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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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