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\begin{document}
\def\ub{\underbar{~}}
\def\sec{$^{\prime\prime}$}
\def\etal{{\it et al.}}
\begin{deluxetable}{lclcl}
\tablenum{3}
\tablecolumns{5}
%\tablewidth{285pt}
%\tablewidth{0pc}
\tablecaption{Uncertain Redshifts in the HDF}
%\scriptsize
%
\tablehead{
\colhead{Name}  & 
\colhead{$z$ \tablenotemark{a}} &
\colhead{$Q_z$ \tablenotemark{b}} &
\colhead{$r_{1/2}$ \tablenotemark{c}} & 
\colhead{Ref \tablenotemark{d}}  \\  
%
\colhead{} & 
\colhead{} & 
\colhead{} & 
\colhead{(\sec)} &
\colhead{}
}

\startdata

hd4\ub0259\ub1947 & 3.30     &  2x &   0.49  &  L4-553*\\                      
hd4\ub1076\ub1847 & 2.15     &  2  &   0.21  &  L4-544\\                       
hd4\ub0818\ub1037 & 2.04     &  2x &   0.29  &  L4-252\\                       
hd2\ub1881\ub0374 & 2.58     &  2x &   0.31  &  L2-42\\                        
hd4\ub1994\ub1406 & 3.63     &  1x &   0.27  &  L4-371\\                       
hd4\ub1486\ub0880 & 2.47     &  2  &   0.36  &  L4-209\\                       
hd2\ub0853\ub0319 & 3.35     &  1x &   0.68  &  L2-28\\                        
hd4\ub1341\ub0299 & 2.31     &  2x &   0.25  &  L4-14/M4-85.2/SC4-01 \\        
hd2\ub1739\ub1258 & 2.72     &  2x &   0.80  &  L2 -291 \\                    
hd2\ub1410\ub1282 & 3.37     &  1x &   0.30  &  L2-301\\                       
hd3\ub1455\ub0430 & 2.64     &  2  &   0.17  &  L3-38/SC3-01\\                 
hd2\ub0743\ub1844 & 2.39     &  1x &   0.33  &  L2-501/C2P4\\                  

\enddata

\tablenotetext{a}{Tentative redshift.}
\tablenotetext{b}{Redshift quality.  
1=SNR too low to discern features; 2=real features
detected but redshift uncertain.  An ``x'' indicates the redshift was
derived from cross-correlating the spectrum with that of NGC~1741 (or,
in the case of hd4\ub0818\ub1037, with that of the combined spectrum
shown in Fig. 3).}
\tablenotetext{c}{Half-light radius in arcsec measured from the
``drizzled'' images.}
\tablenotetext{d} {Other published candidate lists in which object
appears: C=Clements \& Couch (1996); L=Lanzetta \etal\ (1996); M=Madau
\etal\ (1996); S=Steidel \etal\ (1996b).  For Lanzetta \etal\, a *
indicates that the predicted redshift was $z>2.2$.}

\end{deluxetable}
\end{document}