\begin{table}%t2
\caption{\label{tab:position}\mbox{X-ray} position (equatorial and Galactic) of the \mbox{X-ray} counterparts to the 17 sources studied with \swift/XRT.}
%\centerline
 {\small \begin{tabular}{lllcll} 
\hline\hline             
Name & RA & Dec & Error & $l$ & $b$ \\
(IGR)  & (J2000) & (J2000) & (\arcsec) & (\degr) & (\degr) \\ 
\hline
J03184$-$0014$^\dagger$ & 03$^{\rm h}$18$^{\rm m}$17.6$^{\rm s}$& $-$00\degr 17\arcmin 48.1\arcsec & 5.7 & 181.8112 & $-$45.7082 \\
J03532$-$6829 & 03$^{\rm h}$52$^{\rm m}$57.4$^{s}$ & $-$68\degr 31\arcmin 18.0\arcsec & 3.5 & 282.8102 & $-$40.7968 \\
J05319$-$6601$^\dagger$ & 05$^{\rm h}$31$^{\rm m}$52.6$^{\rm s}$& $-$65\degr 59\arcmin 40.2\arcsec & 4.7 & 275.9037 & $-$32.6650  \\
J05346$-$5759& 05$^{\rm h}$34$^{\rm m}$50.5$^{\rm s}$ & $-$58\degr 01\arcmin 39.3\arcsec & 3.5 & 266.4230 & $-$32.7788   \\
J09025$-$6814$^\dagger$ & 09$^{\rm h}$02$^{\rm m}$39.4 & $-$68\degr 13\arcmin 38.7\arcsec & 4.8 &  284.1738 & $-$14.1567 \\
J10101$-$5654$^\star$ & 10$^{\rm h}$10$^{\rm m}$11.9$^{\rm s}$ & $-$56\degr 55\arcmin 31.6\arcsec & 4.3 & 282.2567 & $-$0.6719  \\
J13000+2529$^\dagger$ & 12$^{\rm h}$59$^{\rm m}$55.0$^{\rm s}$ & +25\degr 28\arcmin 08.8\arcsec & 6.9 & 352.2816 & +87.4774 \\
J13020$-$6359 & 13$^{\rm h}$01$^{\rm m}$59.2$^{\rm s}$ & $-$63\degr 58\arcmin 06.0\arcsec & 3.5 & 304.0891 & $-$1.1202 \\
J15161$-$3827$^\ddagger$ \#1 & 15$^{\rm h}$15$^{\rm m}$59.3$^{\rm s}$ & $-$38\degr 25\arcmin 48.3\arcsec & 4.3 & 331.6935 & +16.2381 \\
 \#2  & 15$^{\rm h}$16$^{\rm m}$ 29.6$^{\rm s}$ & $-$38\degr 26\arcmin 56.5\arcsec & 4.6 & 331.7689 & +16.1681\\
 \#3$^\dagger$      & 15$^{\rm h}$16$^{\rm m}$12.7$^{\rm s}$ & $-$38\degr 31\arcmin 02.4\arcsec & 4.7 & 331.6819 & +16.1411  \\
 \#4$^\dagger$      & 15$^{\rm h}$15$^{\rm m}$45.8$^{\rm s}$ & $-$38\degr 27\arcmin 36.2\arcsec & 4.7 & 331.6380 & +16.2370 \\
J15479$-$4529 & 15$^{\rm h}$48$^{\rm m}$14.7$^{\rm s}$ & $-$45\degr 28\arcmin 40.4\arcsec & 3.5 & 332.4403 & +7.0228 \\
J16287$-$5021$^\diamond$ & 16$^{\rm h}$28$^{\rm m}$27.2$^{\rm s}$ & $-$50\degr 22\arcmin 38.3\arcsec & 4.4 & 334.1093 & $-$1.1261 \\
J17353$-$3539 & 17$^{\rm h}$35$^{\rm m}$23.5$^{\rm s}$ & $-$35\degr 40\arcmin 13.8\arcsec & 3.5 & 353.1445 & $-$1.7401 \\
J17476$-$2253 & 17$^{\rm h}$47$^{\rm m}$30.0$^{\rm s}$ & $-$22\degr 52\arcmin 43.2\arcsec & 4.8 & 5.3999 & +2.7813 \\
J18214$-$1318$^\star$ & 18$^{\rm h}$21$^{\rm m}$19.7$^{\rm s}$ & $-$13\degr 18\arcmin 38.2\arcsec & 3.5 & 17.6813 & +0.4856  \\
J19267+1325$^\diamond$ & 19$^{\rm h}$26$^{\rm m}$27.0$^{\rm s}$ & +13\degr 22\arcmin 03.4\arcsec & 3.7 & 48.8032 & $-$1.5059 \\
J20286+2544$^\ddagger$ \#1 & 20$^{\rm h}$28$^{\rm m}$34.9$^{\rm s}$ & +25\degr 43\arcmin 59.7\arcsec & 3.9 & 67.0045 & $-$7.5713 \\
 \#2 & 20$^{\rm h}$28$^{\rm m}$28.7$^{\rm s}$ & +25\degr 43\arcmin 22.5\arcsec & 4.4 & 66.9825 & $-$7.5582 \\
J23206+6431& 23$^{\rm h}$20$^{\rm m}$36.8$^{\rm s}$ & +64\degr 30\arcmin 42.8\arcsec & 3.8 & 113.3539 & +3.3424\\
\hline
\hline
\end{tabular}}
\medskip
 $^\dagger$ Source is very faint, just a very slight excess (very few photons) within IBIS error; 
 $^{\star}$~consistent with the {\it Chandra} position published by \citet{tomsick08}; $^\ddagger$~several sources within IBIS error; $^\diamond$ consistent with the {\it Chandra} position published by \citet{tomsick08b}.
\end{table}