Table 6: Previously Known Type 2 AGN, CDF-S.
A03 S04 redshift $\log L_{\rm x}(2{-}8~{\rm keV})$ Notesa
       erg/s  
44 66 0.574 43.31  
48 267 0.720 43.07 QF = 1
60 155 0.545 42.11  
68 62 2.810 44.48  
80 535 0.575 42.20  
84 149 1.033 42.81 QF = 1
86 57 2.562 44.28  
88 56a 0.605 43.41  
90 600 1.327 42.86  
91 266 0.735 42.43  
96 531 1.544 43.19  
118 51a 1.097 44.06  
123 153 1.536 43.97  
126 50 0.670 42.61 QF = 1
131 253 0.481 42.53 QF = 1
134 151 0.604 43.02  
137 612b 0.736 42.55  
146 188 0.734 42.14  
160 606a 1.037 42.89 QF = 1
161 47 0.733 43.08  
162 260 1.043 42.83  
164 150 1.090 43.34  
166 45 2.291 44.20 QF = 1
176 43 0.734 42.90  
179 41 0.668 43.31  
188 202 3.700 44.47  
212 512 0.668 42.08  
220 190 0.735 43.07  
245 27 3.064 44.64  
247 25 0.625 43.15 QF = 0.5
249 611a 0.979 42.74 QF = 1
263 20a 1.016 43.40  
269 170 0.664 42.38  
271 252 1.178 43.29  
276 184 0.667 42.54  
a From Szokoly et al. (2004): QF = 1, spectrum cannot be identified securely, typically only a single narrow line present; QF = 0.5, only a hint of some spectral feature.

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