All Tables

Table 1: Log of XMM-Newton observations and data of EXO 0748-676 used in this paper. From left to right: observation number for this paper, observation date with start and end time, the camera (EPIC-MOS1 or EPIC-pn) with mode and filter, and exposure time.
Table 2: Peak count rates of the 12 observed type I X-ray bursts in the soft (0.3-2 keV) and hard (2-10 keV) X-ray bands, together with their hard/soft ratio. Indicated is whether the bursts occurred during intervals of reduced dipping or full dipping (corresponding to the lowest count rates in the soft band, and, as opposed to reduced dips, sometimes also visible as dips in the hard band). For bursts I, II, and VII this was not completely clear. See Fig. 1 for the labeling (I-XII) of the bursts.
Table A.1: Time and count rate selections used for our spectral analysis. These selections are also displayed in Fig. A.1. Note that the eclipse (E) is excluded from the L1 count rate selection.
Table A.2: Spectral fit results. Models and energy ranges are given for each of the fits. Lower limits on ABB are 90% confidence. All other errors represent 1 $\sigma$ confidence intervals.
Table A.3: Spectral fit results. Models and energy ranges are given for each of the fits. All errors represent 1 $\sigma$ confidence intervals.