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Home All issues Volume 507 / No 2 (November IV 2009) A&A, 507 2 (2009) 747-756 Full HTML
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Table 1:

X-ray spectra of the candidate Compton-thick AGN.
  Power-law Reflection  
ID $\alpha, \delta$ z $N_{\rm H}$ $\Gamma $ $\chi^2$/$\nu$ $\Gamma $ $\chi^2$/$\nu$ $\log L_{\rm x}$ Flux
(1) (2) (3) (4) (5) (6 (7) (8) (9) (10)

35 		12 35 49.44 +62 15 36.9 2.203 <6.7 $0.15^{\rm +0.35}_{-0.40}$ 6.4/8 $1.75^{\rm +0.44}_{-0.42}$ 7.8/9 42.68 1.20
91 12 36 11.40 +62 21 49.9 0.51 (1.78) $3.0^{\rm +3.2}_{-2.7}$ $0.30^{\rm +0.62}_{-0.50}$ 31.2/17 $1.74^{\rm +0.26}_{-0.54}$ 40.3/19 42.65 9.44
92 12 36 11.80 +62 10 14.5 0.91 $4.6^{\rm +8}_{-4.6}$ $-0.14^{\rm +0.94}_{-0.86}$ 17.2/7 $1.16^{\rm +0.44}_{-0.66}$ 23.2/7 42.42 2.69
107 12 36 15.83 +62 15 15.5 0.59 (2.48) $7.4^{\rm +7.5}_{-6.3}$ $0.66^{\rm +0.37}_{-0.46}$ 11.0/12 $1.93^{\rm +0.21}_{-0.21}$ 11.1/13 43.08 1.85
121 12 36 19.89 +62 19 10.1 0.520 $0.3^{\rm +2.1}_{-0.2}$ $0.49^{\rm +0.37}_{-0.43}$ 4.8/8 $2.8^{\rm +0.37}_{-0.40}$ 11.7/9 41.93 1.90
127 12 36 21.21 +62 11 08.8 1.014 $12.3^{\rm +2.5}_{-9.0} $ $0.20^{\rm +1.20}_{-0.70}$ 12.9/12/8 $1.16^{\rm +0.23}_{-0.31}$ 13.2/13 42.76 3.98
135 12 36 22.66 +62 16 29.8 2.466 $275^{\rm +195}_{-138} $ 1.8 5.5/4 - - 43.61 1.14
171 12 36 32.59 +62 07 59.8 1.993 $ 2.2^{\rm +15}_{-2}$ $-0.02^{\rm +0.75}_{-0.47}$ 7.2/9 $1.65^{\rm +0.31}_{-0.36}$ 6.2/10 42.73 1.83
190 12 36 35.58 +62 14 24.1 2.005 $1.5^{\rm +1.0}_{-1.5} $ $0.28^{\rm +0.51}_{-0.29}$ 13.2/13 $1.93^{\rm +0.20}_{-0.20}$ 11.2/14 43.01 2.48
191 12 36 35.86 +62 07 07.7 0.28 (0.93) <20 $-1.4^{\rm +1.40}_{-0.47}$ 38.1/18 $0.20^{\rm +0.44}_{-0.78}$ 27.4/16 41.73 5.35

The columns are: (1) Alexander ID number; (2) X-ray Equatorial Coordinates (J2000); (3) redshift; three and two decimal numbers refer to spectroscopic and photometric redshift respectively; in brackets we quote the possible X-ray spectroscopic redshift; (4) intrinsic column density in units of 1022  $\rm cm^{-2}$ for the power-law model; (5) photon index in the case of the power-law model; (6) $\chi^2$ and degrees of freedom for the power-law model; (7) photon index in the case of the reflection model; (8) $\chi^2$ and degrees of freedom for the reflection model; (9) logarithm of the observed luminosity in the 2-10 keV band in units of $\rm erg~s^{-1}$; (10) observed flux in the 2-10 keV band in units of 10-15  $\rm erg~cm^{-2}~s^{-1}$.


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