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Table 3

Distances and photometric parameters for the sample galaxies.

Object D A g A i μ e,g r e,g (Re,g)maj m T,g M T,g μ e,i r e,i (Re,i)maj m T,i M T,i ϵin ϵout
[Mpc] [mag] [mag] [mag/arcsec2] [arcmin] [kpc] [mag] [mag] [mag/arcsec2] [arcmin] [kpc] [mag] [mag]
(a) (b) (b) (c) (c) (c) (c) (c) (c) (d) (d)

NGC 1399 20.9 0.05 0.04 24.55 5.87 35.65 8.55 –23.05 5.05 30.70 7.51 –24.09 0.095 0.203
NGC 3923 22.9 0.31 0.17 23.22 2.55 16.97 9.14 –22.66 22.30 3.15 20.98 7.78 –24.02 0.356 0.292
NGC 4365 23.1 0.08 0.04 22.82 1.90 12.79 9.41 –22.41 21.15 1.40 9.41 8.52 –23.30 0.238 0.282
NGC 4472 16.9 0.08 0.04 22.68 2.70 13.29 8.37 –22.77 22.23 4.22 20.73 6.92 –24.22 0.137 0.205
NGC 5044 31.2 0.26 0.14 25.04 3.55 32.20 9.88 –22.59 24.20 3.65 33.13 8.76 –23.71 0.068 0.340
NGC 5846 24.9 0.21 0.11 24.72 4.62 33.41 9.21 –22.77 23.32 3.70 26.80 7.99 –24.00 0.067 0.167

Notes.

(a)

Distances of NGC 3923, NGC 5044, and NGC 5846 are from Tonry et al. (2001); distances of NGC 4365 and NGC 1399 are from Blakeslee et al. (2009); and the distance of NGC 4472 is from Mei et al. (2007).

(b)

Sources for the extinction correction in the g and i band are Schlegel et al. (1998) for all objects but NGC 4472 for which we adopt the value used in Paper I.

(c)

Derived by integrating the growth curves and corrected for interstellar extinction.

(d)

g band mean ellipticity in the ranges − 1.5 < log (R/Re)maj< −0.5 (ϵin) and 0 < log (R/Re)maj< 0.5 (ϵout).

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