Table 3:
List of the 6.5 keV Fe emission line EWs, assuming a fixed line
width of 0.1 keV, for the various X-ray observations covering that
spectral energy. Errors and upper limits are at a 90% confidence level.
Pointings are listed in chronological order from top to bottom.
| Observation |
EW (eV) |
|---|
| EXOSAT I |
<56 |
| EXOSAT II |
<73 |
| RXTE |
48
+13-10 |
| BeppoSAX |
51 
20 |
| Swift |
<1100 |
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