Table 2: Spectral analysis results for GRB 040106 with SPI and IBIS/ISGRI for two intervals around the prominent peaks of emission. Errors quoted are for 1 parameter of interest at 1 $\sigma$ confidence level. Fluxes are quoted for the energy range 20-200 keV. Within the large errors on the spectral fits, results are consistent between instruments.
Interval Parameter SPI IBIS / ISGRI

1st pulse Photon index -1.47^+0.52_-0.59 $-1.70\pm0.12$

(9 s) Flux (erg cm^-2 s^-1) $5.9\times10^{-8}$ $2.5\times10^{-8}$

2nd pulse Photon index -1.32^+0.31_-0.34 $-1.41\pm0.1$

(8 s) Flux (erg cm^-2 s^-1) $6.1\times10^{-8}$ $3.2\times10^{-8}$

**Table 2:** Spectral analysis results for GRB 040106 with SPI and IBIS/ISGRI for two intervals around the prominent peaks of emission. Errors quoted are for 1 parameter of interest at 1 $\sigma$ confidence level. Fluxes are quoted for the energy range 20-200 keV. Within the large errors on the spectral fits, results are consistent between instruments.
Interval	Parameter	SPI	IBIS / ISGRI
1st pulse	Photon index	-1.47^+0.52_-0.59	$-1.70\pm0.12$
(9 s)	Flux (erg cm^-2 s^-1)	$5.9\times10^{-8}$	$2.5\times10^{-8}$
2nd pulse	Photon index	-1.32^+0.31_-0.34	$-1.41\pm0.1$
(8 s)	Flux (erg cm^-2 s^-1)	$6.1\times10^{-8}$	$3.2\times10^{-8}$

Source LaTeX | All tables | In the text

	1 Introduction
	2 INTEGRAL observations and results
	3 XMM-Newton
	4 Discussion
	5 Conclusion
	References