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Table 3

Magnitudes and effective parameters.

Name Band m L Δm m T μ e ϵ (μe)V
[arcsec 1/4] [mag] [mag] [mag] [arcsec 1/4] [mag] [arcsec 1/4] [mag] [arcsec1/4]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

NGC 4472 g 5.47 8.55 0.05a 8.50 3.49 22.59 0.16 3.42 22.73 3.73
NGC 4472 g 6.56 8.48 0.11b 8.37 3.71 23.03 0.19 3.61
NGC 4472 g 6.56 8.37 0.10c 8.27 3.86 23.31 0.16 3.78
NGC 4472 i 6.47 7.19 0.23d 6.96 3.99 22.27 0.18 3.89
NGC 4472 i 6.56 7.10 0.10e 7.00 3.90 22.09 0.16 3.82
NGC 4434 g 2.89 12.52 0.60 12.46 1.83 21.08 0.05 1.82 20.08 1.83
NGC 4434 i 2.89 11.45 0.50 11.40 1.83 19.81 0.05 1.82
NGC 4464 g 2.76 13.04 0.40 13.00 1.67 20.43 0.27 1.61 19.92 1.66
NGC 4464 i 2.76 11.84 0.20 11.82 1.67 19.05 0.27 1.61
NGC 4467 g 2.33 14.63 0.40 14.59 1.57 21.31 0.22 1.52 20.91 1.56
NGC 4467 i 2.33 13.50 0.20 13.48 1.55 20.03 0.23 1.50
VCC 1199 g 2.02 15.92 0.10 15.94 1.25 20.81 0.11 1.23 20.28 1.22
VCC 1199 i 2.02 14.71 0.10 14.70 1.25 19.57 0.12 1.23
UGC 7636 g 3.41 14.22 0.07 14.15 2.62 24.91 0.39 1.41
UGC 7636 i 3.41 13.38 0.53 12.85 3.13 21.26 0.39 2.95

Notes. Column 3: major axis of the faintest isophote for which SB is measured. Column 4: magnitude within aL, computed assuming a fixed mean ellipticity ϵ (Col. 7). Column 5: extrapolation of the growth curve to infinity. Column 6: total magnitude mT = mL + Δm. This value is not corrected for interstellar extinction. According to Arrigoni Battaia et al. (2012), the correction would be Ag = 0.074 and Ai = 0.044 mag. Column 7: major axis of the effective isophote of flattening ϵ that encircles half of the total light. Column 8: SB at the effective semi-major axis ae. Column 9: adopted mean ellipticity. Column 10: mean effective radius . Columns 11 and 12: effective parameters for the V band (Kormendy et al. 2009).

(a)

Excluding the ICL tail.

(b)

Including the ICL tail.

(c)

Including the ICL tail, but flattening the ellipticity profile from 1.75 arcmin on.

(d)

With measured ellipticity.

(e)

With ellipticity modified as for the g band (note c).

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