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\begin{table*} %Table I
\caption[]{ Ultraviolet and $Vuvby$ photometry for the 
completely-surveyed region indicated in Fig.~2 }
\begin{flushleft}
\begin{tabular}{lrrrrrrrll}
\hline \noalign{\vskip 0.2cm} 
WT & HD~~~ & $y/V$ & $(b-y)$ & $m_1$~~ & $c_1$~~ & n & $m_{195}$ & error &
Comments \\ 
\noalign{\vskip 0.2cm} \hline \noalign{\vskip 0.2cm} 
002 & 207153 & 9.23 & 0.107 & 0.175 & 0.905 & 3 & 9.00 & 0.14 & ADS 15323ABC \\
003 & 206497 & 8.47 & 0.119 & 0.197 & 0.861 & 3 & 8.46 & 0.11 & ADS 15243AB \\ 
004 & 206648 & 8.99 & 0.020 & 0.179 & 0.999 & 2 & 9.00 & 0.17 & \\ 
005 & 206546 & 6.23 & 0.144 & 0.246 & 0.836 & 2 & 7.47 & 0.03 & \\ 
006 & 205306 & 6.74 & 0.318 & 0.159 & 0.454 & 2 &      &      & confused with
No. 7 on VWFC \\ 
    &        & $^{0.004}$ & $^{0.008}$ & $^{0.016}$ & $^{0.021}$ & & & & \\

007 & 205289 & 5.70 & 0.278 & 0.143 & 0.447 & 2 &      &      & confused with
No. 6 on VWFC \\ 
008 & 205637 & 4.53 & $-$0.069 & 0.069 & 0.272 & 2 & 2.75 &      & Be star,
var? \\ 
009 & 205406 & 8.30 & 0.035 & 0.163 & 0.984 & 2 & 7.97 & 0.09 & ADS 15107AB \\ 
010a & 204779 & 7.14 & 0.216 & 0.159 & 0.686 & 2 &      &      & $b$; ADS
15046AB  \\ 
010b & 204763 & 9.46 & 0.178 & 0.150 & 0.876 & 2 &      &      & $b$ \\ 
     &        & $^{0.014}$ & $^{0.020}$ & $^{0.031}$ & $^{0.013}$ & & & & \\

011 & 204436 & 8.93 & 0.069 & 0.153 & 1.062 & 2 & 9.45 & 0.18 & IDS 21235
$-$1959AB \\ 
012 & 204577 & 6.57 & 0.270 & 0.153 & 0.639 & 2 & 8.96 & 0.12 & \\ 
013 & 204043 & 8.76 & 0.132 & 0.125 & 0.953 & 2 & 8.68 & 0.09 & ADS 14968 ABC
\\ 
    &        & $^{0.002}$ & $^{0.004}$ & $^{0.004}$ & $^{0.025}$ & & & & \\
\noalign{\vskip -0.2cm}
014 & 203209 & 8.92 & $-$0.006 & 0.119 & 0.941 & 2 & 7.77 & 0.06 & \\ 
    &        & $^{0.018}$ & $^{0.027}$ & $^{0.030}$ & $^{0.013}$ & & & & \\
\noalign{\vskip -0.2cm}
015 & 204347 & 8.85 & 0.065 & 0.180 & 1.032 & 2 & 8.43 & 0.10 & IDS 21228
$-$1742AB \\ 
\noalign{\vskip 0.2cm}
016 & 202671 & 5.40 & $-$0.043 & 0.095 & 0.534 & 2 & 3.88 &      & \\ 
017 & 202723 & 7.07 & 0.214 & 0.177 & 0.751 & 2 & 8.54 & 0.12 & \\ 
018 & 202939 & 9.07 & 0.074 & 0.098 & 1.194 & 2 & 8.87 & 0.10 & \\ 
019 & 203311 & 7.45 & 0.389 & 0.175 & 0.438 & 2 &      &      & LTT 8486 \\ 
020 & 203706 & 8.69 & 0.018 & 0.101 & 0.876 & 2 & 7.61 & 0.06 & \\ 
\noalign{\vskip 0.2cm}
021 & 202669 & 8.41 & 0.302 & 0.161 & 0.485 & 2 &      &      & \\ 
    &        & $^{0.014}$ & $^{0.009}$ & $^{0.016}$ & $^{0.024}$ & & & & \\
\noalign{\vskip -0.2cm}
022 & 201057 & 6.19 & $-$0.020 & 0.145 & 0.927 & 2 & 5.52 & 0.06 & \\ 
023 & 200761 & 4.08 & $-$0.008 & 0.170 & 1.051 & 2 & 3.92 &      & \\ 
024 & 201146 & 8.11 & 0.122 & 0.176 & 1.015 & 2 & 8.95 & 0.10 & \\ 
025 & 201462 & 7.54 & 0.209 & 0.150 & 0.693 & 2 & 8.93 & 0.11 & \\ 
\noalign{\vskip 0.2cm}
026 &        & 11.81 & 0.333 & 0.183 & 0.427 & 4 &     &      & $e$; $\dag$
\\ 
    &        & $^{0.018}$ & $^{0.010}$ & $^{0.005}$ & $^{0.044}$ & & & & \\
\noalign{\vskip -0.2cm}
027 & 202291 & 8.19 & 0.131 & 0.176 & 0.931 & 2 & 8.55 & 0.10 & \\ 
    &        & $^{0.023}$ & $^{0.013}$ & $^{0.021}$ & $^{0.006}$ & & & & \\
\noalign{\vskip -0.2cm}
028 & 202495 & 8.10 & $-$0.013 & 0.094 & 0.742 & 2 & 6.73 & 0.05 & \\ 
029 & 202317 & 9.02 & 0.006 & 0.173 & 1.021 & 2 & 8.81 & 0.14 & \\ 
030a & 201707 & 6.46 & 0.186 & 0.177 & 0.893 & 3 &      &      & see text \\ 
     &        & $^{0.021}$ & $^{0.006}$ & $^{0.003}$ & $^{0.010}$ & & & & \\

030b & 201768 & 7.65 & 0.159 & 0.171 & 0.849 & 2 &      &      & \\ 
032 & 209278 & 6.38 & 0.280 & 0.150 & 0.837 & 2 & 6.86 & 0.04 & ADS 15562AB;
comp. A is EB (DX Aqr) \\ 
034 & 208979 & 7.87 & 0.185 & 0.160 & 0.779 & 2 &      &      & \\ 
035 & 208482 & 6.76 & 0.043 & 0.170 & 1.059 & 2 & 6.71 & 0.04 & \\ 
037 & 208087 & 8.73 & 0.002 & 0.133 & 0.948 & 2 & 7.60 & 0.07 & \\ 
\noalign{\vskip 0.2cm}
038 & 207760 & 6.19 & 0.234 & 0.157 & 0.678 & 2 & 7.68 & 0.06 & \\ 
039 & 207439 & 7.57 & 0.167 & 0.172 & 0.787 & 2 & 8.26 & 0.07 & \\ 
041 & 207208 & 7.40 & 0.150 & 0.159 & 0.875 & 2 & 8.35 & 0.07 & \\ 
042 & 207188 & 7.63 & $-$0.034 & 0.138 & 0.532 & 2 & 6.41 & 0.05 & ADS 15325AB,
var \\ 
    &        & $^{0.021}$ & $^{0.001}$ & $^{0.003}$ & $^{0.025}$ & & & & \\
\noalign{\vskip -0.2cm}
043 & 206144 & 9.40 & $-$0.042 & 0.053 & 0.131 & 2 & 6.96 & 0.04 & \\ 
\noalign{\vskip 0.2cm}
044 & 207098 & 2.87 & 0.185 & 0.185 & 0.744 &   & 4.52 &      & ADS 15314A, var
SB; $Vuvby$ from CDS \\ 
045 & 206703 & 7.52 & 0.102 & 0.216 & 0.868 & 2 & 8.09 & 0.07 & \\ 
046 & 206088 & 3.68 & 0.176 & 0.268 & 0.841 & 2 & 5.77 & 0.06 & SB? \\ 
047 & 207438 & 8.07 & 0.080 & 0.175 & 0.993 & 2 & 8.20 & 0.07 & \\ 
048 & 206677 & 5.95 & 0.136 & 0.182 & 0.843 & 2 & 6.64 & 0.05 & \\ 
\noalign{\vskip 0.2cm} \hline
\end{tabular}
\end{flushleft}
\end{table*}
\setcounter{table}{0}
\begin{table*}
\caption[]{ (continued) } 
\begin{flushleft}
\begin{tabular}{lrrrrrrrll}
\hline \noalign{\vskip 0.2cm} 
WT & HD~~~ & $y/V$ & $(b-y)$ & $m_1$~~ & $c_1$~~ & n & $m_{195}$ & error &
Comments \\ 
\noalign{\vskip 0.2cm} \hline \noalign{\vskip 0.2cm} 
049 & 206561 & 5.89 & 0.166 & 0.166 & 0.919 & 2 & 7.07 & 0.05 & \\ 
050 & 206288 & 7.18 & 0.223 & 0.184 & 0.710 & 2 & 9.20 & 0.13 & ADS 15216A
(comp.~B at 16$\arcsec$; $\delta m\simeq$4.3) \\ 
051 & 206301 & 5.15 & 0.425 & 0.197 & 0.397 & 4 &      &      & \\ 
052 & 205828 & 8.30 & $-$0.004 & 0.100 & 0.846 & 2 & 7.07 & 0.06 & \\ 
053 & 205361 & 9.78 & 0.271 & 0.133 & 0.602 & 2 & 9.30 & 0.15 & $c$ \\ 
\noalign{\vskip 0.2cm}
054 & 204220 & 7.12 & $-$0.028 & 0.105 & 0.542 & 2 & 5.64 & 0.08 & \\ 
055 & 203928 & 9.14 & 0.048 & 0.177 & 1.014 & 2 & 8.43 & 0.09 & \\ 
056 & 203893 & 6.87 & 0.038 & 0.134 & 1.157 & 2 & 6.80 & 0.05 & \\ 
057 & 202990 & 7.04 & 0.033 & 0.137 & 1.158 & 2 & 6.90 & 0.04 & \\ 
058 & 203054 & 7.24 & $-$0.026 & 0.103 & 0.609 & 2 & 5.71 & 0.06$^a$ \\ 
\noalign{\vskip 0.2cm}
059 & 202929 & 6.89 & 0.138 & 0.163 & 1.024 & 2 & 7.80 & 0.07 & IDS 21139
$-$1328AB \\ 
060 & 203705 & 5.49 & 0.177 & 0.181 & 0.789 & 2 & 6.81 & 0.04 & IDS 21187
$-$1318A var? \\ 
061 & 203617 & 8.01 & $-$0.029 & 0.070 & 0.333 & 2 & 5.91 & 0.06$^a$ & \\ 
062 & 203769 & 8.29 & 0.067 & 0.138 & 1.076 & 3 & 8.08 & 0.06 & \\ 
065 & 202606 & 6.42 & 0.020 & 0.158 & 1.145 & 2 & 6.26 & 0.05 & \\ 
\noalign{\vskip 0.2cm}
066 & 206797 & 7.35 & 0.255 & 0.161 & 0.671 & 3 & 8.66 & 0.12$^a$ & \\ 
067 & 202701 & 8.76 & 0.328 & 0.152 & 0.509 & 2 & 9.29 & 0.09 & $d$; probable
candidate \\ 
068 & 205003 & 9.11 & 0.034 & 0.172 & 0.995 & 2 & 8.53 & 0.11 & \\ 
069 & 205527 & 7.89 & 0.263 & 0.149 & 0.532 & 2 & 9.67 & 0.19 & \\ 
070 & 205674 & 7.18 & 0.270 & 0.153 & 0.455 & 2 &      &      & \\ 
\noalign{\vskip 0.2cm}
071 & 204762 & 8.40 & 0.168 & 0.189 & 0.822 & 2 &      &      & IDS 21257
$-$1742AB \\ 
072 & 205132 & 7.17 & 0.306 & 0.153 & 0.453 & 2 & 9.41 & 0.16 & ADS 15080AB \\ 
073 & 204957 & 8.93 & 0.196 & 0.142 & 0.704 & 2 & 9.29 & 0.17 & \\ 
075 & 202149 & 6.78 & $-$0.026 & 0.117 & 0.789 & 2 & 5.53 & 0.06$^a$ & \\ 
076 &        &      &             &       &             &   &      &      & 
Saturn Nebula, NGC 7009 \\
\noalign{\vskip 0.2cm}
077 & 200414 & 8.00 & $-$0.014 & 0.107 & 0.948 & 2 & 6.83 & 0.05 & \\ 
078 & 201202 & 8.52 & 0.048 & 0.167 & 1.031 & 2 & 8.27 & 0.05 & mult \\ 
079 & 200582 & 7.22 & 0.150 & 0.196 & 0.869 & 2 &      &      & hidden by No.
23 \\ 
080 & 200171 & 7.86 & 0.145 & 0.141 & 1.020 & 2 & 8.55 & 0.09 & \\ 
081 & 199443 & 5.88 & 0.088 & 0.221 & 0.928 & 2 & 6.55 & 0.05 & \\ 
\noalign{\vskip 0.2cm}
082 & 199295 & 8.23 & 0.121 & 0.167 & 0.983 & 2 &      &      & \\ 
083 & 199047 & 7.87 & 0.197 & 0.158 & 0.732 & 3 & 8.54 & 0.07 & \\ 
084 & 198528 & 7.64 & 0.201 & 0.166 & 0.800 & 2 & 8.76 & 0.13 & var? \\ 
    &        & $^{0.034}$ & $^{0.006}$ & $^{0.006}$ & $^{0.003}$ & & & & \\
\noalign{\vskip -0.2cm}
085 & 199703 & 8.91 & 0.036 & 0.067 & 0.768 & 2 & 7.69 & 0.06 & \\ 
086 & 199897 & 7.94 & 0.231 & 0.154 & 0.597 & 2 &      &      & \\ 
\noalign{\vskip 0.2cm}
087 & 200157 & 7.02 & 0.295 & 0.147 & 0.509 & 2 & 9.21 & 0.26 & \\ 
092 & 199747 & 8.23 & 0.132 & 0.180 & 0.953 & 2 & 8.60 & 0.07 & \\ 
094 & 198648 & 7.29 & $-$0.016 & 0.117 & 0.769 & 2 & 6.22 & 0.05 & \\ 
095 & 199603 & 6.0: & 0.142 & 0.196 & 0.910 & 2 & 6.90 & 0.06 & EB (DV Aqr) \\ 
    &        & $^{0.096}$ & $^{0.001}$ & $^{0.008}$ & $^{0.022}$ & & & & \\
\noalign{\vskip -0.2cm}
096 &       & 13.00 & $-$0.116 & 0.086 & $-$0.161 & 4 &      &      &
LS~IV$-14\degr116$, sdO He-rich $\S$ \\ 
\noalign{\vskip 0.2cm}
097 & 199828 & 6.62 & 0.106 & 0.169 & 0.981 & 3 & 7.19 & 0.06 & \\ 
100 & 204238 & 9.59 & 0.265 & 0.134 & 0.528 & 2 &      &      & \\ 
101 & 203191 & 9.38 & 0.101 & 0.190 & 0.940 & 2 &      &      & \\ 
103 & 199791 & 8.67 & 0.212 & 0.149 & 0.810 & 2 & 9.54 & 0.17 & \\ 
105 & 200415 & 9.82 & 0.158 & 0.133 & 0.923 & 2 &      &      & \\ 
\noalign{\vskip 0.2cm} \hline
\end{tabular}
\end{flushleft}
\end{table*}
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\begin{table*}
\caption[]{ (concluded) }
\begin{flushleft}
\begin{tabular}{lrrrrrrrll}
\hline \noalign{\vskip 0.2cm} 
WT & HD~~~ & $y/V$ & $(b-y)$ & $m_1$~~ & $c_1$~~ & n & $m_{195}$ & error &
Comments \\ 
\noalign{\vskip 0.2cm} \hline \noalign{\vskip 0.2cm} 
107 & 200604 & 9.94 & 0.051 & 0.130 & 1.001 & 2 &      &      & \\ 
109 & 198041 & 6.99 & 0.286 & 0.195 & 0.706 & 2 &      &      & \\ 
112 & 199945 & 10.06 & 0.030 & 0.140 & 0.998 & 2 &     &      & \\ 
113 & 200342 & 8.43 & 0.017 & 0.168 & 1.015 & 2 & 8.01 & 0.07 & \\ 
114 & 200950 & 8.41 & 0.055 & 0.168 & 1.053 & 2 & 8.36 & 0.11 & IDS 21015
$-$1305AB \\ 
\noalign{\vskip 0.2cm}
115 & 201069 & 9.73 & 0.268 & 0.144 & 0.611 & 2 &      &      & \\ 
116 & 201162 & 8.04 & 0.155 & 0.174 & 0.801 & 2 & 8.81 & 0.12 & \\ 
124 & 198774 & 9.48 & 0.081 & 0.107 & 0.910 & 5 & 8.81 & 0.31 & ADS 14388AB \\ 
137 & 205705 & 7.45 & $-$0.025 & 0.095 & 0.683 & 2 &      &      & hidden by
No. 8 \\ 
218 & 200182 & 10.18 & 0.075 & 0.159 & 1.023 & 2 &     &      & \\ 
\noalign{\vskip 0.2cm}
221 & 198601 & 9.38 & 0.348 & 0.146 & 0.463 & 2 &      &      & ADS 14365AB \\ 
222 & 198575 & 10.73 & 0.069 & 0.160 & 1.054 & 2 &     &      & \\ 
225a &       & 9.82 & 0.643 & 0.303 & 0.425 & 2 &     &      &
BD$-17^{\circ}6173$; confused with No. 23 \\ 
     &       & $^{0.012}$ & $^{0.006}$ & $^{0.002}$ & $^{0.025}$ & & & & \\ 
\noalign{\vskip -0.2cm}
225b & 200821 & 9.57 & 0.325 & 0.130 & 0.589 & 2 &     &      & confused with
No. 23 \\ 
226 & 200880 & 9.46 & 0.180 & 0.161 & 0.777 & 2 &     &      & confused with
No. 24 \\ 
\noalign{\vskip 0.2cm}
227 & 205706 & 8.03 & 0.286 & 0.149 & 0.537 & 2 &     &      & \\ 
228 & 206496 & 9.44 & 0.275 & 0.142 & 0.530 & 2 &      &      & \\ 
232 & 205722 & 9.68 & 0.298 & 0.135 & 0.548 & 2 &      &      & hidden by No. 8
\\ 
234 & 205363 & 9.43 & 0.059 & 0.179 & 0.975 & 2 &      &      & hidden by No. 8
\\ 
\noalign{\vskip 0.2cm} \hline
\end{tabular}
\end{flushleft}
{\em Notes:} in this table and subsequent ones, n is the number of observations.
The error given to $m_{195}$ magnitudes is twice the one derived by the {\sc
capella} software. \\ 
	\\
$\S$ see Viton et al. (1991) \\
$\dag$ see Fig.~3 for finding chart \\
$a$ uncertain error bar \\
$b$ VWFC image elongated, both HD204779 and 204763 may contribute \\
$c$ {\sc coravel} data indicate possibly variable velocity \\
$d$ {\sc coravel} data indicate variable velocity \\
$e$ UV detection in fact due to WT026bis (Fig.~3, $V\simeq 12.5$) which 
preliminary spectroscopy and CCD photometry has shown is \phantom{xx}a sdO star
probably in binary association with a cooler companion 
\end{table*}
\vfill
\end{document}
