Table 2: Properties of the host galaxiesa.
  z AHb mH(nuc) mH(gal) $\mu_{\rm e}$c $r_{\rm e}$ $R_{\rm e}$ MH(nuc) MH(gal) N/G
    mag       arcsec kpc      
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
1ES 0120+340 0.272 0.06 14.57 14.32 17.44 2.30 12.8 -26.77 -27.19 0.68
MS 0158.5+0019 0.298 0.03 16.54 15.67 18.41 2.10 12.4 -25.02 -26.02 0.40
MS 0205.7+3509 0.318 0.07 16.15 16.76 17.53 0.90 5.6 -25.57 -25.09 1.6
MS 0317.0+1834 0.190 0.11 15.58 15.16 18.06 1.60 6.8 -24.90 -25.52 0.56
Mrk 180 0.045 0.02 13.71 11.86 18.04 4.30 5.3 -23.50 -25.60 0.14
1ES 1218+304 0.182 0.02 14.51 14.29 18.72 3.15 13.0 -25.87 -26.26 0.70
MS 1221.8+2452 0.218 0.02 14.69 15.83 16.01 0.50 2.4 -26.12 -25.09 2.6
MS 1229.2+6430 0.164 0.02 18.32 15.06 18.36 1.75 6.7 -21.82 -25.23 0.04
1ES 1255+244 0.140 0.01 15.91 14.44 18.69 2.50 8.4 -23.86 -25.54 0.21
1ES 1426+428 0.129 0.02 15.37 13.45 18.57 3.60 11.3 -24.21 -26.21 0.16
1ES 1440+122 0.162 0.02 16.23 14.15 18.87 3.35 12.6 -23.88 -26.14 0.12
MS 1458.8+2249 0.235 0.04 14.21 15.18 17.89 1.70 8.5 -26.78 -25.95 2.1
MS 1552.1+2020 0.273 0.04 15.83 14.42 17.88 2.70 15.0 -25.52 -27.09 0.24
Mrk 501 0.034 0.02 12.22 10.41 17.13 5.30 5.0 -24.36 -26.55 0.13
I Zw 187 0.055 0.03 14.44 13.19 18.51 3.00 4.4 -23.21 -24.68 0.26
3C 371 0.051 0.05 12.53 11.97 16.59 2.15 3.0 -24.95 -25.89 0.42
1ES 1853+671 0.212 0.06 16.87 15.44 19.40 2.80 13.0 -23.87 -25.47 0.23
1ES 1959+650 0.048 0.11 13.69 12.30 18.27 3.95 5.1 -23.66 -25.17 0.25
BL Lac 0.069 0.21 11.90 12.23 15.05 1.00 1.8 -26.26 -26.00 1.3
PKS 2201+04 0.027 0.06 15.50 11.64 17.39 3.30 2.5 -20.58 -24.68 0.02
PKS 2254+074 0.194 0.06 13.96 14.16 18.43 3.05 13.2 -26.57 -26.52 1.0
1ES 2326+174 0.213 0.04 17.12 14.75 17.20 1.40 6.5 -23.63 -26.16 0.10
1ES 2344+514 0.044 0.17 15.69 11.60 17.15 3.20 3.8 -21.46 -25.86 0.02
a Columns 1 and 2 give the name and redshift of the object; Col. 3: the interstellar extinction correction; Cols. 4 and 5: the apparent nuclear and host galaxy magnitude; Col. 6: the surface brightness $\mu$(e); Cols. 7 and 8: the bulge scalelength in arcsec and kpc; Cols. 9 and 10: the absolute nuclear and host galaxy magnitude; and Col. 11: the nucleus/galaxy luminosity ratio.
b The interstellar extinction corrections were computed using R-band extinction coefficient from Urry et al. (2000) and AH/AR = 0.234 (Cardelli et al. 1989).
c Corrected for galactic extinction and cosmological dimming.

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