Table 8: To evaluate the mean energies of the three analysed bands, we used the spectral indexes of the best-fit power-law models in the [0.6-10] keV ranges ( $\alpha = 1.15\pm 0.01$ and $\alpha = 1.535\pm 0.003$ ). We do not report the errors on the mean energies which are of the order of 10^-4 keV. The notations $\delta _{10}$ and $\xi _5$ mean ( $\delta /10$ ) and $\xi /10^5$ , respectively.
E₁ E₂ E₃ $\tau_{12}$ $\tau_{13}$ B₁₂ B₁₃

(keV) (keV) (keV) (s) (s) (G) (G)

November 14 soft lag

0.42 1.44 5.19 5800 11 600 $0.24\pm0.02~\delta_{10}^{-1/3}$ $0.21\pm0.01~\delta_{10}^{-1/3}$

December 1 hard lag

0.40 1.38 4.87 $450\pm200^*$ $950\pm200^*$ $0.53\pm0.12 ~\delta_{10}^{-1} \xi_5^{2/3}$ $0.65\pm0.08 ~\delta_{10}^{-1} \xi_5^{2/3}$

^* Since the uncertainties reported in Table 5 are probably underestimated,
we assumed more conservative errors of 200 s.

**Table 8:** To evaluate the mean energies of the three analysed bands, we used the spectral indexes of the best-fit power-law models in the [0.6-10] keV ranges ( $\alpha = 1.15\pm 0.01$ and $\alpha = 1.535\pm 0.003$ ). We do not report the errors on the mean energies which are of the order of 10^-4 keV. The notations $\delta _{10}$ and $\xi _5$ mean ( $\delta /10$ ) and $\xi /10^5$ , respectively.
E₁	E₂	E₃	$\tau_{12}$	$\tau_{13}$	B₁₂	B₁₃
(keV)	(keV)	(keV)	(s)	(s)	(G)	(G)
November 14 soft lag
0.42	1.44	5.19	5800	11 600	$0.24\pm0.02~\delta_{10}^{-1/3}$	$0.21\pm0.01~\delta_{10}^{-1/3}$
December 1 hard lag
0.40	1.38	4.87	$450\pm200^*$	$950\pm200^*$	$0.53\pm0.12 ~\delta_{10}^{-1} \xi_5^{2/3}$	$0.65\pm0.08 ~\delta_{10}^{-1} \xi_5^{2/3}$

Source LaTeX | All tables | In the text