\begin{table}%t1
      \caption{\label{tab1}Historic summary of~IC~10 distance and reddening determinations.}
   %\centering
\par
       \begin{tabular}{lcll}
            \hline\hline
                       {\rm Mpc}& $E(B-V)$ &{\rm Method}&{\rm Reference}   \\
                      \hline
           1.25&&{\rm HII\  regions}&{\rm de Vaucouleurs\ \&\ Ables\ (\cite{Vaucouleurs1964})}\\
&0.87&{\rm integrated\ UBV}&{\rm de Vaucouleurs\ \&\ Ables\ (\cite{Vaucouleurs1964})}\\
3.0&&{\rm HII\ regions}&{\rm Sandage\ \&\ Tamman (\cite{Sandage1974})}\\
2.0&0.40&{\rm HII\  regions}&{\rm de\  Vaucouleurs\ (\cite{Vaucouleurs1978})}\\
&0.47&{\rm Balmer\ decrement}&{\rm Lequeux\ et\ al.\ (\cite{Lequeux1979})}\\
1.8&&{\rm PN}&{\rm Jacoby\ \&\ Lesser\ (\cite{Jacoby1981})}\\
2.0&&{\rm Tully-Fisher} &{\rm Bottinelli\ et\ al.\ (\cite{Bottinelli1984})}\\
2.2&&{\rm PN} &{\rm Ciardullo\ et\ al.\ (\cite{Ciardullo1989})}\\
&1.85&{\rm H$_\alpha$/radio\ ratio}&{\rm Yang\ \&\ Skillman\ (\cite{Yang1993})}\\
1.04&0.93&{\rm blue\ \&\ red\ stars}&{\rm Karachentsev\ \&\ Tikhonov\ (\cite{Karachentsev1993})}\\
0.95&0.80&{\rm Wolf-Rayet}&{\rm Massey\ \&\ Armandroff\ (\cite{Massey1995})}\\
0.83&0.97&{\rm Cepheids }& {\rm Saha\ et\ al.\ (1996)}\\
0.82&&{\rm IR\ Cepheids}&{\rm Wilson\ et\ al.\ (\cite{Wilson1996})}\\
0.66&1.16&{\rm Cepheids}&{\rm Sakai\ et\ al.\ (\cite{Sakai1999})}\\
0.50&0.85&{\rm TRGB}&{\rm Sakai\ et\ al.\ (\cite{Sakai1999})}\\
0.58&0.99& $V$, $R$, $I$&{\rm Tikhonov\ (\cite{Tikhonov1999})}\\
0.59&1.05& $J$, $H$, $K$&{\rm Borisova\ et\ al.\ (2000)}\\
&0.77&{\rm spectra\ HII\ reg.}&{\rm Richer\ et\ al.\ (\cite{Richer2001})}\\
0.98&&{\rm TRGB}&{\rm Hunter\ (\cite{Hunter2001})}\\
0.74&{\rm Variable}&{\rm C stars}&{\rm This paper}\\
                      \hline
         \end{tabular}   \end{table}