Table 3: 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. $N_{{\rm H}}$ 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.
Name Flux mB $N_{{\rm H}}$ Redshift $\log_{10}L_{{\rm obs}}$ Comments
  10-11 erg s-1 cm-2   1022 cm-2   erg s-1  
IGR J12291+0203* 11.56 $\pm$ 0.12 13.1 <0.01 0.1583 45.97 $N_{{\rm H}}$: Shinozaki et al. (2006)
IGR J12258+1240* 15.27 $\pm$ 0.19 12.2 26.92 0.0084 43.38 $N_{{\rm H}}$: Shu et al. (2007)
IGR J12106+3925* 30.74 $\pm$ 0.72 11.2 7.5 0.0033 42.87 $N_{{\rm H}}$: Cappi et al. (2006)
IGR J12396-0521* 4.48 $\pm$ 0.12 13.5 <0.01 0.0090 42.91 $N_{{\rm H}}$: Shinozaki et al. (2006)
IGR J12562-0547* 1.37 $\pm$ 0.12 18.0 0.05 0.5362 46.39 $N_{{\rm H}}$: Reeves & Turner (2000)
IGR J12392-1612* 2.24 $\pm$ 0.21 10.9 1.9 0.036 43.84 Class: Masetti et al. (2006c); $N_{{\rm H}}$: Sazonov et al. (2005)
IGR J12595+2755 1.52 $\pm$ 0.15 13.5 <0.01 0.0231 43.28 $N_{{\rm H}}$: Arnaud et al. (2001)
IGR J12233+0241* 1.20 $\pm$ 0.12 15.5 (0.25) 0.0234 43.18  
IGR J12226+0414* 1.23 $\pm$ 0.13 17.5 (7.1) 0.9650 47.08  
IGR J13092+1137* 2.36 $\pm$ 0.24 14.6 90.0 0.0251 43.54 Class: Masetti et al. (2006a); $N_{{\rm H}}$: Sazonov et al. (2005)
IGR J12390-2719* 5.48 $\pm$ 0.61 14.6 10 0.0250 43.90 Class: Morelli et al. (2006); $N_{{\rm H}}$: Tueller et al. (2005)
IGR J13383+0434* 3.25 $\pm$ 0.43 14.5 2.89 0.0230 43.60 $N_{{\rm H}}$: Shu et al. (2007)
IGR J12185+2948* 1.45 $\pm$ 0.22 14 <0.02 0.0129 42.74 $N_{{\rm H}}$: Page et al. (2001)
IGR J13225-1645* 2.02 $\pm$ 0.31 14 73.85 0.0165 43.10 $N_{{\rm H}}$: This work (Chandra); see text
IGR J13041-0533* 0.84 $\pm$ 0.14 12 44.98 0.0037 41.41 $N_{{\rm H}}$: Shinozaki et al. (2006)
IGR J12299+0305 0.71 $\pm$ 0.12 - (2.5) - - QSO 2MASS J12301552+0302546, z=0.138, mV=17.5?
IGR J12069-1448 1.55 $\pm$ 0.28 - >2 0.0184 43.08  
IGR J13042-1020* 0.87 $\pm$ 0.16 11 30.0 0.0104 42.33 $N_{{\rm H}}$: Bassani et al. (1999)
IGR J12174-0131 0.70 $\pm$ 0.13 - >2 - - No obviously associated optical or infrared source
IGR J12011+0649* 1.04 $\pm$ 0.19 15.3 6.61 0.0360 43.51 Class: Masetti et al. (2006b); $N_{{\rm H}}$: Landi et al. (2007)
IGR J13415+3023* 1.25 $\pm$ 0.23 15.3 >2 0.0399 43.68  
IGR J12042-0756 1.00 $\pm$ 0.19 - >2 - - mJ=14.1, mK=13.0
IGR J12070+2535 1.42 $\pm$ 0.27 19.9 >2 0.0477 43.90  
IGR J13133-1109* 0.99 $\pm$ 0.19 15.6 (0.32) 0.0344 43.45  
IGR J12060+3818 3.75 $\pm$ 0.71 - >2 - - mJ=15.5, mK=14.3
IGR J13517-0042 2.70 $\pm$ 0.52 19.2 >2 0.0531 44.28  
IGR J12130+0701* 0.81 $\pm$ 0.16 13.2 >2 0.0070 41.95 Class: Masetti et al. (2007)
IGR J11457-1827* 3.29 $\pm$ 0.65 14.6 (<0.01) 0.0329 43.93  
IGR J12172+0710* 0.76 $\pm$ 0.15 13.2 0.15 0.0080 42.04 $N_{{\rm H}}$: Masetti et al. (2006a)
IGR J12136-0527 0.71 $\pm$ 0.14 - (2.0) - - Sy 1 2MASX J12135456-0530193, z=0.066, mV=16.2?
IGR J12310+1221* 0.94 $\pm$ 0.19 10.4 0.02 0.044 43.65 $N_{{\rm H}}$: Lieu et al. (1996)
IGR J11225-0419 3.54 $\pm$ 0.70 17.5 >2 0.0535 44.41  
IGR J13353-1113 1.59 $\pm$ 0.31 - >2 - - No obviously associated optical or infrared source
IGR J11427+0854 2.08 $\pm$ 0.41 15.31 >2 0.0213 43.34  


1 g band.


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