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Table 1

X-ray observations of the DOGs sample.

LID PID RA Dec z f2−10 keV Cts(Chandra) Cts (XMM)
(1) (2) (3) (3) (4) (5) (6) (7)

95 325 53.0349 –27.6796 5.22 4.3 257 385
117 (225) 53.0491 –27.7745 1.51 2.5 964
170 53.0720 –27.8189 1.22 0.1 20
197 140 53.0916 –27.8532 1.81 0.6 125 126
199 (193) 53.0923 –27.8032 2.45 0.6 213
230 53.1052 –27.8752 2.61 0.1 48
232 283 53.1070 –27.7183 2.291 4.6 1791 2279
293 53.1394 –27.8744 3.88 0.2 81
307 102 53.1467 –27.8883 1.90 1.6 697 332
309 172 53.1488 –27.8211 2.579 1.2 129 131
321 118 53.1573 –27.8700 1.603 13.0 7661 9253
326 53.1597 –27.9313 3.10 0.8 254
346 64 53.1703 –27.9297 1.221 5.8 1549 1581
397 (74) 53.2049 –27.9180 2.28 2.1 510

Notes. The columns are: (1) Chandra ID from the Luo et al. (2010) catalogue. (2) XMM ID from the Ranalli et al. (2013) catalogue; numbers in brackets denote sources that are detected by XMM-Newton but with a limited number of counts (so no spectral fit has been carried out). (3) X-ray coordinates (J2000). (4) Redshift: two decimal and three decimal digits denote photometric and spectroscopic redshifts, respectively. (5) 2–10 keV Chandra flux in units of 10-15erg cm-2 s-1 from the Luo et al. (2010) catalogue. (6) Background subtracted Chandra counts in the total band 0.3–8 keV (7) Background subtracted XMM-Newton EPIC(MOS+pn) counts in the 0.3–8 keV band.

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