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Table 3:

Results from X-ray data analysis and spectral fitting.

SDSS Name 		Cts HR $Nx{\rm H}^{\rm gal}$ $Nx{\rm H}$ $\Gamma$ $\chi^2/{\rm d.o.f.}$ f2-10 $L^{\rm abs}x{2-10}$ $L^{\rm int}x{2-10}$ Class
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

J105951.36+301817.4 		237 -0.30 2.0 $\rm 1.84^{+1.05}x{-0.75}$ $\rm 1.90^{+0.40}x{-0.35}$ 25.6/20 16 44.70 44.80 thin
J092640.67+023628.7 65 -0.06 3.8 $\rm 4.40^{+4.00}x{-2.70}$ $\rm 1.67^{+0.75}x{-0.65}$ ... 6.8 44.61 44.75 thin?
J034222.54-055727.9 175 -0.50 5.3 $\rm0.70^{+0.77}x{-0.57}$ $\rm 1.83^{+0.56}x{-0.45}$ 10.4/13 13 44.60 44.61 thin
J104603.17+071907.2 31 -0.16 2.8 $\rm 3.10^{+2.22}x{-1.59}$ $1.8^{\rm fixed}$ ... 3.7 44.04 44.15 thin?
J165158.61+432508.6 313 -0.38 1.9 $\rm0.72^{+0.55}x{-0.44}$ $\rm 1.76^{+0.33}x{-0.30}$ 20.7/27 19 44.76 44.79  thin
J080859.33+204711.8 18 0.80 4.0 ... $\rm --1.2^{+0.9}x{-1.4}$ ... 14 43.95 45.65* thick
J125848.58+120531.1 18 -0.05 2.2 $\rm 2.5^{+3.0}x{-1.8}$ $1.8^{\rm fixed}$ ... 1.8 43.88 43.97 thin?
J145503.94+515539.9 125 -0.43 1.8 $\rm0.36^{+0.98}x{-0.36}$ $\rm 1.82^{+0.58}x{-0.41}$ 14.4/9 5.7 44.67 44.69 thin
J085600.88+371345.5 <4 ..... 2.9 ... ... ... <2.0 <43.50 <45.20* thick

Notes. Column description: (1) Source name. (2) Net counts in the 0.5-8 keV band. (3) Hardness ratio, defined as (H-S)/(H+S), where H and S are the number of photons observed in the 0.5-2 keV and 2-8 keV bands, respectively. (4) Galactic column density in units of 1020 cm-2 (Dickey & Lockman 1990). (5) Absorbing column density at the source redshift in units of 1022 cm-2. (6) Photon index. (7) Chi-square value over number of degrees of freedom: for sources with less than 100 net counts C-statistics has been used. (8) Observed 2-10 keV flux in units of 10-14 erg cm-2 s-1. (9) Logarithm of the 2-10 keV rest frame luminosity, not corrected for absorption, in units of erg s-1. (10) Logarithm of the intrinsic 2-10 keV rest frame luminosity, i.e. corrected for absorption, in units of erg s-1; * for the two candidate Compton-thick objects it is assumed $L^{\rm int} = 50$ $\times $ $L^{\rm obs}$ (see text). (11) Object classification based on the X-ray spectral analysis and the X/NeV ratio.


Source LaTeX | All tables | In the text

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