\begin{table}%ta.1
\caption{\label{GBother} The other Galactic Bulge PNe observed with Spitzer/IRS (program $\#$3633).} %\centerline
 {\small   
\begin{tabular}{r l c c c c c c} 
\hline  \hline \noalign{\smallskip}
IRAS name    & PN name  & RA  & Dec  &  Spectral type$^a$  & Optical diameter$^{{e}}$ & Distance from GC & Dust type \\ 
 &          & J2000.0    & J2000.0   &  & (arcsec) & ($\degr$)  &   \\
\hline
17230$-$3459   & H 1-12   & 17 26 24.3 & --35 01 41 & unknown  & 6.8 & 7.33 & O \\
17385$-$2211   & M 3-13   & 17 41 36.6 & --22 13 03 & none$^b$    & 0.0 & 6.78 & O \\
17427$-$3402   & H 1-32   & 17 46 06.3 & --34 03 45 & none$^b$    & $<$5.0 & 5.13 & O \\
17459$-$3421   & H 1-35   & 17 49 14.0 & --34 22 52 & none$^c$    & 2.0 & 5.50 & O \\
17585$-$2825   & M 2-23   & 18 01 42.7 & --28 25 44 & none$^d$    & 8.5 & 3.56 & O \\
\hline                
\end{tabular}}
\medskip
$^a$ None -- neither [WC]~nor {\it wels}; $^{{b}}$~G\'orny et~al. (2004); $^c$~\cite{Wang2007}; $^d$~G\'orny et~al. (2008); $^e$~Strasbourg-ESO Catalogue of Galactic Planetary Nebulae \cite{Acker1992}, 0.0 -- PN is a point-like source.
\end{table}