Table 2.
Results of the single power-law spectral fit for observations #4187, 5795, 6262, and 6263.
| Error bars are 90% confidence level | ||||||||
|---|---|---|---|---|---|---|---|---|
| ObsID | Γ | NH | χ2/d.o.f. | Flux | Flux | Luminosity | Luminosity | cnt |
| [1020 cm−2] | [0.5–7.0 keV] | [0.2–12.0 keV] | [0.5–7.0 keV] | [0.2–12.0 keV] | ||||
| 4187 |
 |
 |
24.11/28 |
 |
 |
 |
 |
526 |
| 5795 |
 |
 |
93.07/82 |
 |
 |
 |
 |
1700 |
| 6262 |
 |
 |
123.28/119 |
 |
 |
 |
 |
2541 |
| 6263 |
 |
 |
150.15/141 |
 |
 |
 |
 |
3334 |
Notes. Γ denotes the photon index of the power-law and NH gives the intrinsic hydrogen column density of the source. Fluxes derived from the best fits are in units of 10−12 erg s−1 cm−2. Luminosities are in 1042 erg s−1 and “cnt” is the net count (background subtracted).
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