All Tables

Table 1: Characteristics of the observations of HESS J1745-303 with HESS (Aharonian et al. 2006a) and XMM-Newton. The ``full'' dataset is what is presented here, while the 2006 subset was presented by Aharonian et al. (2006d). The energy range for the HESS case is the range used to fit the statistically significant spectral points; the full sensitivity of the detector extends to approximately 100 TeV.
Table 2: Integral fluxes of the three test regions A, B, and C (shown in Fig. 1), compared with the total integral flux from the full source. The photon index $\Gamma$ is derived from a fit to the spectrum for each region. Note that region A is chosen to correspond with the molecular cloud position and radius described in Sect. 5.1.
Table 3: Sources detected using the detection algorithm emldetect. The parameters given here are for the energy range between 0.5 and 10 keV. Column 2: name recommended by the XMM-Newton SOC and the IAU for source detections. Columns 3 and 4: J2000.0 coordinates. Units of right ascension are hours, minutes, and seconds, and units of declination are degrees, arc-minutes, and arc-seconds. Column 5: error on the source position in arc-seconds. Column 6: number of counts in EMOS1 and EMOS2 within a 10 $^{\prime \prime }$ integration region using events above 0.5 keV. Column 7: statistical significance of the detection derived with emldetect. Column 8: source flux above 0.5 keV in $10^{-14}~{\rm erg~cm^{-2}~s^{-1}}$ .