Table D.1
X-ray catalogue properties of the selected cluster candidates.
| OBSID | 2XMMp... | EP_EXTENT | 3XMM-DR6... | EP_EXTENT | M1/M2/PN |
| [″] | [″] | [ks] | |||
|
|
|||||
| 0041170101 | J030212.0-000133 | 9.3 ± 1.3 | J030212.1-000132 | 8.5 ± 1.3 | 46.7/46.7/37.3 |
| 0092800101 | J083026.2+524133 | 18.4 ± 1.1 | J083026.2+524133 | 18.8 ± 1.1 | 16.3/16.4/12.4 |
| 0092800201 | J083026.2+524133 | 16.48 ± 0.4 | J083026.2+524133 | 16.18 ± 0.43 | 71.9/72.3/62.3 |
| 0502220201 | – | – | J083026.2+524133 | 18.47 ± 0.57 | 56.1/61.4/37.2 |
| 0502220301 | – | – | J083026.2+524133 | 17.64 ± 0.5 | 72.4/73.3/58.4 |
| 0085150101 | J084836.4+445345 | 9.7 ± 1.9 | J084836.1+445343 | 12.6 ± 2.1 | 39.8/39.8/36.4 |
| 0085150201 | J084836.4+445345 | 0.0 ± 0.0 | J084836.1+445343 | 0.0 ± 0.0 | 19.3/19.2/17.9 |
| 0085150301 | – | – | J084836.1+445343 | 0.0 ± 0.0 | –/–/22.3 |
| 0085150101 | J084858.3+445158 | 12.29 ± 0.86 | J084858.4+445158 | 12.41 ± 0.9 | 39.8/39.8/36.4 |
| 0085150201 | J084858.3+445158 | 13.9 ± 1.2 | J084858.4+445158 | 10.15 ± 0.95 | 19.3/19.2/17.9 |
| 0085150301 | J084858.3+445158 | 8.7 ± 1.3 | J084858.4+445158 | 10.3 ± 1.4 | –/–/22.3 |
| 0149010201 | J092120.2+371735 | 11.6 ± 1.6 | J092120.2+371735 | 13.1 ± 1.8 | 54.2/54.3/46.4 |
| 0112520101 | J093437.4+551340 | 8.4 ± 1.2 | J093437.5+551342 | 8.30 ± 1.3 | 28.5/28.3/22.4 |
| 0112520201 | – | – | J093437.5+551342 | 9.4 ± 2.1 | 10.4/10.4/9.8 |
| 0085640201 | J093607.2+613245 | 9.98 ± 0.69 | J093607.3+613245 | 9.28 ± 0.69 | |
| 0207130201 | J100451.6+411626 | 6.65 ± 0.24 | J100451.6+411627 | 6.45 ± 0.28 | 33.5/33.5/30.2 |
| 0146990201 | – | – | J105320.2+440815 | 14.9 ± 2.4 | 11/10.9/6.9 |
| 0146990901 | J105319.8+440817 | 13.6 ± 2.3 | J105320.2+440815 | 14.6 ± 2.7 | 5.1/5.5/4 |
| 0022740201 | J105344.2+573517 | 33.9 ± 2.6 | J105343.5+573518 | 26.2 ± 1.50 | 26.7/26.7/23.8 |
| 0123700101 | J105344.2+573517 | 23.8 ± 1.9 | J105343.5+573518 | 30.3 ± 2.1 | 32.8/32.8/29.9 |
| 0123700401 | – | – | J105343.5+573518 | 33.1 ± 3.2 | 12.2/12.4/11.9 |
| 0147510901 | J105344.2+573517 | 28.2 ± 1.4 | J105343.5+573518 | 27.4 ± 1.4 | 40.6/40.5/37.8 |
| 0147511101 | J105344.2+573517 | 27.2 ± 1.2 | – | – | 24.5/24.5/22.7 |
| 0147511301 | J105344.2+573517 | 32 ± 1.9 | J105343.5+573518 | 38.6 ± 2.2 | 15/15/13.9 |
| 0147511601 | J105344.2+573517 | 23.2 ± 1.1 | J105343.5+573518 | 25.9 ± 1 | 98.1/98.4/89.4 |
| 0147511701 | – | – | J105343.5+573518 | 24.5 ± 1.1 | 89.8/89.9/81.7 |
| 0147511801 | J105344.2+573517 | 29.8 ± 1.2 | J105343.5+573518 | 29 ± 1.1 | 65.4/65.5/60.2 |
| 0151400201 | J120735.1+250538 | 6.6 ± 1.3 | J120735.2+250537 | 7.8 ± 1.5 | 13/13.2/9.4 |
| 0151400201 | J120815.5+250001 | 24.2 ± 3.2 | J120816.0+250002 | 20.8 ± 2.7 | 13/13.2/9.4 |
| 0106061001 | J123113.1+1545508 | 20.9 ± 1.7 | J123113.1+154548 | 19.5 ± 1.6 | 5.6/5.6/5 |
| 0200020101 | J123759.3+180332 | 13 ± 1.3 | J123759.2+180335 | 14.4 ± 1.4 | 13.3/13.5/9.7 |
| 0112240301 | J133038.6-013832 | 6.8 ± 1 | J133038.7-013832 | 6.82 ± 0.92 | |
| 0152940101 | J133852.5+044309 | 15.7 ± 1.9 | J133852.4+044309 | 23.2 ± 2.3 | |
| 0055990501 | J133853.9+482033 | 7.6 ± 1.3 | J133854.1+482034 | 6.8 ± 1.2 | 18/18.1/13 |
| 0057560301 | J144854.8+085400 | 15.6 ± 1.5 | J144854.7+085359 | 16.6 ± 1.6 | |
| 0148520101 | – | – | J144854.7+085359 | 15.3 ± 2.3 | |
| 0148520301 | J144854.8+085400 | 29.9 ± 3.6 | J144854.7+085359 | 28.5 ± 3.5 | |
| 0091140201 | J145220.8+165458 | 6.2 ± 1.2 | J145220.6+165457 | 0.0 ± 0.0 | |
| 0103860601 | J151716.8+001302 | 7.6 ± 1.8 | J151716.9+001258 | 8 ± 1.8 | |
| 0201902001 | – | – | J151716.9+001258 | 0.0 ± 0.0 | |
Notes. The OBSIDs for the individual cluster candidates selected in this work are listed in Col. 1. We identify the corresponding X-ray source in the 2XMMp catalogue in Col. 2 and list its extent measured from the respective OBSID in Col. 3. Columns 4 and 5 add the same properties for the 3XMM-DR6 catalogue. We note again that 2XMMp was decisive for the selection of the sample, while the X-ray analysis further included more recent XMM-Newton observations. Differences in source position and extent between the two catalogues can be addressed to updates in their respective reduction procedures. The last column lists the available cleaned exposure time per EPIC instrument for the confirmed clusters, either in this or other works.
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