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\begin{planotable}{llll}
\tablenum{12}
\tablewidth{4.0in}
\tablecaption{ADOPTED HOST GALAXY PARAMETERS}
\tablehead{
\colhead{Object}&
\colhead{Log Luminosity}&
\colhead{Half-Light Radius}&
\colhead{Ref}\\
\colhead{ }&
\colhead{H band}&
\colhead{kpc}&
\colhead{}
}
\startdata
\input{table12.tgt}
\tablecomments{Adopted luminosities and half light radii
for host galaxies, derived as discussed in the text. 
No spatial information was available for objects marked with reference (0),
and they have been assigned the median luminosity of the remainder
of the sample.}
\tablerefs{
(1) Boroson, Oke and Green (1982);
(2) Gehren et al (1984);
(3) Smith et al (1986);
(4) Boroson and Oke (1984);
%(5) Boroson, Persson and Oke (1985);
(5) McAlary et al (1983);
(6) Neugebauer et al (1985);
(7) Yee and Green (1987);
(8) Hutchings, Crampton and Campbell (1984);
(9) Griersmith and Visvanathan (1979).
(10) Hutchings, Johnson and Pike (1988);
(11) Hutchings, Janson and Neff (1989)
(12) Neizvestnii (1986);
(13) MacKenty (1990).
}
\end{planotable}
\end{document}
Q0003+158 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q0007+106 &  44.43$\pm^{ 0.08}_{ 0.05}$  &  7.00&1   \\
Q0026+129 &  44.30$\pm^{ 0.03}_{ 0.02}$  &  5.76&6   \\
Q0049+171 &  43.60$\pm^{ 0.04}_{ 0.04}$  &  4.34&3   \\
Q0050+124 &  44.62$\pm^{ 0.04}_{ 0.04}$  &  7.68&3   \\
Q0052+251 &  44.78$\pm^{ 0.09}_{ 0.05}$  & 12.61&1   \\
Q0054+144 &  44.71$\pm^{ 0.04}_{ 0.04}$  & 12.44&2   \\
Q0121-590 &  44.90$\pm^{ 0.04}_{ 0.04}$  & 11.53&9   \\
Q0134+329 &  45.44$\pm^{ 0.04}_{ 0.04}$  &  9.24&2   \\
Q0205+024 &  44.19$\pm^{ 0.04}_{ 0.04}$  &  0.19&3   \\
Q0312-770 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q0637-752 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q0804+761 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q0837-120 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q0844+349 &  44.60$\pm^{ 0.25}_{ 0.60}$  & 10.00&0   \\
Q1028+313 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1100+772 &  44.49$\pm^{ 0.03}_{ 0.01}$  & 11.05&4   \\
Q1116+215 &  44.74$\pm^{ 0.04}_{ 0.03}$  & 13.76&5   \\
Q1137+660 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1146-037 &  44.60$\pm^{ 0.25}_{ 0.60}$  & 10.00&0   \\
Q1202+281 &  44.71$\pm^{ 0.03}_{ 0.02}$  & 12.02&5   \\
Q1211+143 &  43.39$\pm^{ 0.00}_{ 0.04}$  &  1.95&6   \\
Q1219+755 &  44.60$\pm^{ 0.11}_{ 0.60}$  & 10.00&0   \\
Q1226+023 &  44.79$\pm^{ 0.03}_{ 0.01}$  &  9.67&4   \\
Q1307+085 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1352+183 &  44.21$\pm^{ 0.04}_{ 0.04}$  &  6.78&8   \\
Q1407+265 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1416-129 &  44.60$\pm^{ 0.15}_{ 0.60}$  & 10.00&0   \\
Q1426+015 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1501+106 &  44.09$\pm^{ 0.04}_{ 0.03}$  &  4.07&6   \\
Q1545+210 &  44.90$\pm^{ 0.04}_{ 0.03}$  & 16.38&6   \\
Q1613+658 &  44.89$\pm^{ 0.04}_{ 0.04}$  & 13.04&7   \\
Q1704+608 &  44.60$\pm^{ 0.03}_{ 0.02}$  &  9.69&6   \\
Q1721+343 &  44.60$\pm^{ 0.30}_{ 0.60}$  & 10.00&0   \\
Q1803+676 &  43.38$\pm^{ 0.04}_{ 0.04}$  &  3.24&8   \\
Q2130+099 &  44.42$\pm^{ 0.04}_{ 0.04}$  &  4.64&2   \\
Q2135-147 &  44.89$\pm^{ 0.04}_{ 0.04}$  & 14.36&3   \\