GX 3+1

Light curves
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Remarks
Flare-up in 56190 - 56270 is by contamination of the bright transient
Swift J174510.8-262411 (ATel #4383). The flare around 56782 is by
another south-west source. The jump-up at 57000 and 59400 are by GRO J1750-27
(ATel #14930). The jumps are clearly seen in 10-20 keV band, and about 0.07 ph/cm2/s
in the band.


The data is updated in every day.
The data was processed with version 7.7L, where both 1650V and 1550V data
are used.
Evaluation of the shadow of solar paddles are improved. This decreased the
number of dropping data points.
A-system camera 0 (gas leaking camera) is also used until 57900 MJD.
There, 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 normal cameras.
After 57900 MJD, A-system Camera 0 is no-longer used in version 7L,
and the data have smaller error bars, although data gaps appears
for some sources.


Light curve Data
1orbit LC
1day LC
please visit v7l page for previous data.

README for light curve data