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Table 2

X-ray spectral fits.

ID XID z N H Γ NH (Γ = 1.8) Γ (NH = 0) L X
(1) (2) (3) (4) (5) (6) (7) (8)

W-4 LE-97 2.58  <15.3  <15.0 2.9
W–9 LU-114 LE-319 3.99 97.
W-11 LU-131 , LE-332 6.07 7.3
W-40 LU-385 1.90 1.1
W-45 LU-230 2.50  <5.53 0.37
W-57 LU-26, LE-203 2.940 6.8
W-59 LU-441 1.38  <6.1 0.12
W-66 LE-725 0.58  <0.17  <0.06 2.4
W-67 LU-362 2.122 1.8 0.24
W-84 LU-33 3.20  <30.5 7.3
W-92 LE-112 2.10 1.80
W-101 LU-25 2.53  <7.9  <2.8 1.53
W-108 LE-634 0.0875  <0.62 2 × 10-3
W-114 LU-23 1.605  <45.0 0.43

Notes. The columns are: (1) Laboca ID in Weiß et al. (2009); (2) CDFS (LU) or eCDFS(LE) ID in Luo et al. (2008) or Lehmer et al. (2005), respectively; (3) redshift; (4), (5) rest-frame column density and photon index in the case of sources with good photon statistics (see text); (6) rest-frame column density in units of 1022 cm-2 for fixed Γ = 1.8; (7) photon-index Γ for column density NH = 0; (8) Intrinsic X-ray luminosity in the 2–10 keV band in units of 1043 erg   s-1, obtained by setting NH = 0 in Col. (6);

(†)

Denotes a possible star-forming galaxies on the basis of the X-ray properties i.e. low X-ray luminosity and soft spectrum (see text).

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