\begin{table}
\begin{center}
\caption{Comparison of the total ejecta of stellar models of $15\msun$ at $Z=0.02$  
of this work (delay, rapid) with those of P16. Units in $\msun$.} %, CL04 and K06.}
\begin{tabular}{ccccc}
\hline  
\hline  
specie & delay & rapid & P16 (delay) & P16 (rapid) \\ %& CL04      & K06        \\  
\hline  
 C-12   & 1.543E-01 & 1.528E-01 &1.761E-01	 & 1.785E-01	\\% & 2.050E-01 & 6.510E-02  \\ 
 C-13   & 1.000E-03 & 1.001E-03 &9.805E-04	 & 9.813E-04	\\ %& 1.310E-03 & 1.150E-03  \\ 
 N-14   & 4.965E-02 & 4.989E-02 &4.967E-02	 & 4.973E-02	\\% & 5.070E-02 & 6.150E-02  \\ 
 N-15   & 8.457E-05 & 9.629E-05 &5.308E-05	 & 5.457E-05	\\% & 2.190E-05 & 5.970E-05  \\ 
 O-16   & 9.162E-01 & 8.137E-01 &2.986E-01	 & 3.011E-01	\\% & 5.160E-01 & 1.620E-01  \\ 
 O-17   & 6.673E-05 & 6.110E-05 &7.713E-05	 & 7.736E-05	\\% & 1.550E-04 & 8.120E-04  \\ 
 O-18   & 5.592E-03 & 6.444E-03 &4.882E-03	 & 5.004E-03	\\% & 4.190E-03 & 2.540E-03  \\ 
 F-19   & 1.876E-05 & 1.537E-05 &1.518E-05	 & 1.483E-05	\\% & 4.190E-06 & 1.640E-05  \\ 
 Ne-20  & 7.256E-02 & 6.391E-02 &3.151E-02	 & 3.141E-02	\\% & 3.600E-02 & 3.390E-02  \\ 
 Na-23  & 2.597E-03 & 2.215E-03 &1.299E-03	 & 1.301E-03	\\% & 1.380E-03 & 1.060E-03  \\ 
 Mg-24  & 2.842E-02 & 2.523E-02 &1.548E-02	 & 1.505E-02	\\% & 3.390E-02 & 3.790E-02  \\ 
 Al-27  & 2.965E-03 & 2.510E-03 &1.259E-03	 & 1.264E-03	\\% & 1.730E-03 & 2.440E-03  \\ 
 Si-28  & 1.494E-01 & 1.442E-01 &9.677E-02	 & 8.910E-02	\\% & 1.310E-01 & 8.380E-02  \\ 
 S-32   & 5.666E-02 & 6.022E-02 &6.575E-02	 & 6.385E-02	\\% & 6.060E-02 & 3.470E-02  \\ 
 Ar-36  & 5.762E-03 & 7.807E-03 &2.651E-02	 & 2.651E-02	\\% & 9.990E-03 & 4.900E-03  \\ 
 Ca-40  & 1.970E-03 & 4.160E-03 &1.971E-02	 & 1.967E-02	\\% & 8.230E-03 & 4.010E-03  \\ 
 Ti-48  & 8.435E-05 & 2.085E-04 &5.717E-04	 & 4.802E-04	\\% & 2.060E-04 & 1.070E-04  \\ 
 V-51   & 3.294E-05 & 8.094E-05 &1.024E-04	 & 9.875E-05	\\% & 3.350E-05 & 9.960E-06  \\ 
 Cr-52  & 8.825E-04 & 1.280E-03 &3.766E-03	 & 3.564E-03	\\% & 2.040E-03 & 1.270E-03  \\ 
 Mn-55  & 1.092E-03 & 1.853E-03 &2.124E-03	 & 2.159E-03	\\%& 1.360E-03 & 3.800E-04  \\ 
 Fe-56  & 4.306E-02 & 5.395E-02 &1.915E-01	 & 1.681E-01	\\% & 1.150E-01 & 8.520E-02  \\ 
 Co-59  & 4.033E-04 & 3.047E-03 &1.023E-02	 & 1.148E-02	\\% & 2.980E-04 & 9.000E-05  \\ 
 Ni-58  & 1.058E-02 & 6.879E-02 &1.823E-01	 & 1.131E-01	\\% & 5.020E-03 & 1.150E-03  \\ 
 Zn-70  & 1.327E-06 & 8.782E-07 &2.820E-06	 & 2.846E-06	\\% & 9.130E-07 & 5.590E-07  \\ 
 Ge-70  & 5.866E-06 & 7.985E-04 &8.356E-04	 & 3.634E-03	\\% & 1.130E-06 & 8.380E-07  \\ 
 Se-76  & 1.499E-06 & 8.123E-05 &3.013E-05	 & 1.847E-04	\\% & 2.900E-07 &            \\ 
 Kr-80  & 3.052E-07 & 2.279E-05 &1.555E-05	 & 5.410E-05	\\% & 8.460E-08 &            \\ 
 Kr-82  & 1.332E-06 & 1.011E-05 &4.350E-06	 & 3.938E-05	\\% & 2.140E-07 &            \\ 
 Sr-86  & 4.457E-07 & 6.409E-06 &3.747E-06	 & 1.756E-05	\\% & 1.080E-07 &            \\ 
 Sr-87  & 2.883E-07 & 1.397E-06 &6.093E-07	 & 3.172E-06	\\% & 5.650E-08 &            \\ 
 Sr-88  & 5.537E-06 & 1.752E-05 &2.648E-06	 & 4.056E-05	\\%& 7.880E-07 &            \\ 
\hline  
\noalign{\smallskip}          
\hline  
\end{tabular}
\label{compareOtherWork_M15_set1_2}
\end{center}
\end{table}