Table 4
Source-flux-independent parameters, the iron line equivalent widths, the parameters
of the Galactic ridge emission, and the HEXTE calibration constant as determined
from the combined spectral analysis (
).
| TBnew | N H | 
× 1022 cm -2 |
| BBODY | kT |  keV |
| CUTOFFPL | E fold |  keV |
| Iron line | W 2005 |  eV |
| W 2007 |  eV |
|
| W 2011 |  eV |
|
| Constantsa | c HEXTE |
|
| c XRT |
|
|
| c XIS0 |
|
|
| c XIS1 |
|
|
| c XIS3 |
|
|
| c PIN |
|
|
| c GSO |
|
|
| BREMSS b | kT |  keV |
| F 3 - 10 keV | 
× 10-12 erg s-1 cm-2 |
|
| Blended iron linesb | E |  keV |
| σ |  keV |
|
| F | 
× 10-4 photons s-1 cm-2 |
Notes.
Component belongs to the Galactic ridge emission and is applied to RXTE-PCA only (Eq. (5)).
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