All Tables
- Table 1:
Best-fit parameters and 68% confidence limits for various fits to
the combined EPIC data. The basic model used was a power-law with
neutral absorption fixed at the Galactic level
(
cm-2). Added to this was either i) a
neutral, solar abundance absorber at z=0.351, ii) a neutral,
solar abundance absorber at variable redshift, iii) an ionised,
solar abundance absorber at variable redshift or iv) a neutral
variable abundance absorber at z=0.351. Columns 1-6 are the
fitted model, absorbing column density, redshift, abundance and
ionisation parameter, and the
statistic over the number
of degrees of freedom for the fit.