... listed[*]
Observations G and H are listed for completeness, but are of scarce utility due to their short integration time and presence of contaminating sources in the PDS instrument; they will not be discussed further.
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... analysis[*]
The spectral results for the bursts detected in observation E are reported in Feroci et al. (2004).
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... range[*]
See the Cookbook for BeppoSAX NFI Spectral Analysis, http://www.asdc.asi.it/bepposax/software/cookbook/
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... area[*]
We assume for SGR 1900+14a distance of 15 kpc (Vrba et al. 2000).
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... XTE J1908+94[*]
The source went in outburst in February 2002 and reached its flux peak about two months later (in't Zand et al. 2002).
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... larger[*]
The uncertainty in the relative calibration of the two satellite in the energy band considered here is of $\approx$10% (Kirsch et al. 2005).
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Copyright ESO 2006