Table 3: RXTE and BeppoSAX simultaneous observations log and spectral fit parameters. We adopted a power law model with fixed absorption parameter: $N_{\rm H}= 2.5\times 10^{21}$ cm-2.
26-27 July
Instrument Time start Time end Duration $\alpha$ $F_{1~\rm keV}$ $F^{*}_{2-10~\rm keV}$ $\chi^2_{\rm r}$/d.o.f.
      (s)   ($\mu$Jy) ( $\times10^{-12}$)  
PCA 26/7/00 26/7/00 2208 0.9+0.7-0.6 1.4 6.3 0.42/25
3-15 keV 18:23:44 19:00:32          
MECS 26/7/2000 27/7/2000 23309 $0.8\pm0.1$ 1.18 5.8 0.86/43
1-10 keV 10:12:39 06:43:33          
30 October-2 November
PCA 2/11/2000 2/11/2000 2000 1.45+0.3-0.25 10.3 19.7 0.45/25
3-15 keV 10:56:16 11:29:36          
MECS 31/10/2000 2/11/2000 33 661 $1.6\pm0.05$ 12.7 19.7 0.61/58
1-10 keV 20:46:55 09:59:28          
* Erg cm-2 s-1.


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