Table 5.

Results of absorbed power law fits to X-ray spectra.

3XMM name*N  H  L  2–10  C/dof§3XMM name*N  H  L  2–10  C/dof§
(1022 cm−2)(1044 erg s−1)(1022 cm−2)(1044 erg s−1)
J021502.3−034111|$5.8^{+4.3}_{-3.1}$|2.30101.7/113J022205.0−033238|$7.2^{+3.7}_{-4.5}$|2.21491.7/564
J021529.4−034233|$0.069^{+0.15}_{-0.069}$|1.21298.1/281J022214.4−034619|$0.2^{+0.14}_{-0.12}$|0.688660.0/801
J021532.3−035124|$0.17^{+0.73}_{-0.17}$|2.38116.2/118J022231.7−044910|$2.2^{+2.4}_{-1.5}$|6.6339.0/45
J021541.0−034505|$0.051^{+0.34}_{-0.051}$|0.721142.3/139J022314.5−041017|$0.17^{+0.67}_{-0.17}$|0.75777.3/81
J021606.6−050303|$0.17^{+0.18}_{-0.13}$|0.0613140.7/125J022326.5−041837|$0.064^{+0.21}_{-0.064}$|0.0848158.4/197
J021614.5−050351|$0.84^{+0.82}_{-0.56}$|1.19117.6/122J022330.8−044632|$1.4^{+0.40}_{-0.35}$|7.65280.2/328
J021625.7−050518|$0.17^{+0.41}_{-0.17}$|2.29100.7/122J022331.0−044234|$2.0^{+1.6}_{-1.1}$|5.8079.4/95
J021634.3−050724|$0.23^{+0.22}_{-0.18}$|0.892192.8/215J022334.3−040841|$12^{+7.6}_{-5.1}$|0.861171.3/174
J021642.3−043552|$3.3^{+0.53}_{-0.47}$|21.6465.6/531J022337.9−040512|$3.2^{+1.5}_{-1.1}$|5.00233.0/260
J021644.6−040651|$0.94^{+0.5}_{-0.55}$|2.10188.1/151J022343.3−041622|$0.51^{+0.48}_{-0.11}$|0.437174.5/181
J021705.4−045655|$0.39^{+0.42}_{-0.29}$|1.29108.5/107J022347.1−040051|$1.5^{+2.2}_{-1.3}$|4.70176.4/189
J021705.7−052546|$1.1^{+0.54}_{-0.42}$|1.27150.2/180J022352.0−052421|$0.12^{+0.38}_{-0.12}$|3.2898.7/98
J021721.2−052336|$0^{+0.14}_{-0}$|0.423127.6/129J022353.2−041532|$0.54^{+0.51}_{-0.37}$|0.721246.1/235
J021721.9−043655|$0.92^{+0.55}_{-0.40}$|0.744137.0/161J022358.2−050946|$0.21^{+0.65}_{-0.21}$|1.1486.1/90
J021725.8−051955|$0.40^{+0.52}_{-0.37}$|0.247170.5/145J022405.2−041612|$0.16^{+0.19}_{-0.16}$|1.70337.9/440
J021729.3−052122|$6.5^{+3.5}_{-2.5}$|2.17138.8/137J022408.6−041151|$18^{+10}_{-6}$|1.84232.5/253
J021736.4−050106|$1.00^{+0.81}_{-0.58}$|1.00161.9/157J022410.3−040224|$0.39^{+1.4}_{-0.39}$|1.38131.2/118
J021744.1−034531|$0^{+0.083}_{-0}$|0.6581.9/83J022412.5−035740|$0.46^{+1.2}_{-0.46}$|1.2195.4/72
J021810.1−051844|$0.7^{+1.2}_{-0.7}$|4.3109.6/137J022417.4−041812|$3.8^{+5.5}_{-3.3}$|0.516130.1/144
J021813.2−045051|$0.81^{+0.43}_{-0.31}$|0.261147.3/137J022420.7−041224|$0.15^{+0.20}_{-0.15}$|0.687244.7/302
J021825.6−045945|$9.5^{+3}_{-2.4}$|3.11196.5/203J022421.1−040355|$1.1^{+0.68}_{-0.51}$|1.25246.1/259
J021842.8−051934|$7.3^{+2.8}_{-2.2}$|5.49200.7/246J022500.1−050831|$1.5^{+0.89}_{-0.65}$|0.836116.8/114
J021914.8−045139|$0.19^{+0.34}_{-0.19}$|1.96149.6/159J022504.5−043706|$2.2^{+1.5}_{-1.1}$|1.2477.7/91
J022015.5−045654|$2.2^{+1.3}_{-0.94}$|4.80177.4/177J022510.6−043549|$1.4^{+0.61}_{-0.5}$|7.59232.0/260
J022129.0−035359|$0.65^{+1.6}_{-0.62}$|0.659481.4/556J022624.3−041344|$0^{+0.23}_{-0}$|2.0480.5/89
J022145.5−034346|$3.6^{+2.0}_{-1.4}$|3.24495.5/646J022625.2−044648|$1.1^{+0.64}_{-0.51}$|4.39120.2/124
J022154.7−032558|$0.84^{+0.98}_{-0.72}$|9.75159.4/137
3XMM name*N  H  L  2–10  C/dof§3XMM name*N  H  L  2–10  C/dof§
(1022 cm−2)(1044 erg s−1)(1022 cm−2)(1044 erg s−1)
J021502.3−034111|$5.8^{+4.3}_{-3.1}$|2.30101.7/113J022205.0−033238|$7.2^{+3.7}_{-4.5}$|2.21491.7/564
J021529.4−034233|$0.069^{+0.15}_{-0.069}$|1.21298.1/281J022214.4−034619|$0.2^{+0.14}_{-0.12}$|0.688660.0/801
J021532.3−035124|$0.17^{+0.73}_{-0.17}$|2.38116.2/118J022231.7−044910|$2.2^{+2.4}_{-1.5}$|6.6339.0/45
J021541.0−034505|$0.051^{+0.34}_{-0.051}$|0.721142.3/139J022314.5−041017|$0.17^{+0.67}_{-0.17}$|0.75777.3/81
J021606.6−050303|$0.17^{+0.18}_{-0.13}$|0.0613140.7/125J022326.5−041837|$0.064^{+0.21}_{-0.064}$|0.0848158.4/197
J021614.5−050351|$0.84^{+0.82}_{-0.56}$|1.19117.6/122J022330.8−044632|$1.4^{+0.40}_{-0.35}$|7.65280.2/328
J021625.7−050518|$0.17^{+0.41}_{-0.17}$|2.29100.7/122J022331.0−044234|$2.0^{+1.6}_{-1.1}$|5.8079.4/95
J021634.3−050724|$0.23^{+0.22}_{-0.18}$|0.892192.8/215J022334.3−040841|$12^{+7.6}_{-5.1}$|0.861171.3/174
J021642.3−043552|$3.3^{+0.53}_{-0.47}$|21.6465.6/531J022337.9−040512|$3.2^{+1.5}_{-1.1}$|5.00233.0/260
J021644.6−040651|$0.94^{+0.5}_{-0.55}$|2.10188.1/151J022343.3−041622|$0.51^{+0.48}_{-0.11}$|0.437174.5/181
J021705.4−045655|$0.39^{+0.42}_{-0.29}$|1.29108.5/107J022347.1−040051|$1.5^{+2.2}_{-1.3}$|4.70176.4/189
J021705.7−052546|$1.1^{+0.54}_{-0.42}$|1.27150.2/180J022352.0−052421|$0.12^{+0.38}_{-0.12}$|3.2898.7/98
J021721.2−052336|$0^{+0.14}_{-0}$|0.423127.6/129J022353.2−041532|$0.54^{+0.51}_{-0.37}$|0.721246.1/235
J021721.9−043655|$0.92^{+0.55}_{-0.40}$|0.744137.0/161J022358.2−050946|$0.21^{+0.65}_{-0.21}$|1.1486.1/90
J021725.8−051955|$0.40^{+0.52}_{-0.37}$|0.247170.5/145J022405.2−041612|$0.16^{+0.19}_{-0.16}$|1.70337.9/440
J021729.3−052122|$6.5^{+3.5}_{-2.5}$|2.17138.8/137J022408.6−041151|$18^{+10}_{-6}$|1.84232.5/253
J021736.4−050106|$1.00^{+0.81}_{-0.58}$|1.00161.9/157J022410.3−040224|$0.39^{+1.4}_{-0.39}$|1.38131.2/118
J021744.1−034531|$0^{+0.083}_{-0}$|0.6581.9/83J022412.5−035740|$0.46^{+1.2}_{-0.46}$|1.2195.4/72
J021810.1−051844|$0.7^{+1.2}_{-0.7}$|4.3109.6/137J022417.4−041812|$3.8^{+5.5}_{-3.3}$|0.516130.1/144
J021813.2−045051|$0.81^{+0.43}_{-0.31}$|0.261147.3/137J022420.7−041224|$0.15^{+0.20}_{-0.15}$|0.687244.7/302
J021825.6−045945|$9.5^{+3}_{-2.4}$|3.11196.5/203J022421.1−040355|$1.1^{+0.68}_{-0.51}$|1.25246.1/259
J021842.8−051934|$7.3^{+2.8}_{-2.2}$|5.49200.7/246J022500.1−050831|$1.5^{+0.89}_{-0.65}$|0.836116.8/114
J021914.8−045139|$0.19^{+0.34}_{-0.19}$|1.96149.6/159J022504.5−043706|$2.2^{+1.5}_{-1.1}$|1.2477.7/91
J022015.5−045654|$2.2^{+1.3}_{-0.94}$|4.80177.4/177J022510.6−043549|$1.4^{+0.61}_{-0.5}$|7.59232.0/260
J022129.0−035359|$0.65^{+1.6}_{-0.62}$|0.659481.4/556J022624.3−041344|$0^{+0.23}_{-0}$|2.0480.5/89
J022145.5−034346|$3.6^{+2.0}_{-1.4}$|3.24495.5/646J022625.2−044648|$1.1^{+0.64}_{-0.51}$|4.39120.2/124
J022154.7−032558|$0.84^{+0.98}_{-0.72}$|9.75159.4/137

*Observation ID and assumed Galactic absorption column density are the same as in table 4.

Intrinsic absorption column density at source redshift in units of 1022 cm−2. Photometric or spectroscopic (when available) redshifts are assumed in the spectral fits.

X-ray luminosity in 2–10 keV corrected for the Galactic and intrinsic absorption in units of 1044 erg s−1. Photometric or spectroscopic (when available) redshifts are assumed.

§  C statistic/degrees of freedom.

Table 5.

Results of absorbed power law fits to X-ray spectra.

3XMM name*N  H  L  2–10  C/dof§3XMM name*N  H  L  2–10  C/dof§
(1022 cm−2)(1044 erg s−1)(1022 cm−2)(1044 erg s−1)
J021502.3−034111|$5.8^{+4.3}_{-3.1}$|2.30101.7/113J022205.0−033238|$7.2^{+3.7}_{-4.5}$|2.21491.7/564
J021529.4−034233|$0.069^{+0.15}_{-0.069}$|1.21298.1/281J022214.4−034619|$0.2^{+0.14}_{-0.12}$|0.688660.0/801
J021532.3−035124|$0.17^{+0.73}_{-0.17}$|2.38116.2/118J022231.7−044910|$2.2^{+2.4}_{-1.5}$|6.6339.0/45
J021541.0−034505|$0.051^{+0.34}_{-0.051}$|0.721142.3/139J022314.5−041017|$0.17^{+0.67}_{-0.17}$|0.75777.3/81
J021606.6−050303|$0.17^{+0.18}_{-0.13}$|0.0613140.7/125J022326.5−041837|$0.064^{+0.21}_{-0.064}$|0.0848158.4/197
J021614.5−050351|$0.84^{+0.82}_{-0.56}$|1.19117.6/122J022330.8−044632|$1.4^{+0.40}_{-0.35}$|7.65280.2/328
J021625.7−050518|$0.17^{+0.41}_{-0.17}$|2.29100.7/122J022331.0−044234|$2.0^{+1.6}_{-1.1}$|5.8079.4/95
J021634.3−050724|$0.23^{+0.22}_{-0.18}$|0.892192.8/215J022334.3−040841|$12^{+7.6}_{-5.1}$|0.861171.3/174
J021642.3−043552|$3.3^{+0.53}_{-0.47}$|21.6465.6/531J022337.9−040512|$3.2^{+1.5}_{-1.1}$|5.00233.0/260
J021644.6−040651|$0.94^{+0.5}_{-0.55}$|2.10188.1/151J022343.3−041622|$0.51^{+0.48}_{-0.11}$|0.437174.5/181
J021705.4−045655|$0.39^{+0.42}_{-0.29}$|1.29108.5/107J022347.1−040051|$1.5^{+2.2}_{-1.3}$|4.70176.4/189
J021705.7−052546|$1.1^{+0.54}_{-0.42}$|1.27150.2/180J022352.0−052421|$0.12^{+0.38}_{-0.12}$|3.2898.7/98
J021721.2−052336|$0^{+0.14}_{-0}$|0.423127.6/129J022353.2−041532|$0.54^{+0.51}_{-0.37}$|0.721246.1/235
J021721.9−043655|$0.92^{+0.55}_{-0.40}$|0.744137.0/161J022358.2−050946|$0.21^{+0.65}_{-0.21}$|1.1486.1/90
J021725.8−051955|$0.40^{+0.52}_{-0.37}$|0.247170.5/145J022405.2−041612|$0.16^{+0.19}_{-0.16}$|1.70337.9/440
J021729.3−052122|$6.5^{+3.5}_{-2.5}$|2.17138.8/137J022408.6−041151|$18^{+10}_{-6}$|1.84232.5/253
J021736.4−050106|$1.00^{+0.81}_{-0.58}$|1.00161.9/157J022410.3−040224|$0.39^{+1.4}_{-0.39}$|1.38131.2/118
J021744.1−034531|$0^{+0.083}_{-0}$|0.6581.9/83J022412.5−035740|$0.46^{+1.2}_{-0.46}$|1.2195.4/72
J021810.1−051844|$0.7^{+1.2}_{-0.7}$|4.3109.6/137J022417.4−041812|$3.8^{+5.5}_{-3.3}$|0.516130.1/144
J021813.2−045051|$0.81^{+0.43}_{-0.31}$|0.261147.3/137J022420.7−041224|$0.15^{+0.20}_{-0.15}$|0.687244.7/302
J021825.6−045945|$9.5^{+3}_{-2.4}$|3.11196.5/203J022421.1−040355|$1.1^{+0.68}_{-0.51}$|1.25246.1/259
J021842.8−051934|$7.3^{+2.8}_{-2.2}$|5.49200.7/246J022500.1−050831|$1.5^{+0.89}_{-0.65}$|0.836116.8/114
J021914.8−045139|$0.19^{+0.34}_{-0.19}$|1.96149.6/159J022504.5−043706|$2.2^{+1.5}_{-1.1}$|1.2477.7/91
J022015.5−045654|$2.2^{+1.3}_{-0.94}$|4.80177.4/177J022510.6−043549|$1.4^{+0.61}_{-0.5}$|7.59232.0/260
J022129.0−035359|$0.65^{+1.6}_{-0.62}$|0.659481.4/556J022624.3−041344|$0^{+0.23}_{-0}$|2.0480.5/89
J022145.5−034346|$3.6^{+2.0}_{-1.4}$|3.24495.5/646J022625.2−044648|$1.1^{+0.64}_{-0.51}$|4.39120.2/124
J022154.7−032558|$0.84^{+0.98}_{-0.72}$|9.75159.4/137
3XMM name*N  H  L  2–10  C/dof§3XMM name*N  H  L  2–10  C/dof§
(1022 cm−2)(1044 erg s−1)(1022 cm−2)(1044 erg s−1)
J021502.3−034111|$5.8^{+4.3}_{-3.1}$|2.30101.7/113J022205.0−033238|$7.2^{+3.7}_{-4.5}$|2.21491.7/564
J021529.4−034233|$0.069^{+0.15}_{-0.069}$|1.21298.1/281J022214.4−034619|$0.2^{+0.14}_{-0.12}$|0.688660.0/801
J021532.3−035124|$0.17^{+0.73}_{-0.17}$|2.38116.2/118J022231.7−044910|$2.2^{+2.4}_{-1.5}$|6.6339.0/45
J021541.0−034505|$0.051^{+0.34}_{-0.051}$|0.721142.3/139J022314.5−041017|$0.17^{+0.67}_{-0.17}$|0.75777.3/81
J021606.6−050303|$0.17^{+0.18}_{-0.13}$|0.0613140.7/125J022326.5−041837|$0.064^{+0.21}_{-0.064}$|0.0848158.4/197
J021614.5−050351|$0.84^{+0.82}_{-0.56}$|1.19117.6/122J022330.8−044632|$1.4^{+0.40}_{-0.35}$|7.65280.2/328
J021625.7−050518|$0.17^{+0.41}_{-0.17}$|2.29100.7/122J022331.0−044234|$2.0^{+1.6}_{-1.1}$|5.8079.4/95
J021634.3−050724|$0.23^{+0.22}_{-0.18}$|0.892192.8/215J022334.3−040841|$12^{+7.6}_{-5.1}$|0.861171.3/174
J021642.3−043552|$3.3^{+0.53}_{-0.47}$|21.6465.6/531J022337.9−040512|$3.2^{+1.5}_{-1.1}$|5.00233.0/260
J021644.6−040651|$0.94^{+0.5}_{-0.55}$|2.10188.1/151J022343.3−041622|$0.51^{+0.48}_{-0.11}$|0.437174.5/181
J021705.4−045655|$0.39^{+0.42}_{-0.29}$|1.29108.5/107J022347.1−040051|$1.5^{+2.2}_{-1.3}$|4.70176.4/189
J021705.7−052546|$1.1^{+0.54}_{-0.42}$|1.27150.2/180J022352.0−052421|$0.12^{+0.38}_{-0.12}$|3.2898.7/98
J021721.2−052336|$0^{+0.14}_{-0}$|0.423127.6/129J022353.2−041532|$0.54^{+0.51}_{-0.37}$|0.721246.1/235
J021721.9−043655|$0.92^{+0.55}_{-0.40}$|0.744137.0/161J022358.2−050946|$0.21^{+0.65}_{-0.21}$|1.1486.1/90
J021725.8−051955|$0.40^{+0.52}_{-0.37}$|0.247170.5/145J022405.2−041612|$0.16^{+0.19}_{-0.16}$|1.70337.9/440
J021729.3−052122|$6.5^{+3.5}_{-2.5}$|2.17138.8/137J022408.6−041151|$18^{+10}_{-6}$|1.84232.5/253
J021736.4−050106|$1.00^{+0.81}_{-0.58}$|1.00161.9/157J022410.3−040224|$0.39^{+1.4}_{-0.39}$|1.38131.2/118
J021744.1−034531|$0^{+0.083}_{-0}$|0.6581.9/83J022412.5−035740|$0.46^{+1.2}_{-0.46}$|1.2195.4/72
J021810.1−051844|$0.7^{+1.2}_{-0.7}$|4.3109.6/137J022417.4−041812|$3.8^{+5.5}_{-3.3}$|0.516130.1/144
J021813.2−045051|$0.81^{+0.43}_{-0.31}$|0.261147.3/137J022420.7−041224|$0.15^{+0.20}_{-0.15}$|0.687244.7/302
J021825.6−045945|$9.5^{+3}_{-2.4}$|3.11196.5/203J022421.1−040355|$1.1^{+0.68}_{-0.51}$|1.25246.1/259
J021842.8−051934|$7.3^{+2.8}_{-2.2}$|5.49200.7/246J022500.1−050831|$1.5^{+0.89}_{-0.65}$|0.836116.8/114
J021914.8−045139|$0.19^{+0.34}_{-0.19}$|1.96149.6/159J022504.5−043706|$2.2^{+1.5}_{-1.1}$|1.2477.7/91
J022015.5−045654|$2.2^{+1.3}_{-0.94}$|4.80177.4/177J022510.6−043549|$1.4^{+0.61}_{-0.5}$|7.59232.0/260
J022129.0−035359|$0.65^{+1.6}_{-0.62}$|0.659481.4/556J022624.3−041344|$0^{+0.23}_{-0}$|2.0480.5/89
J022145.5−034346|$3.6^{+2.0}_{-1.4}$|3.24495.5/646J022625.2−044648|$1.1^{+0.64}_{-0.51}$|4.39120.2/124
J022154.7−032558|$0.84^{+0.98}_{-0.72}$|9.75159.4/137

*Observation ID and assumed Galactic absorption column density are the same as in table 4.

Intrinsic absorption column density at source redshift in units of 1022 cm−2. Photometric or spectroscopic (when available) redshifts are assumed in the spectral fits.

X-ray luminosity in 2–10 keV corrected for the Galactic and intrinsic absorption in units of 1044 erg s−1. Photometric or spectroscopic (when available) redshifts are assumed.

§  C statistic/degrees of freedom.

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