Table 1: Basic data and model-free parameters of the early-type dwarfs considered in this study (extinction-corrected).
VCC Name Type $M_{B_{\rm T}}$ $v_{\odot}$ $B_{\rm T}$ $r_{\rm eff}^B$ $\mu_{\rm eff}^B$ $R_{\rm T}$ $r_{\rm eff}^R$ $\mu_{\rm eff}^R$ B-R Notes
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)  
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    
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. (1998) regard it as non-nucleated. Stiavelli et al. (2001) 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. 2001; Barazza et al. 2002).
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. (1989).
d Spiral structure discovered (Jerjen et al. 2000).
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. 1998): $I_{\rm TRGB} = 26.82 \pm 0.06$. 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 BT=14.52 from Binggeli & Cameron (1993) and our $\langle B-R \rangle = 1.27$.

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