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Table 3:

Main results obtained from the analysis of the X-ray spectra of the 17 sources of the present sample.

Source
RA Dec $N_{\rm H}$ Gal $N^{\bullet}_{\rm H}$ $\Gamma^{+}$ $F_{(2-10)~{\rm keV}}$ $F_{(14-195)~{\rm keV}}$ $L_{\rm X}$ Ref.*
      $\times 10^{22}$ cm-2 $\times 10^{22}$ cm-2   $\times 10^{-12}$ erg s-1 cm-2 $\times 10^{-11}$ erg s-1 cm-2 1043 erg s-1  
Swift J0059.4+3150A 00 59 53.29 +31 49 36.6 0.055 - $\rm 1.67^{+0.03}_{-0.03}$ 7.3 4.2 0.6 (2-10) 1
                3.1 (14-195)  
Swift J0134.1-3625A 01 33 57.71 -36 29 38.4 0.019 $\rm 75^{+34}_{-21}$ [1.8] 1.9 5.4 0.8 (2-10) 1
                7.2 (14-195)  
Swift J0342.0-2115A 03 42 03.62 -21 14 39.6 0.023 - $\rm 1.94^{+0.05}_{-0.05}$ 23.8 4.6 $\sim$1.3 (2-10) 1
                1.8 (14-195)  
Swift J0350.1-5019A 03 50 23.08 -50 18 11.4 0.012 $\rm 17^{+9}_{-7}$ [1.8] 3.1 3.1 1.0 (2-10) 1
                9.5 (14-195)  
Swift J0505.7-2348A 05 05 45.70 -23 51 13.3 0.021 $\rm 6^{+0.5}_{-0.5}$ $\rm 1.4^{-0.4}_{+0.3}$ 15.5 7.2 5.3 (2-10) 1
                21.6 (14-195)  
Swift J0501.9-3239A 05 19 35.82 -32 39 26.6 0.018 - $\rm 1.45^{+0.05}_{-0.05}$ 13.6 6.2 0.5 (2-10) 1
                1.2 (14-195)  
Swift J0640.1-4328A 06 40 37.89 -43 21 19.8 0.025 $\rm 11.7^{+4.5}_{-3.6}$ [1.8] 2.2 2.0 2.3 (2-10) 1
                28.9 (14-195)  
Swift J0727.5-2406C 07 27 21.05 -24 06 32.2 0.650 - - 0.6 2.2 2.7 (2-10) 2
                93.2 (14-195)  
        $\rm 47^{+13}_{-12}, { [0.7]}$          
Swift J0739.6-3144B 07 39 44.61 -31 43 01.6 0.431   $\rm 1.77^{+0.07}_{-0.09}$ 0.9 2.5 0.2 (2-10) 2
        $\rm 14^{+2.3}_{-1.9},{ [0.9]}$       4.5 (14-195)  
Swift J0743.0-2543B 07 43 14.95 -25 45 44.3 0.581 - - 14.7 $^{\triangle}$ 2.0 2.1 (2-10) 2
                2.8 (14-195)  
Swift J0811.5+0937C 08 11 30.99 +09 33 51.6 0.024 - - 0.1 2.6 3.0 (2-10) 2
                778.1 (14-195)  
Swift J0902.0+6007A 09 01 58.81 +60 09 05.8 0.043 $\rm 8^{+8.6}_{-4.0}$ [1.8] 1.1 3.1 0.04 (2-10) 1
                1.2 (14-195)  
Swift J0904.3+5538A 09 04 36.92 +55 35 59.7 0.022 - $\rm 1.44^{+0.07}_{-0.07}$ 4.9 1.9 1.8 (2-10) 1
                7.2 (14-195)  
Swift J0911.2+4533A 09 11 29.98 +45 28 04.1 0.012 $\rm 30^{+9.5}_{-7}$ [1.8] 2.0 1.8 0.4 (2-10) 1
                5.8 (14-195)  
Swift J0917.2-6221A 09 16 09.14 -62 19 28.4 0.158 $\rm0.7^{+0.3}_{-0.3}$ $\rm 1.67^{+0.2}_{-0.2}$ 16.0 3.3 14.8 (2-10) 1
                28.8 (14-195)  
Swift J0923.7+2255A 09 23 42.89 +22 54 33.2 0.031 - $\rm 1.95^{+0.05}_{-0.05}$ 11.8 4.5 3.7 (2-10) 1
                12.7 (14-195)  
Swift J1049.4+2258A 10 49 30.88 +22 57 52.9 0.019 $\rm 20^{+5}_{-3}$ [1.8] 0.7 3.7 0.2 (2-10) 1
                10.9 (14-195)  

+ The square brackets in the $\Gamma$ column indicate that we used a fixed value; * this column reports the references for the hard X-ray flux; $^{\triangle}$ source fluxes were calculated from count rates (see http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3table.pl); $^{\bullet}$ the values in the square brackets indicate the covering fraction; 1 Tueller et al. (2009); 2 Ajello et al. (2007); A soft X-ray data from Swift/XRT; B soft X-ray data from XMM/EPIC; C soft X-ray data from Chandra.


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