Table 3
Time-selected intervals used for the spectral analysis of Chandra and RXTE observations.
| Spectrum | Tstart − Tstop | HEG rate | RXTE datasets |
| s | cts s-1 | ||
|
|
|||
| Pre-dip | 995–16734 | 24.43 ± 0.04 | 04/03/02 |
| Ingress | 16734–17084 | 19.4 ± 0.6 | NONE |
| Dip | 17084–17784 | 15.2 ± 0.3 | NONE |
| Egress | 17784–18134 | 22.0 ± 0.6 | NONE |
| Post-dip | 18134–30065 | 20.30 ± 0.05 | 01/05 |
Notes. Start and stop times are relative to the start time of the Chandra observation corresponding to 2010-08-01 00:32:37 UTC. The HEG rate is the summed (positive and negative) first-order 1.0–10 keV rate (uncorrected for pile-up).The RXTE/PCA spectra used to cover the broad-band spectrum are listed in the last column.
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