All Tables

Table 2: Coordinates of the detected X-ray point sources with their individual count rates for each of the three detectors, in the 0.4-10 keV range. A missing value means the source is in a gap or out of the field-of-view for this particular detector. The Hardness Ratios ( HRs) were evaluated on the EPIC pn data. The right-hand side of the table shows the results of the correlation with the GSC 2.2 catalog, the 2MASS All-Sky Catalog of Point Sources, and the USNO B1.0 catalog. In these last columns, No. represents the number of counterparts in the correlation region, while d corresponds to the distance between the X-ray source and its counterpart, if unique.
Table 3: X-ray sources previously detected in the field. The number in the first column refers to our internal numbering scheme (see Table 2). Identifications with the 2RXP and 1WGA catalogs have only an indicative value. When there were two entries with the same name in the 1WGA catalog, we kept only the source detected with the smallest off-axis angle, as recommended by the WGA team. The second part of the Table deals with the diffuse extended emissions. Several spurious X-ray sources were detected in the 2RXP and 1WGA catalogs at their position, and we will not list them here.
Table 4: Photometry of the OM counterparts lying within 5 $^{\prime \prime }$ from X-ray sources. The number in the first column refers to our internal numbering scheme (see Table 2).
Table 5: Parameters of the spectral fits for the brightest point sources. Stated errors correspond to the 90% confidence level. The global metallicity was set to $0.3~Z_{\odot}$ , as appropriate for the LMC, for all sources except XMMU J045534.9-661525 (source # 19), for which we adopt solar abundances since it corresponds to a foreground star. Absorbed fluxes are given in the spectral range 0.4-10 keV and in units 10^-14 ergs cm^-2 s^-1. The results correspond to a simultaneous fit of all EPIC spectra available. A constrained fit for XMMU J045744.1-662741 is also listed below.
Table 6: Parameters of the spectral fits for the extended sources. Stated errors correspond to the 90% confidence level. The global metallicity was set to $0.3~Z_{\odot}$ for all sources. Fluxes are given in the spectral range 0.4-10 keV, and in units 10^-14 ergs cm^-2 s^-1. Unabsorbed fluxes are corrected for the fitted N(H). The results correspond to a simultaneous fit of all EPIC spectra, except for the NE source, for which only a pn spectrum was available. Constrained fits are also listed below when the fitted N(H) was outside the "allowed'' range (see Sect. 4.1). Note that solutions with $\chi ^2>2$ were not included.