Table 2
Results of the X-ray spectral fitting.
(a) Continuum variations | (b) Absorption variations | |||
923/10394 | 15181/15666/15667 | 923/10394 | 15181/15666/15667 | |
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0.94 | 0.95 | ||
T (keV) ... | 0.61 ± 0.03 * | 0.61 ± 0.03 * | ||
N1 ... | (1.2 ± 0.1) × 10-5 * | (1.2 ± 0.1) × 10-5 * | ||
N2 ... | (7.9 ± 0.9) × 10-6 * | (8.2 ± 0.9) × 10-6 * | ||
NH(1022 cm-2) ... | 32.3 ± 1.6 * | 89.7 ± 12.3 | 32.0 ± 1.7 | |
N3 ... | (2.1 ± 0.9) × 10-4 | (1.16 ± 0.08) × 10-3 | (1.14 ± 0.08) × 10-3 * | |
EW(FeKα) (eV) ... | 800 ± 320 | 140 ± 60 | 310 ± 170 | 110 ± 60 |
L(0.5−2 keV) (obs.) ... | 0.67 ± 0.02 | 0.67 ± 0.20 | 0.67 ± 0.02 | 0.67 ± 0.02 |
L(2−10 keV) (obs.) ... | 2.4 ± 0.3 | 20 ± 8 | 3.8 ± 0.4 | 11.9 ± 0.3 |
L(0.5−2 keV) (intr.) ... | 7.3 ± 0.2 | 7.3 ± 0.2 | 36.2 ± 1.1 | 36.2 ± 1.1 |
L(2−10 keV) (intr.) ... | 8.6 ± 1.1 | 46 ± 18 | 45.2 ± 4.7 | 45.2 ± 4.7 |
Notes. X-ray luminosities in units of 1040 erg/s. Normalisations (N1, N2, and N3) are in units of photons keV-1 cm-2 s-1 at 1 keV. Parameters marked with asterisks are set to be tied for all the observations. Including the FeKα slightly improved the final statistic of the fit with a for both continuum and absorption variations (see text).
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