*****E140 F2 and R  FROM LARRY'S THESIS**************                           
 ---Taken from THESIS ALL  in Whitlow's archives----                            
 ---Tables 4.4---                                                               
                                                                                
                                                                                
\hidetab\Rtab={E140 deuterium and iron structure functions}{Shown are           
the E140 deuterium and iron structure functions.  Uncertainties are             
fractional in \Ft\ and absolute in \R.  Not shown are uncertainties due         
to radiative corrections, which are less than \z.5\% for \Ft\ (see              
Equation 5.39) and \z.025 for \R.  Normalization uncertainties in \Ft\          
are given in Table 3.2.  In Chapter 5, more precise values of \Ft\ are          
extracted directly from the cross sections using a model for \R\xq.}            
{\vskip-.8cm\tablewidth=5in\columns=4\begintable                                
           \|                   \|                 \|\nr\msp\dbl                
\B\x\ \B\B\B\Q\|\p\Ft\sz\dFST\sz\dFSS\|\p\R\sz\dRST\sz\dRSS\|\Xdf \dbl          
Deuterium  \|                   \|                  \|      \lnp                
.20\b\p1.0 \| .2964\b.010\b.010 \| .370\b.049\b.005 \| \p.7 \nr                 
.20\b\p1.5 \| .2996\b.011\b.010 \| .280\b.050\b.005 \|  1.8 \nr                 
.20\b\p2.5 \| .2907\b.017\b.010 \| .105\b.051\b.005 \| \p.0 \nr                 
.20\b\p5.0 \| .3034\b.025\b.010 \| .233\b.065\b.011 \| \p.2 \nr                 
.35\b\p1.5 \| .2331\b.012\b.010 \| .308\b.062\b.005 \| \p.3 \nr                 
.35\b\p2.5 \| .2198\b.010\b.010 \| .159\b.040\b.005 \| \p.6 \nr                 
.35\b\p5.0 \| .2081\b.013\b.010 \| .126\b.045\b.005 \| \p.4 \nr                 
.50\b\p2.5 \| .1412\b.007\b.010 \| .202\b.029\b.005 \| \p.8 \nr                 
.50\b\p5.0 \| .1174\b.009\b.010 \| .100\b.033\b.006 \| \p.8 \nr                 
.50\b\p7.5 \| .1109\b.022\b.010 \| .152\b.065\b.005 \| \y$-$\nr                 
.50\b 10.0 \| .1019\b.019\b.010 \| .045\b.044\b.008 \| \p.0 \lnp                
\Ione      \|                   \|                  \|      \lnp                
.20\b\p1.0 \| .2990\b.010\b.009 \| .284\b.045\b.005 \|  1.8 \nr                 
.20\b\p1.5 \| .3002\b.011\b.009 \| .159\b.042\b.005 \| \p.5 \nr                 
.20\b\p2.5 \| .3112\b.017\b.010 \| .254\b.062\b.005 \|  1.5 \nr                 
.35\b\p1.5 \| .2360\b.012\b.009 \| .356\b.069\b.005 \|  1.2 \nr                 
.35\b\p2.5 \| .2239\b.010\b.009 \| .260\b.051\b.005 \|  1.1 \nr                 
.35\b\p5.0 \| .2063\b.014\b.009 \| .151\b.050\b.005 \| \p.1 \nr                 
.50\b\p2.5 \| .1325\b.008\b.009 \| .220\b.033\b.005 \| \p.6 \nr                 
.50\b\p5.0 \| .1100\b.014\b.009 \| .078\b.048\b.006 \| \p.1 \lnp                
\Itwo      \|                   \|                  \|      \lnp                
.20\b\p1.0 \| .2968\b.010\b.010 \| .340\b.048\b.005 \| \p.2 \nr                 
.50\b\p2.5 \| .1310\b.022\b.009 \| .218\b.056\b.006 \| \y$-$\lnp                
Gold       \|                   \|                  \|      \lnp                
.20\b\p1.0 \| .3024\b.010\b.010 \| .339\b.046\b.005 \| \p.4 \dbl                
\msp\endtable}