Table 2: The HBS28 sample.
name Observation ID Gal. $N_{\rm H}$ CR $_{4.5{-}7.5~\rm keV}$ EPIC cameras Notes
    ($\times$1020) ($\times$10-3)    
    [cm-2] [s-1]    
XBS J002618.5+105019 0001930101 5.07 2.3 MOS2, MOS1, pn  
XBS J013240.1-133307 0084230301 1.64 3.2 MOS2, MOS1, pn  
XBS J013944.0-674909 0032140401 2.49 2.0 MOS2, MOS1, pn  
XBS J014100.6-675328 0032140401 2.49 70.9 MOS2, MOS1 a
XBS J015957.5+003309 0101640201 2.59 3.8 MOS2, MOS1, pn  
XBS J021640.7-044404 0112371701 2.42 2.1 MOS2, MOS1, pn  
XBS J021808.3-045845 0112371001* 2.52 2.7 MOS2, MOS1, pn  
XBS J021817.4-045113 0112371001* 2.52 3.3 MOS2, MOS1, pn  
XBS J021822.2-050615 0112371001* 2.52 4.5 MOS2, MOS1, pn  
XBS J023713.5-522734 0098810101 3.28 3.2 MOS2, MOS1, pn  
XBS J030206.8-000121 0041170101 7.16 3.1 MOS2, MOS1, pn  
XBS J030614.1-284019 0042340501 1.36 4.6 MOS2, MOS1 e
XBS J031015.5-765131 0122520201 8.21 4.4 MOS2, MOS1, pn  
XBS J031146.1-550702 0110970101 2.55 5.9 MOS2, MOS1, pn  
XBS J031859.2-441627 0105660101 2.60 2.2 MOS2, pn c
XBS J033845.7-352253 0055140101 1.31 2.4 MOS2, MOS1, pn  
XBS J040658.8-712457 0111970301 7.57 3.4 MOS2, MOS1, pn b
XBS J040758.9-712833 0111970301 7.57 5.0 MOS2, pn c
XBS J041108.1-711341 0111970301 7.57 2.2 MOS2, MOS1 a, b
XBS J185613.7-462239 0067340101 5.29 8.2 MOS2, MOS1, pn  
XBS J193248.8-723355 0081341001 5.95 4.5 MOS2, MOS1, pn  
XBS J204043.4-004548 0111180201 6.72 3.2 MOS2, MOS1, pn  
XBS J205635.7-044717 0112190601 4.96 2.1 MOS2, MOS1 e
XBS J205829.9-423634 0081340401 3.89 3.9 MOS2, MOS1, pn  
XBS J213002.3-153414 0103060101 4.99 2.3 MOS2, MOS1 d
XBS J213824.0-423019 0061940201 2.68 2.5 MOS2, MOS1 e
XBS J214041.4-234720 0008830101 3.55 3.3 MOS2, MOS1, pn  
XBS J220601.5-015346 0012440301 6.13 2.3 MOS2, MOS1 d
Column 1: source name;

Col. 2: identification number of the corresponding XMM observation;

Col. 3: Galactic column density;

Col. 4: source count-rate in the 4.5-7.5 keV energy band;

Col. 5: EPIC cameras used for the spectral analysis (see notes);

Col. 6: notes.

a = source on a gap in the pn.

b = MOS1 and MOS2 not summed.

c = source on a gap in MOS1.

d = source outside the pn field of view.

e = problems with the pn data.

* for the spectral analysis we have summed these data with the 0112370101 sequence.


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