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13.1 Analyzing Individual Observations

Sometimes an FGS observer may find that a single observation requires a detailed investigation, such as a particular star in a POSITION mode observation that appears on one or more plate overlays with large, unexplained residuals. The object might not be a single star as originally assumed, or perhaps a stellar flare occurred while the target was being tracked in FineLock. Either of these cases might become readily apparent through close inspection of the FineLock vs. Coarse Track centroids in the first case or the photometry data in the second case.

The interactive graphics tool fgs_plotter can display a variety of FGS quantities as functions of other data. For example, you can display the location of the IFOV in pickle coordinates as a function of x vs. y, or the fine error signal (partial S-curve) as a function of x during the WalkDown to FineLock. This tool works with guide star data as well as astrometry data.

The fgs_plotter tool is both versatile and essential for analyzing failed observations and retrieving useful data from marginal observations. For example, Figure 13.1, generated with fgs_plotter, shows a failed observation in which the FGS was not able to acquire a star in FineLock because the fine error signal (Sx) did not exceed the necessary threshold. The tool can also be a valuable eductional aid for an observer who is unfamiliar with FGS data. Figure 13.2 shows the menu of functions in FGS_PLOTTER that are available to the observer.

Figure 13.1: Example of a Failed Observation Analyzed with FGS_PLOTTER

Figure 13.2: Options Available in FGS_PLOTTER



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