Table 4.
Clump candidate properties.
| ID | RA | Dec | Nbins | σ | F0.7 − 2 keV | Area | Hardness ratio | Possible |
|---|---|---|---|---|---|---|---|---|
| (photon cm−2 s−1) | (arcsec2) | source | ||||||
| C1 | 13:48:06.18 | +26:25:36.96 | 1 | 2.03 | (5.30 ± 0.78)×10−6 | 4992 |
 |
… |
| C2 | 13:47:34.57 | +26:31:43.49 | 1 | 2.22 | (1.88 ± 0.21)×10−6 | 2573 |
 |
QSO |
| C3 | 13:50:18.07 | +26:40:50.04 | 1 | 2.23 | (1.12 ± 0.11)×10−5 | 13694 |
 |
QSO |
| C4 | 13:48:07.42 | +26:16:38.06 | 5 | 3.75 | (9.02 ± 0.58)×10−6 | 5766 |
 |
GClstr |
| C5 | 13:47:23.09 | +26:22:41.29 | 9 | 3.65 | (7.42 ± 0.36)×10−6 | 5009 |
 |
G (A1795 member) |
| C6 | 13:48:36.82 | +27:01:20.64 | 2 | 3.27 | (1.67 ± 0.17)×10−6 | 1388 |
 |
G |
| C7 | 13:50:47.17 | +26:27:46.04 | 6 | 2.82 | (4.90 ± 0.26)×10−6 | 6323 | … | GGroup |
| C8 | 13:48:09.90 | +26:09:42.93 | 1 | 2.06 | (1.86 ± 0.17)×10−6 | 3559 |
 |
QSO |
| C9 | 13:46:55.73 | +26:22:37.15 | 1 | 2.10 | (5.31 ± 0.75)×10−7 | 1027 | … | QSO |
| C10 | 13:48:44.71 | +27:05:16.77 | 1 | 2.09 | (7.93 ± 0.95)×10−7 | 1482 |
 |
QSO |
| C11 | 13:50:51.15 | +26:21:09.22 | 1 | 2.09 | (5.95 ± 0.74)×10−7 | 1189 |
 |
QSO(?) |
| C12 | 13:46:45.91 | +26:47:24.09 | 1 | 2.55 | (2.26 ± 0.19)×10−6 | 3401 | … | GClstr |
| C13 | 13:46:36.96 | +26:27:24.04 | 1 | 3.18 | (1.32 ± 0.20)×10−6 | 1386 |
 |
QSO |
| C14 | 13:48:06.73 | +26:04:44.26 | 1 | 2.20 | (1.33 ± 0.20)×10−6 | 2430 |
 |
QSO/GClstr |
| C15 | 13:50:25.01 | +26:10:16.26 | 2 | 2.84 | (2.58 ± 0.21)×10−6 | 3300 |
 |
QSO |
| C16 | 13:48:17.21 | +26:03:29.99 | 2 | 4.17 | (3.73 ± 0.34)×10−6 | 2232 |
 |
G/QSO |
| C17 | 13:49:51.01 | +27:06:25.29 | 11 | 4.60 | (1.36 ± 0.06)×10−5 | 6352 |
 |
GClstr |
| C18 | 13:47:30.44 | +27:03:37.55 | 1 | 2.85 | (1.19 ± 0.18)×10−6 | 1190 |
 |
QSO |
| C19 | 13:47:13.59 | +27:01:26.47 | 1 | 2.38 | (8.84 ± 1.33)×10−7 | 1559 | … | clump(?)/G |
| C20 | 13:46:42.98 | +26:54:21.56 | 1 | 8.18 | (1.21 ± 0.23)×10−6 | 82 |
 |
QSO |
| C21 | 13:47:15.25 | +27:05:22.13 | 1 | 2.61 | (8.82 ± 1.47)×10−7 | 1326 |
 |
QSO |
| C22 | 13:47:22.56 | +27:07:36.14 | 1 | 2.45 | (8.11 ± 1.28)×10−7 | 1429 | … | GClstr(?) |
| C23 | 13:51:50.11 | +26:27:39.34 | 1 | 2.11 | (6.21 ± 0.63)×10−6 | 12427 | … | ... |
| C24 | 13:47:45.51 | +25:56:34.98 | 1 | 2.25 | (3.13 ± 0.45)×10−6 | 6222 |
 |
... |
Notes. Nbins shows the number of adjacent contbin bins forming a single source, and σ represents the candidate’s significance measured in units of the log-normal fit’s standard deviation in the host annulus. The possible source of the candidates’ emission is also reported following the notation used in NED. For details, see Appendix A.
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