All Tables

Table 1: Source flux value (20-60 keV), significance, average off-axis angle, and exposure time when IGR J16393-4643 is detected at the 4 $\sigma$ level in the mosaic image of a spacecraft revolution. The median MJD of the visibility period is also given in reference to Fig. 4.
Table 2: Parameters from the Compton emission (CE) model fit to the spectra of EPIC and ISGRI combined. Also listed are the values of the CE model (without a blackbody) fit to the pulse and plateau states of the phase-resolved EPIC/PN spectra constrained with the ISGRI spectrum. The integrated fluxes are listed as observed (F_2-10) or unabsorbed ( $F^{{\rm UA}}_{2-10}$ ). Errors denote 90% confidence.