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Table 2

Manual spectral-fitting results: highly absorbed sources with NH> 1023 cm-2.

3XMM name(nobs) Model N H Γ S.F. EW kT Flux Log (Luminosity) C-stat/d.o.f. Goodness
1022 cm-2 (%) eV keV erg cm-2 s-1 erg s-1 (%)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
3XMMJ080535.0+240950 2PL+T+L 48 1.9f 2.5 290 0.25 2.73 × 10-13 42.94 195/260 100
3XMMJ080741.0+390015 2PL+T+L 40 1.9f 6 900 0.7 2.15 × 10-13 41.94 202/209 93
3XMMJ082443.2+295923 2PL+2T+L 20 1.9 1 360 0.121(0.69) 1.03 × 10-12 42.56 1472/1653 100
3XMMJ083139.0+524205(3) 2PL+T+L 30 2.3 1 180 0.18 7.71 × 10-14 42.35 1114/1254 100
3XMMJ084002.3+294902 2PL+T+L 62 1.9f 1 300 0.33 7.29 × 10-13 43.55 1103/1328 100
3XMMJ085331.0+175338 2PL+T 50 1.9f 2 ... 0.20 1.56 × 10-13 43.72 189/255 100
3XMMJ091804.2+514113 PL+R+L >100 1.9f ... 360 ... 7.49 × 10-14 42.76r 119/120 51
3XMMJ093551.5+612111 2PL+T+L 130 1.9f 4 400 0.7 1.92 × 10-13 42.88 712/839 100
3XMMJ093952.7+355358 PL+R+L >100 1.9f 11 370 ... 4.38 × 10-13 43.26 800/904 100
3XMMJ095906.6+130134 2PL+T+L 17 1.9 0.3 150 0.44 9.90 × 10-13 42.82 1081/1273 100
3XMMJ103408.5+600152 2PL+T+L 80 1.9f 9 1100 0.19 1.99 × 10-13 42.75 560/533 66
3XMMJ104930.9+225752 2PL+T+L 55 1.5 2 220 0.18 1.59 × 10-12 43.17 895/1025 100
3XMMJ113240.2+525701(2) 2PL+T+L 60 2.28 0.3 410 0.66 4.72 × 10-13 42.69 863/985 100
3XMMJ113549.0+565708 2PL+T+L 70 2.84 3 700 0.8 5.22 × 10-14 42.43 515/514 83
3XMMJ114454.8+194635 2PL 29 1.7 11 ... ... 6.72 × 10-14 41.44 394/428 99
3XMMJ115704.8+524903 2PL+T+L 60 2.6 3 1500 0.20 9.26 × 10-14 42.18 634/617 74
3XMMJ120429.6+201858(2) 2PL+T+L 34 1.8 1 320 0.14 1.73 × 10-12 42.81 416/477 100
3XMMJ120429.6+201858(1) 2PL+T+L 22 1.8f 1 320 0.25 2.98 × 10-12 42.93 293/332 100
3XMMJ121839.4+470626(2) 2PL+T+L 44 2.2 4 700 0.14 7.95 × 10-14 42.80 412/420 89
3XMMJ122546.7+123943(1) 2PL+T+L 27 1.4 3 500 0.27 7.44 × 10-12 42.45 1896/2106 100
3XMMJ122546.7+123943(1) 2PL+T+L 28.7 1.52 0.7 220 0.27 2.11 × 10-11 42.96 2879/2801 92
3XMMJ122546.7+123943(1) 2PL+T+L 23.6 1.59 0.3 90 0.30 4.13 × 10-11 43.23 4268/3129 0
3XMMJ123843.4+092736 2PL+2T+L 35 1.5 2 180 0.15(0.70) 1.11 × 10-12 43.69 1530/1618 100
3XMMJ131104.6+272806 2PL+T+L 200 1.9f 3 970 0.19 3.40 × 10-14 43.80 398/446 100
3XMMJ132348.4+431804 2PL+T+L 60 2.4 0.2 260 0.7 8.70 × 10-13 43.02 790/971 100
3XMMJ140700.3+282714 PL+R+L >100 1.9f ... 600 ... 2.85 × 10-13 42.58r 646/808 100
3XMMJ141546.2+112943(2) 2PL+L 70 1.9f 4 150 ... 5.97 × 10-14 45.61 302/365 100
3XMMJ150754.3+010817 2PL+T+L 60 1.9f 5 1300 0.15 1.12 × 10-13 42.61 392/426 99
3XMMJ150946.8+570002 2PL+T 23 1.9f 3 ... 0.34 1.36 × 10-13 39.72 118/124 83
3XMMJ153457.2+233011(4) PL+T+R+L >100 1.9f ... 1500 0.9 1.11 × 10-13 40.92r 556/610 100
3XMMJ215649.5-074531(2) 2PL+T+L 40 1.9f 9 1400 0.20 4.80 × 10-14 41.99 461/463 75

Notes. Columns: (1) source name in the 3XMM-DR4 catalog. (2) Best-fit model. (3) Intrinsic column density. (4) Power-law photon index. (5) Scattered fraction in the double power-law model (ratio between the power-law normalizations). (6) Equivalent width of the Fe Kα emission line. (7) Plasma temperature in the thermal model. (8) Observed flux in 2–10 keV. (9) Intrinsic luminosity in 2–0 keV. (10) C-stat likelihood value over degrees of freedom. (11) Goodness of fit estimated as 100-XSPEC goodness. Numbers between parenthesis after the name of the source correspond to the number of merged observations. Compton-thick candidates are in boldface.

(f)

Fixed parameter.

(r)

No direct continuum.

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