All Tables

Table A.1: M 83 sources detected at the 3- $\sigma$ level in the 0.3-8.0 keV band, and respective net fluxes in a soft, medium and hard band. Counts in a given band are given in brackets when the source was detected at less than 3- $\sigma$ level in that band. The exposure time was 50.851 ks. The ROSAT cross-identification refers to the HRI sources listed by Immler et al. (1999); SW02 is the cross-identification with Soria & Wu (2002).
Table B.1: XSPEC best-fit parameters for the galactic nucleus (No. 63 in Table A.1). Here and hereafter, the Galactic line-of-sight column density has been fixed at $4.0\times 10^{20}$ cm^-2.
Table B.2: XSPEC best-fit parameters for the two brightest supersoft sources. (An asterisk indicates that we could not determine an error for that fit parameter.)
Table B.3: XSPEC best-fit parameters for emission-line sources. (Parameters listed as "undetermined'' are those for which we could not obtain meaningful values with XSPEC.)
Table B.4: XSPEC best-fit parameters for other selected bright sources in the ACIS-S3 chip. (An asterisk indicates that we could not obtain a meaningful best-fit value for that parameter.)