\begin{table}%t4
\caption{\label{masslimits}Mass ranges for various supernova progenitors, supernova types, and compact remnants at different metallicities (in ${M}_\odot$).}
%\centerline
 {
\begin{tabular}{c c c c c c c c c c c}
\hline\hline 
Z & SG & WNL & WNE & WC & WO & Type II & Type Ib & Type Ic & NS & BH  \\
\hline
\multicolumn{11}{c}{\textbf{Reference case}}\\
$0.004$ & $8 {-} 32$ & $32 {-} 54$ & $-$ & $54 {-} 59;114 {-} 120$ & $59 {-} 114$ & 
$8 {-} 54$ & $54 {-} 59$ & $59 {-} 120$ & $8 {-} 29$ & $29 {-} 120$\\
$0.008$ & $8 {-} 25$ & $25 {-} 30 $ & $ - $ &$30 {-} 41; 113 {-} 120$ & $41 {-} 113$ & $8 {-} 30$ &  --  & $30 {-} 120$ & $8 {-} 29$ & $29 {-} 120$\\
$0.020$ & $8 {-} 23$ & $23 {-} 26$ & $26 {-} 29$ & $29 {-} 120$ & $-$ & $8 {-} 25$ & 
$25 {-} 39$ & $39 {-} 120$ & $8 {-} 35$ & $35 {-} 120$\\
$0.040$ & $8 {-} 20$ & $20 {-} 20.5$ & $20.5 {-} 22$ & $22 {-} 120$ & $-$ & $8 {-} 20.5$ & $20.5 {-} 25$ & $25 {-} 120$ & $8 {-} 120$ & --\textsuperscript{1}\\
\hline  
\end{tabular}}
\smallskip
(1) At this metallicity, only the $40~  {M}_\odot$ model produces a BH.
Note: The SN type is given for $m^{\rm min}_{\rm H}=0$, $m^{\rm min}_{\rm He}=0.6$ and supposing that an SN~occurs even when a BH is formed (see text for more details).
\end{table}