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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