Results of the spectral fits for the three types of fits performed (Table 3). The three panels on the top line provide the variations with phase of the spectral parameters (norm in units 10^-3 cm^-5, kT in keV, and N_H in units 10²² cm^-2) while the three panels on the bottom line yield observed fluxes in units 10^-12 erg cm^-2 s^-1. The panel pairs in the left, middle, and right columns correspond to results from single temperature fits, two-temperature fits with solar abundances, and two-temperature fits with non-solar abundances, respectively.