2\\
IC 5264      &  Sab &   2.3 &    13.58   &  90& elliptical  & group       &4,5  &   82 &  12~600 &2.8&0.1&230.6\\
UGC 10043    &  Sbc &   4.1 &    15.17   &  90&             & cluster     &2    &   61 &  12~200 &1.0&0.3&143.6\\
UGC 11552    &  Sab &   2.0 &    15.68   &  75&             &             &5    &   16 &   7200 &11.7&0.6&243.0\\
UGC 11587    &  S0  &  $-1.9$ &  14.52   &  90&             &             &1    &   76 &  15~000 &5.7&0.7& \\
ESO 079-003  &  SBb &   3.1 &    13.91   &  90& close to box&             &4,5  &  134 &  10~800 &5.9&2.0&192.2\\
ESO 234-053  &  S0  &  $-1.9$ &  14.32   &  90&             &             &5    &   81 &   5400 &1.7&0.1& \\
ESO 311-012  &  S0-a&   0.1 &    12.38   &  90& box         & isolated    &3    &   14 &   7200 &7.4&1.3&95.9\\
ESO 443-042  &  Sb  &   3.1 &    13.85   &  90& peanut      & companions? &3    &  130 &  10~800 &3.8&0.7&166.3\\
ESO 512-012  &  Sbc  &   3.2 &    14.42   &  90& peanut      &             &3    &  113 &   5400 &1.4&0.3&224.9\\
\hline
\end{tabular}}
\medskip
\par
$^{a}$ From L\"utticke et~al.\ (2000).
$^{b}$ Run number in which each galaxy was observed.
$^{c}$ Position angle of the long slit.
$^{d}$ Total exposure time (in seconds).
$^{e}$ Effective radius (in arcseconds) of the bulge,
computed as explained in Sect.~\ref{s:reduction}.
$^{f}$ Maximum rotational velocity (in km s$^{-1}$) along the disk major axis, corrected from inclination when necessary.
Hubble type $T$, total apparent magnitude $B_{\rm T}$,
galaxy inclination $i$ and $V_{\rm max}$ have been taken from
HyperLeda ({\tt http://leda.univ-lyon1.fr/}).
\end{table}