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 data is updated in every day.
The data was processed with version 6L, where both 1650V and 1550V data
are used. A-system camera 0 (gas leaking camera) and A-system camera 3
and B-system camera 0 (degraded cameras) are also used.
The coverage is increased. However, when A-system camera 0 is used until 57900 MJD,
the flux has a large uncertainty (a few tens of % in 2-4 keV).
Even in 4-10 keV, the data have larger uncertainty than those in
the other cameras.
After 57900 MJD, A-system Camera 0 is no-longer used in version 6L,
and the data have smaller error bars, although data gaps appears
for some sources.
Light curve Data
README for light curve data