All Tables
- Table 1:
List of sources that are detected in the area covered by the
Cartwheel system and displayed in
Fig. 1. Unabsorbed fluxes are computed in the 0.5-2 keV
and 2-10 keV bands assuming the best fit model of the sum of point
sources (see text for details).
Unabsorbed, k-corrected luminosities in erg s-1 are in the 2-10 keV
band.
The sources are also reported in the
Appendix in RA order for completeness; however, in the Appendix the fluxes
are all computed under a different spectral hypothesis (see text).
These sources are identified by their number in the last column of
Table A.1 for easy reference.
- Table 2:
Spectral fit results for source N.10.
- Table A.1:
Sources detected by the wavelet algorithm in the S3 field of view.
Count rates have been converted into flux by assuming a power law with
index
and Galactic low energy absorption
cm-2. An X-ray spectral analysis is presented in the
text for sources indicated with *.