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Table 1

X-ray observations of XMMU J010147.5-715550.

ObsID MJD F in (0.2–1.0) keV ML Exp.
(10-16 erg cm-2 s-1) (ks)

0123110201 51 650.9 92.8  ±  11.9 88.0 17.9
0123110301 51 651.3 74.3  ±  13.7 31.5 11.7
0135720601 52 014.1 99.3  ±  16.6 36.0 13.4
0135720801 52 269.0 32.0  ±  10.5 5.8 27.6
0135720901 52 385.0 25.1  ±  11.1 6.6 10.1
0135721001 52 412.5 12.4  ±  8.8 2.1 9.4
0135721001 52 412.7 66.1  ±  29.8 2.9 7.5
0135721101 52 560.3 15.1  ±  11.8 0.0 23.1
0135721301 52 622.3  <11.1 0.2 28.4
0135721401 52 749.8  <12.4 0.1 30.4
0135721501 52 939.5  <9.7 0.1 24.2
0135721701 52 959.4  <7.4 0.0 25.2
0135721901 53 123.5  <12.3 0.2 33.0
0135722001 53 304.5  <11.2 1.4 31.6
0135722101 53 316.3 8.6  ±  5.0 0.6 24.0
0135722301 53 317.1  <26.5 0.0 14.0
0135722401 53 292.6  <20.8 0.0 30.4
0135722501 53 478.1  <15.0 0.0 23.8
0135722601 53 679.5  <7.9 0.0 29.0
0135722701 53 845.3 17.5  ±  10.9 1.3 30.2
0412980101 54 044.2  <9.2 0.1 31.0
0412980201 54 215.7  <11.8 0.0 19.6
0412980301 54 399.6 12.0  ±  6.7 0.1 35.0
0412980501 54 575.6  <16.7 0.0 22.0
0412980701 54 785.0  <13.9 0.0 28.6
0412980801 54 934.2  <15.3 0.0 6.5
0412980901 55 125.5 15.4  ±  10.0 0.5 28.6
0412981001 55 307.2 27.2  ±  16.6 0.2 27.3

Notes. Combined EPIC-pn and EPIC-MOS source detection. Fluxes are calculated from count rates by assuming the best-fit black-body model. Uncertainties are for 1σ. For observations marked with , the source was not covered by EPIC-pn, but both MOS cameras. For observations, marked with , the source was in the FoV of EPIC-MOS2 only. In all other observations, the source was observed with all EPIC instruments.

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