: X-ray sources that are correlated with photometric candidate members of NGC 2547. The Table is only available electronically and contains 108 rows. The first two rows are shown here as a guide to form and content. Columns are as follows: (1) running source identification number (produced by the SAS analysis system), (2) the conventional [*XMM-Newton*]{} source name, (3), (4) RA and Dec (J2000.0), (5) 1-sigma positional uncertainty of the X-ray source (corrected for a mean astrometry shift and including an additional systematic error – see section 2.2), (6) the maximum likelihood statistic returned by the SAS analysis; then for the pn (7)–(10), MOS1 (11)–(14) and MOS2 (15)–(18) detectors we list the count-rates in the 0.3-3keV, 0.3-1.0keV, 1.0-3.0keV ranges and their uncertainties, followed by a hardness ratio (e.g. defined as \[col.9$-$col.8\]/\[col.9$+$col.8\] for the pn) and its uncertainty.

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                                  HR (M1)                                      HR (M2)                                                                               
       (0.3-3.0)keV            (0.3-1.0)keV            (1.0-3.0)keV                               (0.3-3.0)keV            (0.3-1.0)keV            (1.0-3.0)keV       
           (10)                    (11)                    (12)                  (13)                 (14)                    (15)                    (16)                  (17)
   1.62E-02$\pm$8.15E-04   8.77E-03$\pm$5.89E-04   7.46E-03$\pm$5.62E-04   -0.081$\pm$0.050   1.74E-02$\pm$1.03E-03   9.38E-03$\pm$7.52E-04   8.01E-03$\pm$7.02E-04   -0.079$\pm$0.059
   2.03E-02$\pm$9.37E-04   1.24E-02$\pm$7.26E-04   7.81E-03$\pm$5.93E-04   -0.229$\pm$0.045   2.13E-02$\pm$9.96E-04   1.46E-02$\pm$8.20E-04   6.77E-03$\pm$5.66E-04   -0.365$\pm$0.044
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  : X-ray sources that are correlated with photometric candidate members of NGC 2547. 