\begin{table}%t1
\caption{\label{Tab:Sample}Galaxy sample.}
%\centerline
{{
\begin{tabular}{cccrcclrcllccc}
\hline\hline
  NGC   & $V_{\rm{LG}}$  &    Scale    & Type &  $M_R^{\rm tot}$  &  $M_R^{\rm bul}$  &  $B/D$   &  PA     & Exp. time & \Large{$\epsilon$}\tiny{$_{\rm D}$}  & \Large{$\epsilon$}\tiny{$_{\rm B}$} &     r$_{\rm bulge}$  & Best templ.& {\it S/N}\\
   ~    &      km~s$^{-1}$      & kpc/\arcsec &   ~  &  mag	   &	  mag	      &      ~   &   deg   &   s     &      ~ 		        &	     ~  		&        \arcsec   & ~   	& pix$^{-1}$\\
  (1)   &      (2)       &     (3)     &  (4) &  (5)	   &	  (6)	      &    (7)   &   (8)  &   (9)    &    (10) 		        &	   (11)  		&      (12)        & (13)	&  (14)\\
\noalign{\smallskip}\hline\noalign{\smallskip}
  5326  & 2576  	 & 0.25        &  1   &  $-$22.16  & $-$21.22	      &  0.73	 & --138    & 1500      &  0.50  		        &  0.43  			&  5.97            & $+$0.2, 3.16    	     &  83\\
  5389  & 1990  	 & 0.19        &  0   &  $-$21.32  & $-$20.70	      &  1.30	 &   93    & 1500      &  0.80  		        &  0.46  			&  2.85            & M1 III / $+$0.2, 4.47   &  61\\
  5422  & 1929  	 & 0.19        & $-$2 &  $-$21.96  & $-$21.33	      &  1.28	 &   64    & 1500      &  0.80  		        &  0.35  			&  3.33            & $+$0.2, 7.08    	     &  68\\
  5443  & 2060  	 & 0.20        &  3   &  $-$21.53  & $-$19.09	      &  0.12	 &  --52    & 1400      &  0.68  		        &  0.54  			&  1.98            & $+$0.2, 3.16    	     &  37\\
  5475  & 1861  	 & 0.18        &  0   &  $-$20.98  & $-$18.72	      &  0.14	 & --101    & 1500      &  0.68  		        &  0.24  			&  2.45            & $+$0.2, 1.41    	     &  57\\
  5587  & 2291  	 & 0.22        &  0   &  $-$21.07  & $-$19.43	      &  0.29	 &   73    & 1500      &  0.70  		        &  0.47  			&  1.51            & $-$0.4, 14.12   	     &  36\\
  5689  & 2290  	 & 0.22        &  0   &  $-$22.29  & $-$21.47	      &  0.89	 &   --5    & 1500      &  0.75  		        &  0.48  			&  2.04            & 0.0, 4.47       	     &  58\\
  5707  & 2354  	 & 0.23        &  2   &  $-$21.43  & $-$20.11	      &  0.42	 &  --59    & 1500      &  0.75  		        &  0.20  			&  3.79            & 0.0, 2.51      	     &  51\\
  5719  & 1684  	 & 0.16        &  2   &  $-$21.60  & $-$20.00	      &  0.30	 &   5     & 1500      &  0.64  		        &  0.61  			&  7.71            & K3 Ib / $-$0.4, 3.55    &  51\\
  5746  & 1677  	 & 0.16        &  3   &  $-$22.68  & $-$21.70	      &  0.68	 &  --99    & 1200      &  0.84  		        &  0.52  			&  2.37            & M1 III / $+$0.2, 3.16   &  44\\
  5838  & 1337  	 & 0.13        & $-$3 &  $-$21.89  & $-$20.93	      &  0.71	 &  134    & 1500      &  0.65  		        &  0.22  			&  8.39            & 0.0, 12.59      	     &  86\\
  5854  & 1708  	 & 0.17        & $-$1 &  $-$21.43  & $-$20.18	      &  0.46	 &  --33    & 1500      &  0.70  		        &  0.32  			&  4.85            & $-$0.7, 6.31    	     &  64\\
  5879  & 1065  	 & 0.10        &  4   &  $-$20.30  & $-$19.08	      &  0.48	 &   89    & 1500      &  0.62  		        &  0.32  			&  0.85            & $-$0.4, 3.16    	     &  41\\
  5965  & 3603  	 & 0.35        &  3   &  $-$22.92  & $-$21.76	      &  0.53	 &  --38    & 1500      &  0.84  		        &  0.50  			&  2.32            & $-$0.4, 5.01    	     &  46\\
  6010  & 1923  	 & 0.19        &  0   &  $-$21.57  & $-$19.88	      &  0.27	 &   12    & 1500      &  0.75  		        &  0.28  			&  2.70            & 0.0, 14.12      	     &  67\\
  6504  & 4680  	 & 0.46        &  2   &  $-$24.57  & $-$23.30	      &  0.45	 &  135    & 1500      &  0.83  		        &  0.44  			&  4.05            & $-$0.4, 3.16    	     &  52\\
  7331  & 1138  	 & 0.11        &  3   &  ---	   & ---	      & 0.001$^1$&   80    & 1500      &  0.63$^1$		        &  0.62  			&  4.57            & $-$0.4, 15.85   	     & 117\\
  7332  & 1550  	 & 0.15        & $-$2 &  $-$21.86  & $-$20.52	      &  0.41	 & --114    & 1500      &  0.74  		        &  0.29  			&  2.99            & $-$0.4, 11.22   	     & 101\\
  7457  & 1114  	 & 0.11        & $-$3 &  $-$20.91  & $-$20.91	      & 10.00	 &  35     & 1500      &  0.48  		        &  0.34  			&  3.29            & $+$0.2, 2.51    	     &  51\\
\hline
\end{tabular}}}
\smallskip
{\bf Notes:} Description of the columns:\\
(1): The NGC numbers of the galaxies.\\
(2): Recession velocity of each galaxy in km~s$^{-1}$, corrected to the Local Group 
\citep{kk96}, from optical heliocentric velocities given in the {\it Third Reference 
Catalogue of Bright Galaxies} \citeyearpar{RC3} (hereafter RC3).
 (3): Scale in kpc/arcsec from \citet{fpb02}.\\
 (4): Type index $T$ from the RC3.\\
 (5) and (6): Absolute magnitudes, in $R$-band, from \citet{pb97} ($H_0=50$~km~s$^{-1}$~Mpc$^{-1}$).\\
(7): Bulge-to-disk ratio from an $R$-band bulge-disk decomposition 
           following Kent's \citeyearpar{Kent84} method \citep{pb97}.\\
(8): The position angle, in degrees, (N -- E) of the dust-free minor axis \citep{pb97}.\\
(9): Integration time, in sec, for each galaxy during the observations.\\
(10): Disk ellipticity from \citet{pb97}.\\
  (11): Effective bulge ellipticity, from HST $H$-band ellipticity profiles, measured 
at the geometric effective radius \citep{balcells03}.\\
 (12): Minor axis bulge radius, derived from \citet{balcells03} HST $H$-band profiles,
as the radius at which the contribution from the disk and bulge light are equal, except for
NGC~7332 for which a ground-based image was used instead \citep{pb97} (Alister W. Graham, private
communication).\\
 (13): Best template fit for each galaxy. The metallicity ([m/H]) and age
(Gyr) of the best fit SSP~models is shown. In those cases where the stellar 
template performed better, the adopted SSP best template is also given. \\
  (14): Signal-to-noise ratio per pixel in the central aperture ($1.2 \times 0.36$~arcsec$^2$).\\
$^1$ From \citet{prada96}.
\end{table}