Table 1: Galaxy sample.
NGC $V_{\rm {LG}}$ Scale Type $M_R^{\rm tot}$ $M_R^{\rm bul}$ B/D PA Exp. time $\epsilon$ $_{\rm D}$ $\epsilon$ $_{\rm B}$ r $_{\rm bulge}$ Best templ. S/N
  km s-1 kpc/ $^{\prime\prime}$   mag mag   deg s     $^{\prime\prime}$   pix-1
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)

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 -- -- 0.0011 80 1500 0.631 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
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 (Karachentsev & Makarov 1996), from optical heliocentric velocities given in the Third Reference Catalogue of Bright Galaxies (1991) (hereafter RC3). (3): Scale in kpc/arcsec from Falcón-Barroso et al. (2002).
(4): Type index T from the RC3.
(5) and (6): Absolute magnitudes, in R-band, from Peletier & Balcells (1997) (H0=50 km s-1 Mpc-1).
(7): Bulge-to-disk ratio from an R-band bulge-disk decomposition following Kent's (1984) method (Peletier & Balcells 1997).
(8): The position angle, in degrees, (N - E) of the dust-free minor axis (Peletier & Balcells 1997).
(9): Integration time, in sec, for each galaxy during the observations.
(10): Disk ellipticity from Peletier & Balcells (1997).
(11): Effective bulge ellipticity, from HST H-band ellipticity profiles, measured at the geometric effective radius (Balcells et al. 2003).
(12): Minor axis bulge radius, derived from Balcells et al. (2003) 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 (Peletier & Balcells 1997) (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 ( $1.2 \times 0.36$ arcsec2).
1 From Prada et al. (1996).

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