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Table 10

X-ray count rates.

Mission – Instrument HJD Observed count rate Relative Simulated count rate Relative Energy
error deviation1 range
–2 440 000 (10-2 cts s-1) (%) (10-2 cts s-1) (%) keV

XMM–Newton MOS2 15 686.713 5.42 ± 0.18 3.3 4.97 ± 0.15 8.4 0.2–10
15 694.768 5.03 ± 0.18 3.6 5.00 ± 0.16 0.5 0.2–10
15 700.152 5.54 ± 0.17 3.1 5.14 ± 0.15 7.1 0.2–10
XMM–Newton pn 15686.713 17.95 ± 0.41 2.3 15.87 ± 0.34 11.6 0.2–10
15 694.768 15.28 ± 0.40 2.6 15.84 ± 0.35 –3.7 0.2–10

Einstein–IPC2 3972.050 1.00 ± 0.40 40.0 2.09 ± 0.20 –109.4 0.2–4.5
ROSAT All Sky Survey 8210.000 3.26 ± 0.873 26.7 3.20 ± 0.57 1.8 0.1–2
ROSAT PSPC 6928.585 4.50 ± 0.50 11.1 2.66 ± 0.25 40.8 0.1–2
9508.604 3.30 ± 0.50 15.2 2.54 ± 0.26 23.1 0.1–2
ROSAT HRI 9669.924 1.17 ± 0.11 9.8 1.68 ± 0.06 –43.6 0.1–2
Swift 15 635.350 1.75 ± 0.42 24.1 1.20 ± 0.24 31.5 0.3–10
Chandra 15 213.113 6.58 ± 0.12 1.8 6.30 ± 0.10 4.3 0.2–10

Notes.

(1)

The relative error corresponds to 100 × (obs−simulation)/obs. The count rates have been obtained with XSPEC.

(2)

Values from Pollock (1987).

(3)

This value is in good agreement with the one derived by Pollock et al. (1995) who reported a ROSAT All Sky Survey PSPC count rate of (3.26 ± 0.87) × 10-2 cts s-1. Note that ROSAT HRI had little or no energy resolution.

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