Table A.1

Summary of the fluxes for all point sources within 60″ of the cluster centre.

XXLID Class z RA Dec Flux Resolved Separation from
XXL (J2000) (J2000) (10−14 erg s−1 cm−2) by XMM cluster centre (″)
XLSSC 072a C1 1.00 33.852 −3.726 <0.08 No 8
XLSSC 029a C1 1.05 36.002 −4.225 0.04 No 52
36.012 −4.229 0.05 No 23
XLSSC 005a C1 1.06
3XLSS J021825.9-045947 C1 1.13 34.609 −4.996 0.27 No 5
XLSSC 122a C1 1.99

XLSSC 048a C2 1.01
XLSSC 073a C2 1.03 33.749 −3.515 0.08 No 37
33.737 −3.519 0.37 3XLSS J021456.8-033108 53
3XLSS J022755.7-043119 C2 1.05 36.972 −4.516 0.05 No 10
36.984 −4.521 0.11 No 43
36.994 −4.520 0.61 3XLSS J022758.7-043110 44
3XLSS J021320.3-053411 C2 1.08 33.331 −3.571 0.12 No 11
XLSSC 203 C2 1.08 34.429 −4.988 0.10 No 4
XLSSC 634 C2 1.08 355.692 −54.185 0.20 No 4
355.704 −54.185 0.22 No 29
355.683 −54.177 1.30 3XLSS J234244.2-541033 34
355.687 −54.175 0.09 3XLSS J234244.2-541033 36
355.712 −54.176 0.04 No 54
3XLSS J021325.0-042000 C2 1.20
3XLSS J022005.5-050826a C2 1.65 35.022 −5.140 0.15 No 5
35.021 −5.139 0.01 No 10
35.030 −5.137 0.07 No 29
35.014 −5.134 0.04 No 41
3XLSS J022418.4-043956a C2 1.67

XLSSC 034 C3 1.04 35.372 −4.093 1.00 3XLSS J022129.1-040534 22
35.375 −4.111 0.15 No 45
3XLSS J022059.0-043922a C3 1.11 35.247 −4.656 1.52 No 5
XLSSC 046a C3 1.22
3XLSS J022351.3-041841 C3 1.27
3XLSS J021700.4-034746a C3 1.54 34.253 −3.795 0.41 No 8
34.258 −3.784 0.07 No 50
3XLSS J022812.3-043836a C3 1.67 37.051 −4.651 0.10 3XLSS J022812.2-043906 25
37.045 −4.648 0.22 No 26
3XLSS J022554.3-045059a C3 2.24 36.477 −4.851 0.13 No 5
36.472 −4.846 0.24 No 20
36.471 −4.837 0.89 3XLSS J022552.8-045013 50

Notes. Column 6: individual point source flux as calculated from the Chandra data with 1σ errors. All fluxes are in the 0.5–2 keV energy band. XXLIDs marked with (a) appear in Willis et al. (2013) and are therefore part of the XMM-LSS subset of clusters. Column 7 states whether the Chandra detected point source was previously resolved by XXL and thus excluded from the F60 measurements; for cases where the point source was resolved by XXL, its name as in XXL Paper XXVII is provided. In the case of XLSSC 634, two sources were blended into one by the XMM PSF, reported as one point source by XXL, and were masked from the F60 calculation.

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