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Table 3

MCXC-I cluster pairs at a separation distance of less than θ500, that are considered as the same object in MCXC-II.

MCXC Sub-catalogue Distance Redshift L500 Note
ID1 ID2 ID1 ID2 (′) 500) ID1 ID2 MCXC ID1 ID2
J0034.2–0204 J0034.6–0208 SGP REFLEX 6.75 0.70 0.0822 0.0812 0.0822 1.24 1.28 Simbad; XMM , C
J0125.4+0145 J0125.4+0144 NORAS BCS 1.8 0.09 0.0183 0.0181 0.0183 0.042 0.061 XMM
J1010.2+5430 J1010.2+5429 400SD_SER NORAS 0.9 0.10 0.047 0.045 0.047 0.013 0.076 NED,PSPC pointed; A,
J1058.1+0135 J1058.2+0136 REFLEX 400SD_SER 1.9 0.17 0.0398 0.0385 0.0398 0.084 0.068 NED; XMM
J1311.7+2201 J1311.5+2200 NORAS eBCS 2.8 0.60 0.1716 0.266 0.1716 1.00 2.48 XMM; B,C
J1652.9+4009 J1652.6+4011 NORAS eBCS 3.8 0.66 0.1492 0.1481 0.1492 1.67 1.57 NED; Chandra; C
J2350.5+2929 J2350.5+2931 NORAS BCS 2.0 0.33 0.1498 0.095 0.1498 2.03 2.66 NED; B

Notes. Columns 1–2: name of each cluster. Columns 3–4-: source catalogue. Columns 5–7: redshift in source catalogue; final MCXC-II redshift. Columns 8–9: L500 luminosity computed from the flux at the final redshift. Column 10: Notes, where we indicate whether the duplicate was identified by NED or Simbad, respectively, and the existence of XMM-Newton, Chandra, or ROSAT-PSPC pointed observations. Cases of differences in L500 (A), in redshift (B), or of large positional offset as compared to θ500 (C) are flagged and discussed in Appendix A.2.

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