\begin{table}%t1
\caption{Basic data and model-free parameters of the early-type dwarfs
considered in this study (extinction-corrected).\label{tab1}}
%\centerline
{\begin{tabular}{llllrlllllllc}
\hline\hline
\multicolumn{1}{l}{VCC} &
\multicolumn{1}{l}{Name} &
\multicolumn{1}{l}{Type} &
\multicolumn{1}{c}{$M_{B_{\rm T}}$} &
\multicolumn{1}{c}{$v_{\odot}$} &
\multicolumn{1}{c}{$B_{\rm T}$} &
\multicolumn{1}{c}{$r_{\rm eff}^B$} &
\multicolumn{1}{c}{$\mu_{\rm eff}^B$} &
\multicolumn{1}{c}{$R_{\rm T}$} &
\multicolumn{1}{c}{$r_{\rm eff}^R$} &
\multicolumn{1}{c}{$\mu_{\rm eff}^R$} &
\multicolumn{1}{c}{$B-R$} &
\multicolumn{1}{c}{Notes} \\
\multicolumn{1}{l}{(1)} &
\multicolumn{1}{l}{(2)} &
\multicolumn{1}{l}{(3)} &
\multicolumn{1}{c}{(4)} &
\multicolumn{1}{c}{(5)} &
\multicolumn{1}{c}{(6)} &
\multicolumn{1}{c}{(7)} &
\multicolumn{1}{c}{(8)} &
\multicolumn{1}{c}{(9)} &
\multicolumn{1}{c}{(10)} &
\multicolumn{1}{c}{(11)} &
\multicolumn{1}{c}{(12)} &
\multicolumn{1}{c}{} \\
\hline
0009 & IC~3019  & dE1,~N        & $-$17.11  & 1804 & 14.04  & 30.81      & 23.48  
&
12.66  & 34.48       & 22.35  & 1.38  & a \\
0490 & IC~0783  & dS0(3),~N     & $-$17.18  & 1293 & 13.97  & 27.31      & 23.15  
&
12.63  & 28.35       & 21.89  & 1.34  & b \\
0781 & IC~3303  & dS0(5),~N:    &         & $-$254 &        &            &        
&
13.56  & 10.30       & 20.62  &       &   \\
0810 &         & dE0,~N        & $-$14.47  & $-$340 & 16.68  & $~$ 9.92  & 23.66 
 &
15.45  & $~$ 9.94   & 22.44  & 1.23  &   \\
0815 &         & dE2, N       & $-$15.20: & $-$700 & 15.95: & 13.54:     & 
23.61: &
14.90: & 12.93:      & 22.46: & 1.05: &   \\
0846 &         & dE1,~N:       & $-$14.96  & $-$730 & 16.19  & 12.35      & 23.65 
 &
14.73  & 15.35       & 22.66  & 1.46  &   \\
0850 &         & dE,~N         & $-$12.63: &      & 18.52: & $~$ 8.81: & 25.24: 
&
17.46: & $~$ 8.27:  & 24.05: & 1.06: & c \\
0856 & IC~3328  & dE1,~N        & $-$16.96  &  972 & 14.19  & 20.66      & 22.76  
&
12.98  & 18.07       & 21.26  & 1.21  & d \\
0928 &         & dE6,~N        & $-$15.02  & $-$254 & 16.13  & $~$ 9.11  & 22.93 
 &
14.98  & $~$ 8.60   & 21.65  & 1.15  &   \\
0929 & NGC~4415 & d:E1,~N       & $-$17.46  &  910 & 13.69  & 19.26      & 22.11  
&
12.18  & 20.72       & 20.76  & 1.51  &   \\
0940 & IC~3349  & dE1,~N        & $-$16.34  & 1563 & 14.81  & 19.42      & 23.25  
&
13.56  & 18.35       & 21.88  & 1.25  & b \\
0962 &         & dE3          & $-$14.18: &      & 16.97: & 22.00:     & 25.68: 
&
15.93: & 17.90:      & 24.19: & 1.04: &   \\
0998 &         & dE4,~N:       & $-$13.21  &      & 17.94  & 11.37      & 25.22  
&
16.75  & 11.11       & 23.98  & 1.19  &   \\
1010 & NGC~4431 & dS0(5),~N     & $-$17.29  &  913 & 13.86  & 17.23      & 22.04  
&
12.47  & 17.05       & 20.63  & 1.39  & b \\
1036 & NGC~4436 & dE6/dS0(6),~N & $-$17.26  & 1163 & 13.89  & 16.37      & 21.96  
&
12.65  & 14.90       & 20.51  & 1.24  &   \\
1087 & IC~3381  & dE3,~N        & $-$17.00  &  645 & 14.15  & 19.35      & 22.58  
&
12.87  & 18.06       & 21.15  & 1.28  &   \\
1093 &         & dE0,~N        & $-$14.22  &      & 16.93  & 12.23      & 24.37  
&
15.45  & 14.34       & 23.23  & 1.48  &   \\
1104 & IC~3388  & dE5,~N        & $-$15.66  & 1704 & 15.49  & 11.76      & 22.84  
&
14.29  & 11.30       & 21.56  & 1.20  & e \\
1129 &         & dE3          & $-$13.26  &      & 17.89  & $~$ 7.56  & 24.28  
&
16.70  & $~$ 7.43   & 23.05  & 1.19  &   \\
1254 &         & dE0,~N        & $-$15.76  & 1350 & 15.39  & 15.11      & 23.29  
&
13.96  & 14.74       & 21.80  & 1.43  & f \\
1261 & NGC~4482 & d:E5,~N       & $-$17.56  & 1850 & 13.59  & 19.18      & 22.00  
&
12.38  & 18.91       & 20.76  & 1.21  &   \\
1355 & IC~3442  & dE2,~N        & $-$16.63  & 1332 & 14.52  & 30.80      & 23.96  
&
13.05  & 36.83       & 22.88  & 1.47  &   \\
1422 & IC~3468  & E1,~N:        & $-$17.35  & 1372 & 13.80  & 20.34      & 22.34  
&
12.64  & 18.95       & 21.03  & 1.16  & b \\
1567 & IC~3518  & dE5/dS0(5),N &         & 1440 &        &            &        &
13.25  & 26.12       & 22.33  &       & g \\
1895 & UGC~7854 & d:E6         &         & 1032 &        &            &        &
13.80  & 11.51       & 21.11  &       &   \\
\hline
\end{tabular}}
\par
\smallskip
Values followed by a colon have to be considered as uncertain due to disturbing
background or foreground objects. \\
$^a$ Whether this galaxy is really nucleated is not clear. The object
considered as nucleus is very faint and largely off-centered. It could 
therefore also
be a bright globular cluster which in projection happens to lie close to the 
center.
In the~VCC the galaxy is classified as dE,~N, whereas Miller et~al. (\cite{Miller98}) regard 
it
as non-nucleated. Stiavelli et~al. (\cite{Stiavelli01}) present a~HST observation of this 
galaxy and
provide the results of different profile fits as well as the determination of 
the
nuclear cusp slope. \\
$^b$ Disk features discovered (Jerjen et~al. \cite{Jerjen01}; Barazza et~al. \cite{Barazza02}). \\
$^c$ The VCC type of this galaxy, which heavily overlaps with VCC~0846, is ImIV?
We suggest a reclassification as dE,~N. In support of this, the galaxy 
has not been detected in the HI survey of Hoffman et~al.~(\cite{Hoffman89}). \\
$^d$ Spiral structure discovered (Jerjen et~al. \cite{Jerjen00}). \\
$^e$ As part of the Hubble Space Telescope (HST) key project the luminosity of
the tip of the red-giant branch (TRGB) for this galaxy has been determined 
(Harris et~al. \cite{Harris98}): $I_{\rm TRGB} = 26.82 \pm 0.06$. The corresponding distance is $d = 15.7 
\pm
1.5$~Mpc (using $M_I^{\rm TRGB} = -4.2 \pm 01$). \\
$^f$ A velocity profile has recently been derived by Geha et~al. (2001),
showing that this galaxy is not rotating. \\
$^g$ This galaxy could not be fully integrated, since its shape is strongly
non-elliptical. The values given are estimates, using $B_T=14.52$ from Binggeli
\& Cameron (\cite{Binggeli93}) and our $\langle B-R \rangle = 1.27$.
\end{table}