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A good first step in checking the output is to examine the light curve plot for
both the source and background, making sure they are reasonable: no isolated,
unusually high (or low) values, and no frequent drop-outs. Users should also check
the image with fv or ds9 in the Fast mode window to see if the
source is near an edge. If it is, it's a good idea to examine the light curves from
diffent exposures to verify that they are consistent from exposure to exposure (while
keeping in mind any intrinsic source variability). If the image is blurred or
unusual in any way, users should check the tracking history file to verify the tracking
was reliable.
Figure 9.2:
Left: The processed FAST mode sky image. Right: the light curve
produced automatically by omfchain.
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Lynne Valencic
2011-07-26