Flare-like events in the soft energy band at MJD= 55320, 55390, 55460, and 55530
are due to comtamination by the up-left source GX 339-4. Please ignore them.
GX 339-4 was bright during this period and the orientation of the
"soft tail" by the detector performance rotates around GX 339-4
in every 70 days (the presession period of the ISS orbit).
The "soft tail" interferes with the XTE J1650-500 region in every 70 days.
After 55600 MJD, GX 339-4 was quiet and there was no interference.
The daily, weekly and monthly images are created for every day.
The spectrum is not available for this source.
The data was processed with version 1.4, where both 1650V and 1550V data are used.
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