Table 4: Multi-wavelength spectral fits of the prompt phase of GRB 060124.

Time/Instrument		 Model $N_{\rm H}^{z}$ Photon index $E_{\rm p}$ Normalization $\chi^2_{\rm red}$ (d.o.f.) Start End
Selectiona   (1022 cm-2)   (keV) (ph cm-2 s-1 keV-1)   (s) (s)

BAT Precursor		 PL   $1.8 \pm$ 0.2   (3.4 $\pm$ 0.4) $\times$ 10-3 b 0.88 (57) -1.5 13.5
XRT-BAT Bin 1 PL <4.0 $1.17 \pm 0.07$   (7.2 $\pm$ 1.1) $\times$ 10-3 b 0.96 (70) 301.2 361.2
XRT-BAT Bin 2 PL 2.8 -0.8+0.9 $1.44 \pm 0.03$   (1.26 $\pm$ 0.09) $\times$ 10-3 b 0.97 (137) 361.2 451.2
XRT-BAT-Konus Bin 3 CPL 3.5 -0.4+0.5 $1.36 \pm 0.02$ 132 -18+29 (3.0 $\pm$ 0.2) $\times$ 10-3 c 1.09 (404) 451.2 571.2
XRT-BAT-Konus Bin 4 CPL 1.6 $\pm$ 0.3 $1.45 \pm 0.02$ 237 -69+153 (1.7 $\pm$ 0.1) $\times$ 10-3 c 0.99 (431) 571.2 691.2
XRT-BAT-Konus Bin 5 CPL 1.9-0.4+0.3 1.78+0.03-0.08 28 -8+10 4.1 -0.5+1.4 $\times$ 10-4 c 0.83 (393) 691.2 811.2
XRT-BAT-Konus (1-5) CPL 1.9 $\pm$ 0.2 $1.48 \pm$ 0.02 193 -39+78 $(1.19 \pm 0.07) \times 10^{-3}$ c 1.06 (618) 301.2 811.2
a See Fig. 9. b Normalization (K) at 50 keV. c Normalization (K) at 100 keV.

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