Table A.1.
Properties of the X-ray-detected sample obtained from an X-ray spectral analysis.
ID | z | Ncts | Γ | log(NH/cm−2) | log(L2 − 10 keV/L⊙) | X/[Ne V] |
---|---|---|---|---|---|---|
lid1856 | 0.73 | 1827 | ![]() |
![]() |
![]() |
![]() |
cid339 | 0.69 | 373 | ![]() |
![]() |
![]() |
![]() |
cid522 | 0.94 | 336 | ![]() |
![]() |
![]() |
![]() |
cid110 | 0.73 | 313 | ![]() |
< 21.7 | ![]() |
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cid173 | 1.00 | 242 | ![]() |
![]() |
![]() |
![]() |
lid1840 | 1.01 | 216 | ![]() |
< 21.7 | ![]() |
![]() |
cid381 | 0.86 | 208 | ![]() |
![]() |
![]() |
![]() |
lid279 | 0.88 | 173 | ![]() |
< 21.7 | ![]() |
![]() |
lid1478 | 0.83 | 168 | ![]() |
![]() |
![]() |
![]() |
cid496 | 0.90 | 165 | ![]() |
![]() |
![]() |
![]() |
cid456 | 1.02 | 162 | ![]() |
![]() |
![]() |
![]() |
cid221 | 0.75 | 142 | ![]() |
< 22 | ![]() |
![]() |
cid620 | 1.18 | 126 | ![]() |
![]() |
![]() |
![]() |
lid1826 | 1.17 | 109 | ![]() |
![]() |
![]() |
![]() |
cid138 | 0.70 | 99 | ![]() |
![]() |
![]() |
![]() |
cid1126 | 0.96 | 93 | ![]() |
![]() |
![]() |
![]() |
lid489 | 0.85 | 93 | ![]() |
< 22.1 | ![]() |
![]() |
cid717 | 0.89 | 85 | ![]() |
> 21.0 | ![]() |
![]() |
cid503 | 0.91 | 80 | ![]() |
![]() |
![]() |
![]() |
cid426 | 0.86 | 75 | ![]() |
![]() |
![]() |
![]() |
cid254 | 0.71 | 60 | ![]() |
![]() |
![]() |
![]() |
lid689 | 0.68 | 59 | ![]() |
< 21.6 | ![]() |
![]() |
lid3483 | 0.66 | 51 | ![]() |
![]() |
![]() |
![]() |
cid1130 | 0.79 | 48 | ![]() |
> 21.9 | ![]() |
![]() |
cid1019 | 0.73 | 41 | ![]() |
![]() |
![]() |
< 105 |
lid1603 | 0.97 | 39 | ![]() |
> 22.7 | ![]() |
![]() |
cid401 | 0.97 | 39 | ![]() |
![]() |
![]() |
![]() |
lid1869 | 1.17 | 36 | ![]() |
![]() |
![]() |
![]() |
cid1230 | 0.75 | 35 | ![]() |
> 22.0 | ![]() |
![]() |
cid1169 | 0.96 | 21 | ![]() |
![]() |
![]() |
![]() |
lid2210 | 0.74 | 18 | ![]() |
![]() |
![]() |
![]() |
lid1459 | 1.00 | 17 | ![]() |
![]() |
![]() |
![]() |
cid1706 | 0.76 | 15 | ![]() |
![]() |
![]() |
< 107 |
cid2454 | 0.76 | 15 | ![]() |
![]() |
![]() |
![]() |
lid3017 | 0.68 | 15 | ![]() |
![]() |
![]() |
![]() |
cid1508 | 0.67 | 11 | ![]() |
![]() |
![]() |
< 89 |
Notes. Ncts refers to the number of net-counts (i.e., background subtracted), Γ to the photon index obtained using a power-law model with Galactic absorption. The amount of obscuration (NH) and intrinsic (i.e. absorption corrected) 2 − 10 keV luminosity are obtained from a model with Galactic absorption, power-law emission with fixed photon index (Γ = 1.8), and absorption component at the source redshift to model the source obscuration.
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