Table 3: Results of the host galaxy fitting for the de Vaucouleurs model.
Object z AI KI Ra $m_{\rm core}$ $M_{\rm core}$ $m_{\rm host}$ $M_{\rm host}$ $r_{\rm e}$ $r_{\rm e}$ $\mu_{\rm e}$ $\chi ^2$ $\frac{\chi^2_{\rm deV.}}{\chi^2_{\exp}}$
                  [''] [kpc] [mag/sq'']    
PKS 0057-338 0.875 0.04 1.22 E+ $19.65\pm0.04$ -24.78 $19.60\pm0.05$ -26.04 $0.34\pm0.06$ $ 3.54\pm0.21$ $16.66\pm0.18$ 4.97 1.09
S4 0218+35 0.936b 0.09 1.50 D $19.42\pm0.05$ -25.25 $19.67\pm0.08$ -25.60 $0.51\pm0.03$ $4.79\pm0.28$ $17.76\pm0.20$ 2.09 0.77
Q 0230+3429 0.500 0.11 0.45 E+ $20.60\pm0.20$ -22.38 $15.61\pm0.06$ -27.82 $4.91\pm0.28$ $39.65\pm2.26$ $20.18\pm0.19$ 1.16 1.04
PKS 0406+121 0.504 1.09 0.46 N+ $19.29\pm0.04$ -24.69 $19.91\pm0.17$ -24.53 $0.54\pm0.03$ $4.38\pm0.24$ $18.64\pm0.29$ 0.96 0.99
PKS 0426-380 1.111c 0.06 0.53 D $16.99\pm0.04$ -28.15 $20.25\pm0.12$ -23.50 $0.82\pm0.03$ $7.01\pm0.26$ $20.69\pm0.20$ 9.30 0.95
PKS 0754+100 0.266 0.04 0.21 E $15.51\pm0.03$ -25.82 $17.76\pm0.04$ -23.78 $2.46\pm0.21$ $13.45\pm1.15$ $21.83\pm0.27$ 2.02 1.17
PKS 0820+225 0.951 0.08 1.46 N+ $18.52\pm0.04$ -26.19 $20.67\pm0.10$ -25.50 $0.73\pm0.05$ $7.82\pm0.54$ $18.93\pm0.25$ 1.20 1.00
PKS 0823+033 0.506 0.18 0.46 U $16.01\pm0.06$ -27.07 <16.9 <-26.6       8.23  
RX J0930.9+3933 0.638 0.03 0.66 E+ $20.30\pm0.05$ -23.25 $18.92\pm0.04$ -25.28 $1.50\pm0.10$ $13.68\pm0.91$ $20.36\pm0.18$ 1.10 1.35
B2 0937+26d 0.498 0.03 0.45 E+     $19.43\pm0.05$ -23.91 $0.85\pm0.13$ $6.84\pm1.08$ $20.23\pm0.39$ 1.09 1.06
TXS 1040+244 0.560 0.06 0.53 E+ $17.40\pm0.04$ -25.83 $18.60\pm0.06$ -25.16 $0.80\pm0.11$ $6.85\pm0.94$ $18.98\pm0.36$ 1.84 1.12
1207+39W4 0.615 0.06 0.62 E $18.49\pm0.03$ -24.99 $18.92\pm0.09$ -25.17 $2.81\pm0.51$ $25.18\pm4.57$ $21.79\pm0.49$ 1.87 1.04
Q 1214+1753 0.679 0.07 0.73 N+ $17.13\pm0.03$ -26.62 $18.99\pm0.05$ -25.50 $1.12\pm0.22$ $10.50\pm2.06$ $19.57\pm0.48$ 1.73 1.01
1ES 1249+174W 0.644 0.04 0.67 U $17.96\pm0.03$ -25.62 <19.1 <-25.2       2.18  
PKS 1349-439e ? 0.15   U $17.64\pm0.04$ -26.28 <18.7         1.58  
RX J1422.6+5801 0.638 0.02 0.66 N+ $17.60\pm0.03$ -25.94 $18.86\pm0.08$ -25.33 $2.26\pm0.43$ $20.60\pm3.92$ $21.20\pm0.49$ 1.62 1.00
TXS 1428+370 0.564 0.02 0.54 E+ $21.36\pm0.60$ -21.85 $18.91\pm0.05$ -24.83 $0.38\pm0.04$ $3.27\pm0.34$ $17.70\pm0.28$ 1.15 1.07
PKS 1519-273 1.294 0.56 2.58 U $17.88\pm0.04$ -28.21 <18.1 <-30.6       2.64  
OV -236 0.352 0.30 0.29 E $17.02\pm0.03$ -25.25 $18.31\pm0.03$ -24.25 $1.65\pm0.13$ $10.86\pm0.86$ $20.89\pm0.20$ 10.06 1.36
PKS 2029+121 1.215 0.19 2.28 U $18.33\pm0.04$ -27.20 <19.9 <-27.9       10.29  
PKS 2131-021 1.285 0.13 2.24 U $18.64\pm0.04$ -27.00 <19.9 <-28.3       1.69  
MH 2133-449e ? 0.05   N+ $18.86\pm0.03$   $21.28\pm0.09$   $3.73\pm0.31$     1.65 0.99
PKS 2240-260 0.774 0.05 0.94 U $16.00\pm0.04$ -28.09 <17.7 <-27.3       4.98  
MS 2347.4+1924f 0.515 0.32 0.47 D     $18.85\pm0.04$ -24.89 $0.53\pm0.08$ $4.36\pm0.66$ $18.27\pm0.37$ 1.37 0.93
a Code for galaxy detection and morphology class: U = unresolved, E = elliptical, D = disk, N = resolved, but unclassified, + new detection.
b Grav. lensed BL Lac. z = 0.96 used for the core, z = 0.685 used for the lensing galaxy.
c z = 1.111 used for the core, z = 0.559 used for the intervening galaxy. See subsection A for details.
d Results given for $\epsilon = 0.28$, PA = 30$^\circ$. See subsection A for details.
e Observations taken through Cousins R-filter. Extinction and K-correction for corresponding filter used.
f Results given for $\epsilon = 0.44$, PA = 65$^\circ$. See subsection A for details.


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