Table 2.

Galactic column densities for the BALQSOs and XMM–Newton observations used in the construction of the X-ray spectra. Column densities are taken from the Leiden/Argentine/Bonn Survey of Galactic H i (Kalberla et al. 2005). The column labelled ‘Counts’ gives the total number of net (i.e. background-subtracted) 0.2–12 keV counts used in the combined EPIC spectrum for each source.

SourceNHCountsObservation IDFiltersExposure time (ks)
(1020 cm−2)pnMOS1MOS2pnMOS1MOS2
XWAS J0050072.581970123920101Medium14.9
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.36.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101ThinThin4.54.5
XWAS J0050442.391330123920101Medium15.4
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.26.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101MediumThin1.74.5
XWAS J0152391.543410112300101ThinThinThin16.124.625.7
0602010101ThinThinThin71.187.387.7
XWAS J0152571.29720109540101MediumMediumMedium42.053.052.9
XWAS J0226452.31780112681301ThinThinThin9.616.716.7
XWAS J0507542.612370110980801ThinThinThin30.139.039.2
SourceNHCountsObservation IDFiltersExposure time (ks)
(1020 cm−2)pnMOS1MOS2pnMOS1MOS2
XWAS J0050072.581970123920101Medium14.9
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.36.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101ThinThin4.54.5
XWAS J0050442.391330123920101Medium15.4
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.26.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101MediumThin1.74.5
XWAS J0152391.543410112300101ThinThinThin16.124.625.7
0602010101ThinThinThin71.187.387.7
XWAS J0152571.29720109540101MediumMediumMedium42.053.052.9
XWAS J0226452.31780112681301ThinThinThin9.616.716.7
XWAS J0507542.612370110980801ThinThinThin30.139.039.2
Table 2.

Galactic column densities for the BALQSOs and XMM–Newton observations used in the construction of the X-ray spectra. Column densities are taken from the Leiden/Argentine/Bonn Survey of Galactic H i (Kalberla et al. 2005). The column labelled ‘Counts’ gives the total number of net (i.e. background-subtracted) 0.2–12 keV counts used in the combined EPIC spectrum for each source.

SourceNHCountsObservation IDFiltersExposure time (ks)
(1020 cm−2)pnMOS1MOS2pnMOS1MOS2
XWAS J0050072.581970123920101Medium14.9
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.36.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101ThinThin4.54.5
XWAS J0050442.391330123920101Medium15.4
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.26.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101MediumThin1.74.5
XWAS J0152391.543410112300101ThinThinThin16.124.625.7
0602010101ThinThinThin71.187.387.7
XWAS J0152571.29720109540101MediumMediumMedium42.053.052.9
XWAS J0226452.31780112681301ThinThinThin9.616.716.7
XWAS J0507542.612370110980801ThinThinThin30.139.039.2
SourceNHCountsObservation IDFiltersExposure time (ks)
(1020 cm−2)pnMOS1MOS2pnMOS1MOS2
XWAS J0050072.581970123920101Medium14.9
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.36.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101ThinThin4.54.5
XWAS J0050442.391330123920101Medium15.4
0125320401MediumMediumMedium17.021.421.4
0125320501ThinMediumMedium3.56.26.2
0125320701MediumThinThin10.514.814.7
0133120301ThinThinThin6.510.710.7
0133120401ThinThinThin7.310.710.6
0153950101MediumThin1.74.5
XWAS J0152391.543410112300101ThinThinThin16.124.625.7
0602010101ThinThinThin71.187.387.7
XWAS J0152571.29720109540101MediumMediumMedium42.053.052.9
XWAS J0226452.31780112681301ThinThinThin9.616.716.7
XWAS J0507542.612370110980801ThinThinThin30.139.039.2
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