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Table 3:

All EPIC-pn observations in full frame mode with the thin filter of RX J0720.4-3125 with the derived variations of the pulse averaged spectra.
Orbit MJD kT EW radius
    [eV] [eV] [km]
78 51 677 86.5 $\pm$ 0.4 -4.0 $\pm$ 4.0 4.79 $\pm$ 0.09
175 51 870 86.0 $\pm$ 0.7 +5.6 $\pm$ 7.0 4.90 $\pm$ 0.14
533/534 52 585/7 88.4 $\pm$ 0.4 -16.8 $\pm$ 3.3 4.70 $\pm$ 0.07
711 52 940 92.0 $\pm$ 0.6 -64.7 $\pm$ 5.4 -
815 53 148 94.6 $\pm$ 0.5 -58.6 $\pm$ 4.2 4.29 $\pm$ 0.08
986 53 489 94.3 $\pm$ 0.4 -57.8 $\pm$ 3.8 4.35 $\pm$ 0.07
1060 53 636 93.7 $\pm$ 0.5 -55.0 $\pm$ 3.8 4.37 $\pm$ 0.08
1086 53 687 93.1 $\pm$ 0.5 -55.9 $\pm$ 3.8 4.50 $\pm$ 0.08
1181 53 877 93.1 $\pm$ 0.6 -51.2 $\pm$ 4.8 4.44 $\pm$ 0.10
1265 54 045 92.7 $\pm$ 0.6 -53.6 $\pm$ 4.7 4.53 $\pm$ 0.11
1356 54 226 92.4 $\pm$ 0.6 -44.1 $\pm$ 4.9 4.45 $\pm$ 0.11
1454 54 421 91.8 $\pm$ 0.6 -44.6 $\pm$ 4.6 4.50 $\pm$ 0.10
Observations done in different observing modes, which were not used for the fit are in italic. The radius obtained from observation 711 is not used at all (see explanation at the end of Sect. 5). All errors correspond to 90% confidence level.

Source LaTeX | All tables | In the text

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