\begin{table}%t3
\caption{Properties of the candidate sources detected in the mosaic. Fluxes and luminosities are in the 20$-$60~keV energy range. $m_{\rm B}$~is the apparent magnitude in filter~$B$, unless specified in the footnote. \nh~is the intrinsic hydrogen column density; values in parenthesis are derived from the RASS-BSC~fluxes; lower limits mean non-detection in the ROSAT-BSC catalog. Unless mentioned in the comments, redshifts and class information have been obtained through Simbad or NED.  Stars indicate a match  with low-redshift AGN or otherwise unquestionable AGN~counterparts.}\label{tab:prop}
\par
\small%\centerline
 {
\begin{tabular}{lcccccl}
\hline \hline
\multicolumn{1}{c}{\rule{0pt}{1.2em}Name}&Flux&$m_{B}$&\nh&Redshift&$\log_{10}L_{{\rm obs}}$&Comments\\
&$10^{-11}$ erg~s$^{-1}$~cm$^{-2}$&&$10^{22}$ cm$^{-2}$&&erg s$^{-1}$\\
\hline  
IGR J12291+0203*& 11.56 $\pm$ 0.12&13.1& $<$$0.01$ & 0.1583 & 45.97 & {\nh: \citet{ShinEtal-2006-SpeSta}}\\
IGR J12258+1240*& 15.27 $\pm$ 0.19&12.2& 26.92 & 0.0084 & 43.38 & {\nh: \citet{ShuEtal-2007-InvNuc}}\\
IGR J12106+3925*& 30.74 $\pm$ 0.72&11.2& 7.5 & 0.0033 & 42.87 & {\nh: \citet{CappEtal-2006-XraSpe}}\\
IGR J12396$-$0521*&\z 4.48 $\pm$ 0.12&13.5& $<$$0.01$ & 0.0090 & 42.91 & {\nh: \citet{ShinEtal-2006-SpeSta}}\\
IGR J12562$-$0547*&\z 1.37 $\pm$ 0.12&18.0& \z 0.05 & 0.5362 & 46.39 & {\nh: \citet{ReevTurn-2000-XraSpe}}\\
IGR J12392$-$1612*&\z 2.24 $\pm$ 0.21&10.9& 1.9 & 0.036\z & 43.84 & {Class: \citet{MaseEtal-2006-UnvNatII}; \nh: \citet{SazoEtal-2005-IdeEig}}\\
IGR J12595+2755&\z 1.52 $\pm$ 0.15&13.5& $<$$0.01$ & 0.0231 & 43.28 & {\nh: \citet{ArnaEtal-2001-XmmObs}}\\
IGR J12233+0241*&\z 1.20 $\pm$ 0.12&15.5& (0.25) & 0.0234 & 43.18 \\
IGR J12226+0414*&\z 1.23 $\pm$ 0.13&17.5& (7.1) & 0.9650 & 47.08 \\
IGR J13092+1137*&\z 2.36 $\pm$ 0.24&14.6& 90.0\z & 0.0251 & 43.54 & {Class: \citet{MaseEtal-2006-UnvNatIV}; \nh: \citet{SazoEtal-2005-IdeEig}}\\
IGR J12390$-$2719*&\z 5.48 $\pm$ 0.61&14.6& 10\phantom{.00} & 0.0250 & 43.90 & {Class: \citet{MoreEtal-2006-OptCla}; \nh: \citet{TuelEtal-2005-SwiDet}}\\
IGR J13383+0434*&\z 3.25 $\pm$ 0.43&14.5& \z 2.89 & 0.0230 & 43.60 & {\nh: \citet{ShuEtal-2007-InvNuc}}\\
IGR J12185+2948*&\z 1.45 $\pm$ 0.22&14\phantom{.0}& $<$$0.02$ & 0.0129 & 42.74 & {\nh: \citet{PageEtal-2001-VarXmm}}\\
IGR J13225$-$1645*&\z 2.02 $\pm$ 0.31&14\phantom{.0}& 73.85 & 0.0165 & 43.10 & {\nh: This work (Chandra); see text}\\
IGR J13041$-$0533*&\z 0.84 $\pm$ 0.14&12\phantom{.0}& 44.98 & 0.0037 & 41.41 & {\nh: \citet{ShinEtal-2006-SpeSta}}\\
IGR J12299+0305&\z 0.71 $\pm$ 0.12&--& (2.5) & -- & -- & {QSO \object{2MASS J12301552+0302546}, $z=0.138$, $m_{V}=17.5$?}\\
IGR J12069$-$1448&\z 1.55 $\pm$ 0.28&--& $>$$2$ & 0.0184 & 43.08 \\
IGR J13042$-$1020*&\z 0.87 $\pm$ 0.16&11\phantom{.0}& 30.0\z & 0.0104 & 42.33 & {\nh: \citet{BassEtal-1999-ThrDia}}\\
IGR J12174$-$0131&\z 0.70 $\pm$ 0.13&--& $>$$2$ & -- & -- & {No obviously associated optical or infrared source}\\
IGR J12011+0649*&\z 1.04 $\pm$ 0.19&15.3& \z 6.61 & 0.0360 & 43.51 & {Class: \citet{MaseEtal-2006-OptCla}; \nh: \citet{LandEtal-2007-AGNNat}}\\
IGR J13415+3023*&\z 1.25 $\pm$ 0.23&15.3& $>$$2$ & 0.0399 & 43.68\\
IGR J12042$-$0756&\z 1.00 $\pm$ 0.19&--& $>$$2$ & -- & -- & {$m_{J}=14.1$, $m_{K}=13.0$}\\
IGR J12070+2535&\z 1.42 $\pm$ 0.27&19.9& $>$$2$ & 0.0477 & 43.90 \\ 
IGR J13133$-$1109*&\z 0.99 $\pm$ 0.19&15.6& (0.32) & 0.0344 & 43.45 \\ 
IGR J12060+3818&\z 3.75 $\pm$ 0.71&--& $>$$2$ & -- & --& {$m_{J}=15.5$, $m_{K}=14.3$}\\
IGR J13517$-$0042&\z 2.70 $\pm$ 0.52&19.2& $>$$2$ & 0.0531 & 44.28 \\
IGR J12130+0701*&\z 0.81 $\pm$ 0.16&13.2& $>$$2$ & 0.0070 & 41.95 & {Class: \citet{MaseEtal-2007-SpeSix}}\\ 
IGR J11457$-$1827*&\z 3.29 $\pm$ 0.65&14.6& ($<$$0.01$) & 0.0329 & 43.93 \\
IGR J12172+0710*&\z 0.76 $\pm$ 0.15&13.2& \z 0.15 & 0.0080 & 42.04 & {\nh: \citet{MaseEtal-2006-UnvNatIV}}\\
IGR J12136$-$0527&\z 0.71 $\pm$ 0.14&--& (2.0) & -- & -- & {Sy 1 \object{2MASX J12135456-0530193}, $z=0.066$, $m_{V}=16.2$?}\\
IGR J12310+1221*&\z 0.94 $\pm$ 0.19&10.4& \z 0.02 & 0.044\z & 43.65 & {\nh: \citet{LieuEtal-1996-DisMil}}\\
IGR J11225$-$0419&\z 3.54 $\pm$ 0.70&17.5& $>$$2$ & 0.0535 & 44.41 \\
IGR J13353$-$1113&\z 1.59 $\pm$ 0.31&--& $>$$2$ & -- & -- & {No obviously associated optical or infrared source}\\
IGR J11427+0854&\z 2.08 $\pm$ 0.41&\phantom{$^1$}15.3$^1$& $>$$2$ & 0.0213 & 43.34 \\
\hline
\end{tabular}}
\medskip
$^1$ $g$ band.
\end{table}