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Table A.4.

Identified candidates for obscured AGN.

Designation RA Dec Error Fx (0.2–12 keV) eFx HR2 HR3 HR4 XMM_id
– ° ° ″ × 10−11 erg cm−2 s−1 erg cm−2 s−1 – – – –
J002523.92−712322.4 6.3497 −71.3896 0.1059 0.0065 0.0010 0.055 −0.42 0.27 –
J002606.42−711301.6 6.5267 −71.2171 0.1505 0.0042 0.0007 −0.490 −0.54 0.43 –
J002636.61−712409.5 6.6525 −71.4027 0.1365 0.0022 0.0002 0.180 −0.80 −0.06 –
J004226.41−730417.5 10.6101 −73.0716 0.0558 0.0035 0.0005 −0.200 0.03 0.43 J004226.3−730418
J004633.42−734443.2 11.6393 −73.7453 0.1022 0.0027 0.0005 0.460 −0.28 0.23 J004632.9−734444
J005231.59−704705.5 13.1317 −70.7849 0.1003 0.0047 0.0010 0.360 −0.69 0.34 J005232.3−704708
J005334.75−750404.0 13.3948 −75.0678 0.0633 0.0100 0.0020 0.063 −0.57 0.41 J005334.5−750406
J005415.32−743153.0 13.5638 −74.5314 0.1259 0.0037 0.0003 0.053 −0.54 0.19 J005415.5−743153
J005749.70−732547.0 14.4571 −73.4297 0.0433 0.0028 0.0005 0.095 −0.23 0.55 J005750.2−732542
J005859.72−711457.2 14.7489 −71.2492 0.0654 0.0079 0.0020 0.230 −0.58 0.10 J005859.7−711458
J010033.38−715037.2 15.1391 −71.8437 0.1435 0.0024 0.0005 −0.009 −0.43 0.45 J010033.4−715039
211.16703.311 15.5600 −73.2739 1 0.0054 0.0010 0.480 −0.84 0.71 –
211.16765.212 15.6450 −72.9061 1 0.0045 0.0010 0.690 −0.58 0.12 J010234.7−725425
J011420.98−722328.4 18.5874 −72.3912 0.1812 0.0030 0.0004 0.450 −0.55 0.22 J011421.3−722327
J011606.88−731725.0 19.0287 −73.2903 0.0981 0.0038 0.0009 1 −0.36 0.46 J011606.7−731725
J011732.79−735228.6 19.3867 −73.8746 0.1794 0.0042 0.0020 0.340 −0.38 0.34 –
J012024.93−734720.3 20.1039 −73.7890 0.1024 0.0030 0.0007 0.430 −0.38 0.15 –
J012938.05−742144.8 22.4086 −74.3625 0.1208 0.0070 0.0010 0.040 −0.61 0.27 –
J013119.92−742505.7 22.8330 −74.4183 0.1324 0.0028 0.0005 0.190 −0.84 0.70 –
J013254.61−743954.3 23.2276 −74.6651 0.0870 0.0071 0.0020 0.500 −0.49 0.40 –

Notes. The designation, RA, Dec, associated error and the X and Y colours correspond to the ALLWISE or HMQ/MILLIQUAS source. The X-ray flux and the associated error (Fx and eFx) are from the corresponding X-ray counterpart. HR2 HR3 and HR4 refer to the hardness ratios in the energy range of 0.5–1, 1–2 and 2–4.5 keV, respectively. XMM_ids correspond to sources already included in Sturm et al. (2013a).

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