Spectra at the three F35 are consistent with a
single input emission model (BB + PL + gaussian lines) and an absorption
component associated with the intervening matter.
PL index ~0.8-0.9 in the (2-12) keV.
Substructure of the soft
emission: at F35 =0.17, 0.60 we
require two blackbodies, with T~0.1-0.2 keV and T~0.06 keV.
Around ~1 keV we include a
set of lines/edges modeling the most prominent ones resolved, at the same F35, by RGS.