TABLE 2 UV EMISSION LINE EQUIVALENT WIDTHS$^a$ Name & \lyb & err &\lya & err & \siiv & err & \civ & err & \heii & err & Al\,III & err \\ & +\,\ovi & & +\,NV & & +\,OIV] & & & & +\,O\,III] & & +\,\ciii & \\ 0026+129 & ... & ... & 59.0 & 1.8 & <6.1 & ... & 32.7 & 1.0 & 18.3 & 0.6 & <29.6 & ... \\ 0044+030 & <11.3 & ... & 63.4 & 6.4 & 50.3 & 5.5 & 50.8 & 1.8 & 9.8 & 0.6 & 27.9 & 1.5 \\ 0052+251 & ... & ... & 91.4 & 2.6 & 8.0 & 1.6 & 119.1 & 2.5 & 15.7 & 0.9 & <82.5 & ... \\ 0117+213$^{l}$ & 10.2 & 1.4 & 27.6 & 1.5 & ... & ... & ... & ... & ... & ... & ... & ... \\ 0119-286 & ... & ... & 89.8 & 4.3 & 33.5 & 2.8 & 76.3 & 2.7 & 12.2 & 0.9 & <36.0 & ... \\ 0134+329 & <12.6 & ... & <13.1 & ... & 13.9 & 2.0 & <133.3 & ... & <35.4 & ... & 19.3 & 2.6 \\ 0205+024 & ... & ... & 52.8 & 4.4 & <5.1 & ... & 38.5 & 1.2 & 9.5 & 0.6 & <33.2 & ... \\ 0312-770 & 24.7 & 1.1 & 72.6 & 2.5 & 5.3 & 0.9 & 69.7 & 1.1 & <563.5 & ... & <139.5 & ... \\ 0405-123 & 4.1 & 0.3 & 50.1 & 0.8 & <6.9 & ... & 25.7 & 1.1 & 3.0 & 0.5 & 5.9 & 0.7 \\ 0414-060 & 9.0 & 0.5 & 109.1 & 6.9 & 12.9 & 1.8 & 57.9 & 1.9 & 9.4 & 1.4 & ... & ... \\ 0558-504 & ... & ... & 27.8 & 0.8 & <2.7 & ... & 23.1 & 0.5 & 10.2 & 0.3 & <14.9 & ... \\ 0624+691 & 7.2 & 0.6 & 60.9 & 1.4 & <1.5 & ... & 51.3 & 6.5 & <16.1 & ... & 12.2 & 0.9 \\ 0736+017 & ... & ... & 132.5 & 10.1 & <14.5 & ... & 94.5 & 3.2 & <681.9 & ... & <125.8 & ... \\ 0743-673$^{l}$ & 6.3 & 1.2 & 57.2 & 3.1 & ... & ... & ... & ... & ... & ... & ... & ... \\ 0804+761 & ... & ... & 101.8 & 2.8 & 28.0 & 1.1 & 81.7 & 1.6 & 19.3 & 0.5 & 63.7 & 4.2 \\ 0837-120 & ... & ... & 87.6 & 5.5 & <13.9 & ... & 91.4 & 2.5 & <32.1 & ... & <39.8 & ... \\ 0859-140$^{l}$ & <193.0 & ... & <78.5 & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 0906+484 & ... & ... & 59.9 & 3.0 & <11.1 & ... & 52.4 & 2.2 & 14.8 & 1.0 & <38.6 & ... \\ 0953+414$^{s}$ & 24.9 & 1.3 & 63.8 & 2.8 & 8.9 & 0.9 & 53.6 & 1.1 & ... & ... & ... & ... \\ 1001+291 & <4.5 & ... & 34.1 & 2.3 & 5.6 & 0.7 & <14.4 & ... & <14.1 & ... & 20.1 & 2.1 \\ 1004+130 & <5.6 & ... & 9.1 & 1.5 & 12.0 & 1.0 & <100.2 & ... & $<$1939.9 & ... & <69.1 & ... \\ 1007+417 & <7.0 & ... & 79.1 & 4.9 & <21.8 & ... & 72.5 & 2.8 & 8.3 & 1.0 & <6.2 & ... \\ 1008+133$^{l}$ & <7.6 & ... & 17.9 & 1.7 & 180.7 & 31.3 & ... & ... & ... & ... & ... & ... \\ 1011-282$^{s}$ & 17.1 & 3.2 & 116.5 & 12.7 & <11.7 & ... & ... & ... & ... & ... & ... & ... \\ 1012+008$^{s}$ & ... & ... & 72.9 & 4.2 & <9.8 & ... & 13.3 & 1.4 & <3.7 & ... & ... & ... \\ 1048-090 & <24.4 & ... & 76.1 & 13.0 & 62.9 & 7.1 & <85.0 & ... & <45.5 & ... & 18.3 & 3.4 \\ 1049-005 & <26.6 & ... & 83.9 & 10.0 & <8.1 & ... & <124.9 & ... & <78.4 & ... & 18.6 & 3.5 \\ 1100+772 & 7.6 & 0.6 & 60.4 & 1.5 & 3.5 & 0.5 & 89.9 & 5.6 & <18.1 & ... & 12.4 & 2.0 \\ 1103-006 & <13.0 & ... & 37.3 & 2.4 & <12.9 & ... & 27.7 & 3.9 & <10.2 & ... & 20.7 & 1.6 \\ 1104+167$^{l}$ & ... & ... & 83.4 & 12.2 & <20.5 & ... & 85.1 & 3.9 & 13.8 & 1.1 & <11.5 & ... \\ 1116+215 & ... & ... & 62.9 & 1.3 & <2.6 & ... & 36.5 & 0.5 & <1.2 & ... & 31.2 & 2.8 \\ 1127-145$^{s}$ & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 1136-135 & <4.7 & ... & 63.5 & 1.6 & <17.6 & ... & 50.7 & 3.1 & 6.7 & 1.0 & 20.0 & 1.0 \\ 1137+660 & 13.9 & 1.0 & 74.4 & 7.9 & 41.4 & 7.2 & 45.9 & 3.9 & <9.7 & ... & <28.4 & ... \\ 1146-037 & <463.7 & ... & <44.4 & ... & <43.2 & ... & 268.1 & 33.5 & <24.5 & ... & 51.8 & 5.0 \\ 1148+549 & <6.3 & ... & 54.6 & 2.3 & 11.3 & 1.2 & 18.0 & 1.6 & <22.9 & ... & ... & ... \\ 1151+117 & ... & ... & 112.0 & 7.2 & <12.7 & ... & 69.6 & 2.6 & 21.8 & 1.5 & <36.6 & ... \\ 1156+295 & <1.9 & ... & <15.6 & ... & 8.8 & 1.6 & <5.7 & ... & <3.9 & ... & ... & ... \\ 1156+631$^{l}$ & ... & ... & <133.4 & ... & <28.8 & ... & 91.3 & 7.8 & <11.2 & ... & <14.3 & ... \\ 1202+281 & ... & ... & 74.2 & 1.3 & <3.5 & ... & 129.1 & 1.2 & 18.9 & 0.4 & <35.4 & ... \\ 1206+459 & <17.6 & ... & 44.5 & 2.1 & <10.5 & ... & ... & ... & ... & ... & ... & ... \\ 1216+069 & 10.1 & 1.7 & 53.9 & 3.9 & 9.3 & 1.4 & 65.0 & 10.3 & <24.7 & ... & 14.1 & 2.2 \\ 1241+176 & 8.0 & 0.9 & 45.4 & 0.5 & <6.3 & ... & ... & ... & ... & ... & ... & ... \\ 1248+401 & <17.1 & ... & 39.6 & 2.5 & <8.7 & ... & <35.3 & ... & ... & ... & ... & ... \\ 1259+593 & <7.1 & ... & 26.8 & 1.1 & <27.7 & ... & 58.6 & 8.6 & 12.2 & 2.2 & 16.6 & 1.0 \\ 1302-102 & <1.5 & ... & 42.9 & 0.8 & 4.4 & 0.3 & 15.9 & 1.8 & <9.7 & ... & 16.6 & 1.0 \\ 1307+085 & ... & ... & 76.1 & 3.4 & <8.1 & ... & 93.7 & 1.9 & 18.8 & 0.8 & <31.1 & ... \\ 1309+355$^{s}$ & ... & ... & 46.7 & 2.3 & <4.9 & ... & 32.9 & 1.0 & <2.6 & ... & ... & ... \\ 1317+277 & 5.9 & 1.1 & 27.0 & 1.0 & 3.0 & 0.4 & 26.5 & 1.2 & ... & ... & ... & ... \\ 1318-113$^{s}$ & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 1333+176 & <9.8 & ... & 28.5 & 2.2 & <83.6 & ... & 42.2 & 6.4 & <9.9 & ... & 7.8 & 1.5 \\ 1334+246 & ... & ... & 54.4 & 5.3 & <25.2 & ... & 63.4 & 6.6 & 39.7 & 2.3 & <133.2 & ... \\ 1338+416 & <10.7 & ... & 25.8 & 1.0 & 26.4 & 1.8 & ... & ... & ... & ... & ... & ... \\ 1352+183 & ... & ... & 71.0 & 3.2 & <7.0 & ... & 85.5 & 2.3 & 17.0 & 1.0 & 35.8 & 6.5 \\ 1354+195$^{s}$ & 17.9 & 1.5 & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 1355-416$^{s}$ & 14.8 & 2.1 & 63.7 & 3.7 & 11.7 & 1.1 & ... & ... & ... & ... & ... & ... \\ 1356+581$^{s}$ & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 1415+451$^{s}$ & ... & ... & 117.0 & 7.0 & 42.2 & 3.7 & 80.3 & 3.4 & 17.9 & 1.1 & ... & ... \\ 1425+267 & <18.9 & ... & 51.3 & 3.4 & 40.5 & 2.2 & 131.3 & 19.7 & <37.7 & ... & 35.1 & 3.8 \\ 1444+407$^{s}$ & <3.5 & ... & 51.3 & 2.2 & 14.0 & 0.9 & ... & ... & ... & ... & ... & ... \\ 1512+370 & 7.6 & 0.5 & 57.0 & 0.8 & 3.5 & 0.3 & 83.7 & 3.6 & 17.4 & 1.7 & 15.2 & 0.7 \\ 1522+101 & <6.3 & ... & 41.2 & 1.6 & ... & ... & ... & ... & ... & ... & ... & ... \\ 1525+227 & <10.5 & ... & 40.1 & 6.4 & <7.8 & ... & <32.7 & ... & <63.4 & ... & <51.2 & ... \\ 1526+285 & 23.7 & 4.7 & 120.9 & 6.3 & <182.4 & ... & <316.5 & ... & <99.3 & ... & <37.5 & ... \\ 1538+477 & 8.1 & 0.8 & 75.8 & 10.0 & 19.8 & 2.7 & 41.7 & 1.7 & 11.5 & 1.1 & ... & ... \\ 1545+210 & <6.6 & ... & 58.1 & 3.6 & <7.4 & ... & 79.9 & 5.1 & <35.6 & ... & <19.6 & ... \\ 1552+085 & ... & ... & 78.7 & 9.0 & <20.4 & ... & 210.3 & 22.1 & 46.3 & 4.0 & <142.4 & ... \\ 1612+261$^{s}$ & ... & ... & 135.7 & 11.1 & 22.0 & 4.4 & 148.7 & 6.4 & 25.1 & 1.7 & ... & ... \\ 1617+175$^{l}$ & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & 41.2 & 7.6 \\ 1630+377 & 3.5 & 0.6 & 39.5 & 1.0 & ... & ... & ... & ... & ... & ... & ... & ... \\ 1634+706 & 2.3 & 0.2 & 44.0 & 0.4 & ... & ... & ... & ... & ... & ... & ... & ... \\ 1641+399 & 9.0 & 1.0 & 54.5 & 3.5 & <14.5 & ... & 33.8 & 1.8 & 4.0 & 0.7 & <5.2 & ... \\ 1656+053$^{s}$ & <7.4 & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 1718+481 & <6.3 & ... & 33.9 & 0.6 & 5.4 & 0.9 & ... & ... & ... & ... & ... & ... \\ 1721+343 & 30.2 & 1.2 & 126.3 & 4.2 & <3.6 & ... & 94.0 & 1.4 & <11.0 & ... & 18.6 & 3.0 \\ 1803+676 & ... & ... & 95.8 & 3.7 & 9.6 & 0.8 & 133.3 & 1.3 & 15.8 & 0.4 & 34.4 & 4.6 \\ 1850-782$^{l}$ & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... & <140.0 & ... \\ 1928+738 & 7.8 & 1.3 & 71.3 & 3.4 & 9.1 & 1.1 & <76.0 & ... & <85.9 & ... & 22.7 & 3.7 \\ 2112+059 & 35.7 & 6.5 & 68.9 & 2.8 & <60.6 & ... & <136.0 & ... & <23.8 & ... & 30.8 & 1.7 \\ 2141+175$^{s}$ & 7.1 & 1.1 & 48.1 & 2.5 & 7.3 & 1.1 & 18.2 & 0.9 & ... & ... & ... & ... \\ 2201+315 & 9.7 & 0.8 & 44.1 & 1.5 & 16.1 & 0.6 & 45.9 & 3.8 & 25.7 & 4.1 & 9.0 & 1.7 \\ 2251+113 & <19.0 & ... & 28.2 & 2.8 & <5.2 & ... & 79.8 & 9.3 & <40.1 & ... & 47.8 & 3.8 \\ 2251+158$^{s}$ & 14.5 & 2.6 & ... & ... & ... & ... & ... & ... & ... & ... & ... & ... \\ 2302+029 & <9.3 & ... & 12.6 & 1.7 & <6.0 & ... & <33.9 & ... & ... & ... & ... & ... \\ 2344+092 & 26.1 & 1.9 & 58.6 & 5.7 & <17.6 & ... & 32.3 & 2.2 & <6.4 & ... & <58.6 & ... \\ TABLE 3 ADOPTED $B$ MAGNITUDE $k$-CORRECTION$^a$ $z$ & $\Delta B$ & $z$ & $\Delta B$ & $z$ & $\Delta B$ & $z$ & $\Delta B$ & $z$ & $\Delta B$ \\ 0.0 & 0.000 & 0.7 & -0.511 & 1.4 & -0.733 & 2.1 & -0.832 & 2.8 & -0.724 \\ 0.1 & -0.071 & 0.8 & -0.529 & 1.5 & -0.772 & 2.2 & -0.870 & 2.9 & -0.669 \\ 0.2 & -0.171 & 0.9 & -0.545 & 1.6 & -0.811 & 2.3 & -0.894 & 3.0 & -0.607 \\ 0.3 & -0.259 & 1.0 & -0.574 & 1.7 & -0.822 & 2.4 & -0.879 & 3.1 & -0.541 \\ 0.4 & -0.349 & 1.1 & -0.631 & 1.8 & -0.828 & 2.5 & -0.849 & 3.2 & -0.466 \\ 0.5 & -0.421 & 1.2 & -0.671 & 1.9 & -0.827 & 2.6 & -0.813 & 3.3 & -0.378 \\ 0.6 & -0.475 & 1.3 & -0.703 & 2.0 & -0.823 & 2.7 & -0.772 & 3.4 & -0.278 \\ $^a$From LBQS composite spectrum, for a Mathews \& Sandage $B$ filter. TABLE 4 CONTINUUM ENERGY DISTRIBUTIONS Name & $z$ & $B$ & $F_x^{a}$ & $N_H^{b}$ & \auv$^{c}$ & $b_{uv}^{d}$ & log$l_{opt}^{e}$ & log$l_{x}^{f}$ & log$l_{uv}^{g}$ & \aox \\ 0026+129 & 0.142 & 14.95 & 905 & 4.6 & -0.7 & -11.5 & 30.54 & 26.89 & 30.12 & 1.40 \\ 0044+030 & 0.624 & 15.97 & 97 & 2.9 & -0.5 & -12.5 & 31.28 & 27.20 & 31.09 & 1.57 \\ 0052+251 & 0.155 & 15.42 & 910 & 4.6 & -1.4 & -9.2 & 30.42 & 26.97 & 30.27 & 1.33 \\ 0117+213 & 1.493 & 16.05 & <170 & 4.8 & -0.2 & -13.9 & 32.03 & <28.19 & 31.25 & $>$ 1.48 \\ 0119-286 & 0.117 & 14.89 & ... & 1.6 & -1.3 & -9.5 & 30.34 & ... & 30.15 & ... \\ 0134+329 & 0.367 & 16.62 & 410 & 4.6 & -1.1 & -11.0 & 30.65 & 27.37 & 30.30 & 1.26 \\ 0205+024 & 0.156 & 15.67 & 660 & 3.3 & -0.8 & -11.4 & 30.29 & 26.84 & 30.05 & 1.32 \\ 0312-770 & 0.223 & 16.26 & 510 & 7.5 & -1.2 & -10.1 & 30.48 & 27.03 & 30.42 & 1.32 \\ 0405-123 & 0.574 & 14.75 & 685 & 3.7 & -1.1 & -9.9 & 31.73 & 27.98 & 31.64 & 1.44 \\ 0414-060 & 0.781 & 16.24 & 230 & 5.1 & -0.5 & -12.5 & 31.44 & 27.77 & 31.12 & 1.41 \\ 0558-504 & 0.137 & 15.18 & ... & 5.4 & -1.3 & -9.5 & 30.44 & ... & 30.25 & ... \\ 0624+691 & 0.370 & 14.50$^v$ & ... & 7.0 & -0.7 & -11.3 & 31.58 & ... & 31.17 & ... \\ 0736+017 & 0.191 & 16.90 & 235 & 9.4 & -0.9 & -11.4 & 30.16 & 26.56 & 29.84 & 1.38 \\ 0743-673 & 1.510 & 16.61 & ... & 11.8 & 0.0 & -14.4 & 32.04 & ... & 31.31 & ... \\ 0804+761 & 0.100 & 15.15 & 1400 & 3.1 & -0.1 & -13.0 & 30.11 & 26.78 & 30.07 & 1.28 \\ 0837-120 & 0.198 & 15.78 & 1200 & 5.9 & -1.0 & -10.9 & 30.52 & 27.30 & 30.12 & 1.24 \\ 0859-140 & 1.327 & 16.79 & 129 & 5.7 & -0.4 & -13.2 & 31.68 & 27.97 & 31.13 & 1.42 \\ 0906+484 & 0.118 & 16.46 & 38 & 1.8 & -1.4 & -9.6 & 29.72 & 25.36 & 29.60 & 1.68 \\ 0953+414 & 0.239 & 14.80$^v$ & ... & 1.3 & -1.5 & -8.6 & 30.97 & ... & 30.81 & ... \\ 1001+291 & 0.329 & 15.62 & ... & 1.9 & -1.6 & -8.8 & 30.90 & ... & 30.81 & ... \\ 1004+130 & 0.241 & 15.93 & <26 & 3.7 & -0.5 & -12.5 & 30.55 & <25.81 & 30.23 & $>$ 1.82 \\ 1007+417 & 0.611 & 16.80$^v$ & ... & 1.2 & -1.1 & -10.5 & 30.93 & ... & 31.15 & ... \\ 1008+133 & 1.287 & 16.24 & <37 & 3.8 & -0.4 & -12.9 & 31.81 & <27.40 & 31.41 & $>$ 1.69 \\ 1011-282 & 0.253 & 16.80 & 230 & 5.7 & -1.3 & -10.2 & 30.31 & 26.80 & 30.14 & 1.35 \\ 1012+008 & 0.185 & 16.30$^v$ & ... & 3.5 & -1.2 & -10.5 & 30.18 & ... & 29.82 & ... \\ 1048-090 & 0.344 & 16.00 & 440 & 3.2 & -1.3 & -10.1 & 30.80 & 27.35 & 30.40 & 1.33 \\ 1049-005 & 0.357 & 16.25$^v$ & ... & 3.9 & -0.5 & -12.6 & 30.75 & ... & 30.33 & ... \\ 1100+772 & 0.311 & 15.86 & 580 & 3.0 & -1.1 & -10.2 & 30.77 & 27.38 & 30.70 & 1.30 \\ 1103-006 & 0.426 & 16.39 & ... & 4.1 & -1.0 & -11.0 & 30.84 & ... & 30.61 & ... \\ 1104+167 & 0.634 & 15.91 & ... & 1.5 & -1.0 & -11.1 & 31.32 & ... & 30.96 & ... \\ 1116+215 & 0.177 & 15.17 & 710 & 1.3 & -1.0 & -10.1 & 30.57 & 26.98 & 30.72 & 1.38 \\ 1127-145 & 1.187 & 17.17 & 150 & 4.1 & -1.4 & -10.3 & 31.38 & 27.94 & 31.24 & 1.32 \\ 1136-135 & 0.557 & 16.15 & ... & 3.5 & -1.6 & -9.0 & 31.14 & ... & 31.19 & ... \\ 1137+660 & 0.646 & 16.50 & 335 & 1.0 & -1.0 & -10.8 & 31.10 & 27.77 & 31.19 & 1.28 \\ 1146-037 & 0.341 & 16.96 & 530 & 2.5 & -0.8 & -12.4 & 30.40 & 27.42 & 29.64 & 1.14 \\ 1148+549 & 0.969 & 16.12$^v$ & ... & 1.2 & -1.0 & -10.9 & 31.60 & ... & 31.62 & ... \\ 1151+117 & 0.176 & 15.81$^v$ & ... & 2.5 & -0.8 & -11.5 & 30.31 & ... & 30.07 & ... \\ 1156+295 & 0.729 & 14.80 & ... & 1.6 & -0.4 & -12.9 & 31.88 & ... & 31.05 & ... \\ 1156+631 & 0.594 & 17.10$^v$ & ... & 1.9 & -1.0 & -11.0 & 30.79 & ... & 30.81 & ... \\ 1202+281 & 0.165 & 15.02 & 870 & 1.7 & -0.9 & -11.2 & 30.58 & 27.01 & 29.83 & 1.37 \\ 1206+459 & 1.158 & 16.09$^v$ & ... & 1.3 & 0.1 & -14.9 & 31.75 & ... & 30.78 & ... \\ 1216+069 & 0.334 & 15.68 & 300 & 1.6 & -1.1 & -10.6 & 30.89 & 27.15 & 30.62 & 1.43 \\ 1241+176 & 1.273 & 15.38 & 55 & 1.8 & 0.2 & -15.3 & 32.11 & 27.56 & 30.77 & 1.75 \\ 1248+401 & 1.030 & 16.36$^v$ & ... & 1.4 & -0.5 & -12.7 & 31.56 & ... & 31.10 & ... \\ 1259+593 & 0.472 & 15.90$^v$ & ... & 1.4 & -0.9 & -11.0 & 31.08 & ... & 30.96 & ... \\ 1302-102 & 0.286 & 15.09 & 540 & 3.4 & -0.8 & -11.1 & 31.02 & 27.28 & 30.78 & 1.44 \\ 1307+085 & 0.155 & 15.28 & 840 & 2.1 & -1.1 & -10.1 & 30.42 & 26.94 & 30.17 & 1.34 \\ 1309+355 & 0.184 & 15.75$^v$ & ... & 1.0 & -1.2 & -10.3 & 30.37 & ... & 29.93 & ... \\ 1317+277 & 1.022 & 16.12 & ... & 1.2 & -0.4 & -12.9 & 31.65 & ... & 31.39 & ... \\ 1318-113 & 2.308 & 17.81 & ... & 2.8 & -1.7 & -9.5 & 31.64 & ... & 31.98 & ... \\ 1333+176 & 0.554 & 15.64 & 49 & 1.8 & -0.9 & -11.3 & 31.31 & 26.80 & 31.02 & 1.73 \\ 1334+246 & 0.107 & 15.30$^v$ & ... & 1.1 & 1.1 & -18.2 & 30.10 & ... & 28.79 & ... \\ 1338+416 & 1.219 & 16.38$^v$ & ... & 0.9 & 0.0 & -14.5 & 31.68 & ... & 30.88 & ... \\ 1352+183 & 0.152 & 15.71 & 530 & 2.0 & -1.4 & -9.5 & 30.23 & 26.72 & 29.90 & 1.35 \\ 1354+195 & 0.720 & 16.48 & ... & 2.2 & -0.4 & -13.1 & 31.20 & ... & 30.82 & ... \\ 1355-416 & 0.313 & 15.76 & 620 & 6.2 & -0.5 & -12.3 & 30.92 & 27.41 & 30.54 & 1.35 \\ 1356+581 & 1.371 & 17.32 & ... & 1.4 & -0.8 & -12.4 & 31.40 & ... & 31.05 & ... \\ 1415+451 & 0.114 & 16.04$^v$ & ... & 1.1 & -1.0 & -11.0 & 29.86 & ... & 29.44 & ... \\ 1425+267 & 0.362 & 15.67 & 73 & 1.7 & -0.4 & -13.1 & 30.96 & 26.61 & 30.16 & 1.67 \\ 1444+407 & 0.267 & 16.25$^v$ & ... & 1.3 & -1.0 & -10.8 & 30.48 & ... & 30.38 & ... \\ 1512+370 & 0.371 & 15.48 & 350 & 1.4 & -1.4 & -9.6 & 31.05 & 27.31 & 30.75 & 1.44 \\ 1522+101 & 1.321 & 16.04$^v$ & ... & 2.9 & 0.1 & -14.4 & 31.88 & ... & 31.31 & ... \\ 1525+227 & 0.253 & 16.79 & 38 & 4.2 & -0.6 & -12.2 & 30.27 & 26.02 & 30.16 & 1.63 \\ 1526+285 & 0.450 & 16.00$^v$ & ... & 2.6 & -1.2 & -10.5 & 31.00 & ... & 30.57 & ... \\ 1538+477 & 0.770 & 16.31$^v$ & ... & 1.6 & -0.1 & -13.8 & 31.33 & ... & 30.88 & ... \\ 1545+210 & 0.264 & 16.05 & 780 & 4.3 & -1.2 & -10.3 & 30.60 & 27.37 & 30.36 & 1.24 \\ 1552+085 & 0.119 & 16.02 & 20 & 3.4 & -0.1 & -13.8 & 29.92 & 25.08 & 29.41 & 1.86 \\ 1612+261 & 0.131 & 16.00 & 710 & 4.1 & -1.0 & -11.2 & 30.03 & 26.72 & 29.53 & 1.27 \\ 1617+175 & 0.114 & 15.53 & 285 & 4.1 & -1.4 & -9.4 & 30.10 & 26.20 & 29.93 & 1.50 \\ 1630+377 & 1.471 & 16.26$^v$ & ... & 1.1 & 0.0 & -14.3 & 31.87 & ... & 31.30 & ... \\ 1634+706 & 1.334 & 14.90 & 93 & 4.6 & -0.2 & -12.9 & 32.40 & 27.83 & 31.92 & 1.75 \\ 1641+399 & 0.595 & 18.70 & 527 & 1.0 & -0.2 & -13.4 & 30.15 & 27.90 & 30.84 & 0.86 \\ 1656+053 & 0.887 & 17.00 & 360 & 6.1 & -0.8 & -11.6 & 31.28 & 28.07 & 31.21 & 1.23 \\ 1718+481 & 1.084 & 15.63$^v$ & ... & 2.3 & -0.3 & -12.9 & 31.89 & ... & 31.74 & ... \\ 1721+343 & 0.206 & 16.80$^v$ & 1700 & 3.0 & -1.4 & -9.2 & 30.06 & 27.49 & 30.51 & 0.99 \\ 1803+676 & 0.136 & 16.04 & 330 & 4.7 & -0.9 & -11.1 & 30.07 & 26.42 & 29.91 & 1.40 \\ 1850-782 & 0.162 & 15.80$^v$ & ... & 9.0 & 0.1 & -14.6 & 30.45 & ... & 29.50 & ... \\ 1928+738 & 0.302 & 16.80$^v$ & ... & 7.8 & -1.2 & -10.1 & 30.52 & ... & 30.57 & ... \\ 2112+059 & 0.466 & 18.90 & <61 & 6.5 & -0.9 & -11.3 & 29.99 & <26.75 & 30.82 & $>$ 1.24 \\ 2141+175 & 0.213 & 15.91 & 165 & 8.2 & -1.4 & -9.4 & 30.61 & 26.51 & 30.50 & 1.57 \\ 2201+315 & 0.297 & 15.56 & 535 & 9.0 & -1.4 & -9.2 & 31.04 & 27.30 & 30.98 & 1.44 \\ 2251+113 & 0.323 & 16.25 & <63 & 5.1 & -1.2 & -10.2 & 30.71 & <26.44 & 30.45 & $>$ 1.64 \\ 2251+158 & 0.859 & 16.57 & 475 & 6.4 & -0.6 & -12.3 & 31.44 & 28.17 & 30.99 & 1.26 \\ 2302+029 & 1.044 & 16.33$^v$ & ... & 5.2 & -0.3 & -13.2 & 31.66 & ... & 31.26 & ... \\ 2344+092 & 0.672 & 16.08 & 180 & 5.8 & -1.2 & -10.5 & 31.39 & 27.53 & 31.02 & 1.48 \\ $^a$Flux in 0.16-3.5keV bandpass, in \fcgs from Wilkes et al. (1994), assuming $\ax=-0.5$. $^b$Galactic column density in $10^{20}$cm\mtwo. $^c$UV spectral slope ($f_{\nu}\sim\nu^{\auv}$) $^d$UV normalization (see text). $^e$Log rest-frame luminosity in \fnucgs, at 2500\AA. $^f$Log rest-frame luminosity in \fnucgs, at 2keV. $^g$Log rest-frame luminosity in \fnucgs, at 1450\AA.