\begin{table}%t3
\par
%\centering
\par
\caption{Eleven stars towards 3C~434.1 with observed reddenings
 that are consistent
with that observed toward the SNR/SWB ($E(B-V)=2.1$~mag), i.e. 
$1.7~{\rm mag} \leq  E(B-V) \leq 2.5$~mag. The uncertainty in the assigned spectral type is on average plus or
minus one sub-type (e.g. an O5 is O4-O6 within uncertainty). Distances
are calculated using reddening law $R_{V}=A_{V}/E(B-V)=3.1$. All distances
have an uncertainty of $\pm $30\%\label{stars}.}
\begin{tabular}{cccccccc}
\hline\hline
Star&
$B-V$&
$U-B$&
$m_{V}$&
Assigned&
$M_{V}$&
$d$ (kpc) &
$E(B-V)$\\
&
($\pm $13\%)&
($\pm $20\%)&
($\pm $0.07 mag)&
MK Type&
($\pm $0.3 mag)&
($\pm $30\%)&
($\pm $0.23 mag)\\
\hline
1&
1.45&
0.06&
14.95&
B0 &
$-$4&
5.1&
1.74\\
2&
1.75&
0.11&
13.55&
O5&
$-$5.7&
3.7&
2.08\\
3&
1.72&
0.44&
13.92&
B2&
$-$2.47&
1.2&
1.95\\
4&
1.46&
0.02&
15.05&
B0&
$-$4&
5.2&
1.77\\
5&
1.62&
0.40&
14.10&
B2&
$-$2.47&
1.0&
1.84\\
6&
1.66&
0.21&
14.04&
B0&
$-$3.9&
2.4&
1.95\\
7&
1.86&
$-$0.01&
14.33&
O4&
$-$6.0&
4.9&
2.22\\
8&
1.61&
0.22&
14.33&
B1&
$-$3.7&
2.7&
1.89\\
9&
1.56&
0.31&
13.78&
B2&
$-$2.47&
1.4&
1.80\\
10&
1.36&
0.00&
14.57&
B0&
$-$4&
4.8&
1.66\\
11&
1.40&
0.14&
14.70&
B1&
$-$3.2&
3.5&
1.66\\
\hline
\end{tabular}
\end{table}