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Home All issues Volume 498 / No 1 (April IV 2009) A&A, 498 1 (2009) 67-81 Full HTML
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Table 3:

X-ray spectral properties of the 23 sources showing a detection in at least one of the two energy bands, S and H.
ID CR0.5-2 CR2-10 HR Flux2-10 $N_{\rm H}$ log( $L_{\rm X,obs}$) log($L_{\rm X}$) log( $\lambda L_{5.8}$/L2-10) Analysis
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
1 $19.4 \pm3.4$ $6.1 \pm2.5$ - $0.52\pm0.19$ $\rm 10.2_{-4.0}^{+3.8}$ $\rm 1.1_{-0.7}^{+1.4}$ 43.68 43.72 1.4 1 SP
4 $1.7 \pm0.8$ $2.2 \pm0.9$ $0.13\pm0.31$ $\rm 8.5_{-4.2}^{+5.9}$ $\rm 19.9_{-14.4}^{+37.8}$ 43.90 44.31 1.31 SP
5 $2.7 \pm1.3$ $1.8 \pm1.2$ - $0.25\pm0.53$ $\rm 2.2_{-0.6}^{+2.8}$ <14.3 42.93 43.03 2.1 SP
6 $21.1 \pm2.5$ $63.7\pm4.3$ $0.49\pm0.07$ $\rm 113.1_{-30.0}^{+17.0}$ $\rm 10.8_{-3.8}^{+3.6}$ 44.49 44.71 0.95 SP
7 $4.0 \pm2.8$ $7.4 \pm3.9$ $0.30\pm0.44$ $\rm 14.2_{-3.0}^{+3.0}$ $\rm 25.0_{-23.0}^{+35.0}$ 44.40 44.48 1.43 HR
8 <6.9 $4.8 \pm4.1$ >-0.53 $\rm 3.4_{-1.6}^{+1.6}$ >0.1 43.13 >43.13a 1.29 HR
9 $1.8 \pm1.6$ $2.8 \pm1.9$ $0.21\pm0.54$ $\rm 5.3_{-1.9}^{+1.9}$ $\rm 25.0_{-24.0}^{+60.0}$ 44.08 44.15 1.47 HR
10 $1.0 \pm0.9$ <1.5 <0.25 < $\rm 2.3_{-1.4}^{+1.4}$ <6.0 42.82 42.87 1.76 HR
11 $5.0 \pm2.3$ $3.5 \pm2.4$ - $0.18\pm0.39$ $\rm 5.8_{-2.7}^{+2.6}$ $\rm 4.9_{-4.0}^{+9.9}$ 43.40 43.57 1.73 SP
12 $1.9 \pm1.6$ $5.7 \pm2.5$ $0.50\pm0.44$ $\rm 27.1_{-3.9}^{+4.8}$ $\rm 267.9_{-144.8}^{+274.7}$ 43.40 45.16 0.34 SP
19 $2.2 \pm1.3$ $8.6 \pm4.4$ $0.60\pm0.62$ $\rm 12.6_{-7.9}^{+7.9}$ $\rm 25.0_{-17.0}^{+75.0}$ 44.10 44.92 1.76 HR
21 $13.0 \pm5.3$ $10.6 \pm4.9$ - $0.10\pm0.31$ $\rm 24.8_{-6.4}^{+6.4}$ $\rm 4.0_{-3.5}^{+8.0}$ 44.19 44.21 1.05 HR
22 $5.9 \pm3.0$ $6.7 \pm3.7$ $0.06\pm0.37$ $\rm 11.3_{-4.2}^{+4.2}$ $\rm 13.0_{-11.0}^{+35.0}$ 44.35 44.39 1.56 HR
25 $10.9 \pm3.7$ $4.5 \pm5.0$ - $0.42\pm0.43$ $\rm 18.6_{-3.8}^{+3.8}$ <45.0 45.26 45.30 1.33 HR
31 <2.2 $0.9 \pm0.4$ >-0.15 $\rm 1.7_{-0.7}^{+0.7}$ >0.1 43.24 >43.24a 1.70 HR
32 $0.7 \pm0.3$ $1.8 \pm0.5$ $0.49\pm0.31$ $\rm 3.1_{-0.5}^{+0.5}$ $\rm 75.0_{-40.0}^{+75.0}$ 44.10 44.53 2.23 HR
33 $0.7 \pm0.3$ $1.9 \pm0.6$ $0.48\pm0.28$ $\rm 3.8_{-0.6}^{+0.6}$ $\rm 60.0_{-30.0}^{+45.0}$ 44.10 44.59 1.82 HR
36 $3.7 \pm2.5$ $9.4 \pm3.8$ $0.43\pm0.40$ $\rm 4.3_{-1.2}^{+6.6}$ <28.0 43.01 43.06 1.21 SP
39 $11.2 \pm2.8$ $25.9 \pm3.9$ $0.40\pm0.14$ $\rm 29.9_{-13.4}^{+7.4}$ $\rm 6.7_{-2.4}^{+3.5}$ 43.65 43.85 1.03 SP
40 $23.2 \pm3.5$ $6.9 \pm2.3$ - $0.53\pm0.16$ $\rm 9.3_{-1.3}^{+2.1}$ <1.5 43.88 43.90 1.34 SP
41 $4.6 \pm1.9$ $17.5\pm2.8$ $0.58\pm0.18$ $\rm 23.7_{-8.1}^{+6.9}$ $\rm 11.9_{-5.0}^{+8.7}$ 43.88 44.05 0.46 SP
43 $40.7 \pm5.8$ $3.3 \pm3.0$ - $0.81\pm0.18$ $\rm 12.0_{-2.7}^{+6.6}$ <0.3 44.44 44.45 1.04 SP
44 $31.2 \pm4.1$ $18.4\pm3.6$ - $0.26\pm0.11$ $\rm 19.5_{-7.5}^{+6.9}$ $\rm 1.7_{-0.8}^{+1.1}$ 43.94 44.01 1.24 SP
Column: (1) ID number; (2) count rate in the S band in units of 10-4 count/s; (3) count rate in the H band in units of 10-4 count/s; (4) Hardness Ratio between the H band and the S band computed with the formula H-S/${\rm H+S}$; (5) H band flux in units of 10-15 erg s-1 cm-2; (6) rest-frame column density $N_{\rm H}$ in units of 1022 cm-2; (7) logarithm of the observed luminosity in the H band (erg s-1); (8) logarithm of the absorption-corrected luminosity in the H band (erg s-1); (9) logarithm of the $\lambda $ $L_{5.8~\mu {\rm m}}$L2-10 ratio; (10) analysis method: SP for spectral fitting, HR for hardness ratio. For Chandra data the 2-10 keV count rate and flux was extrapolated from the 2-8 keV value assuming $\Gamma=1.9$.
a For these sources we computed the absorption-corrected luminosity using the lower limit on the $N_{\rm H}$ value. Accordingly, the intrinsic luminosity shown here is also a lower limit.

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