\begin{table}
\caption{Spectroscopically confirmed Wolf-Rayet stars in IC~10 from
catalogues of Massey et~al. (\cite{Massey92}), Royer et~al. (\cite{Royer01}) and Massey \& Holmes (\cite{Massey02}).
Previous photometric and spectroscopic spectral types are taken from the 
above references, plus Massey \& Armandroff (\cite{Armandroff95}). Broad-band $V$ and narrow-band $v$ 
magnitudes are taken from archival WFPC2 imaging and Royer
et~al. (their c1), respectively, except those in parenthesis, which are 
obtained from  GMOS spectrophotometry. See text for determination of 
absolute magnitudes. Line equivalent widths ($W_{\lambda}$) and $FWHM$ refer 
to He~{\sc ii} $\lambda$4686 for WN stars, and C~{\sc iii}
$\lambda\lambda$4647--50/He~{\sc ii} 
$\lambda$4686 plus 
C~{\sc iv} $\lambda\lambda$5801--12 for WC stars.}
\label{wrcat}
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\par
\includegraphics[angle=90,clip]{tab1.eps}
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\par
\end{table}