All Tables
- Table 1:
XMM- Newton and Chandra net number of counts (background
subtracted) collected by each instrument in the specifiedextraction region
and spectral range.
- Table 2:
XMM- Newton EPIC-PN spectral fitting results when the thermal
emission model is applied (2 APEC: two temperature model; 3 APEC: three
temperature model). The last column displays the result of the combined
PN+MOS fit with the 3 APEC model. Fluxes are given in units of
10-13 erg cm-2 s-1, luminosities in units of
1043 erg s-1; both are corrected for absorption.
* denotes a fixed parameter.
- Table 3:
XMM- Newton EPIC-PN spectral fitting results using the
photoionized gas model described in the text. Fluxes are given in units of
10-13 erg cm-2 s-1, luminosities in units of
1043 erg s-1; both are corrected for absorption.
* denotes a fixed parameter.
- Table 4:
Chandra ACIS-S spectral fitting results when the thermal
emission model (Model 1) and the photoionized gas model (Model 2) are applied
to the spectrum of the inner 10''. The last column refers to the
spectrum of the extended hot gas halo instead. Fluxes are given in units of
10-13 erg cm-2 s-1, luminosities in units of
1043 erg s-1; both are corrected for absorption.
* denotes a fixed parameter.