\begin{table}%tB.1
   {%\centering
\par
      \caption{Recent galactic supernova record.        \label{histrec}}
      $$
         \begin{array}{p{0.3\linewidth}lcccc}
            \hline\hline
            \noalign{\smallskip}
            Name            & {\rm Year}  & {\rm Distance} & l & b & {\rm Type} \\
                            &       & ({\rm kpc})    &   &   &      \\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            Lupus (SN 1006) & 1006  & 2.2  & 327.57 & 14.57 & \rm{Ia} \\
            Crab            & 1054  & 2.0  & 184.55 & -5.79 & \rm{II} \\
            3C 58 (SN 1181)  & 1181  & 2.6  & 130.73 &  3.07 & \rm{II} \\
            Tycho           & 1572  & 2.4  & 120.09 &  1.42 & \rm{Ia}^a \\
            Kepler          & 1604  & 4.2  &   4.53 &  6.82 & \rm{Ib/II}^b \\
            Cas A           & 1680  & 2.92 & 111.73 & -2.13 & \rm{Ib}  \\
            \noalign{\smallskip}
            \hline
         \end{array}
      $$}
     {\small \hspace*{-1mm}$^a$  Studies of X-ray emission from Tycho's shocked ejecta show the SNR was created by a type Ia SN (Hwang et~al. 1998; Badenes et~al.   2003, 2005).\\
        $^b$  The uncertainty of Kepler's SN Type was reviewed by 
              \citet{2005ASPC..342..416B}}.
   \end{table}