The “Make track curve” dialog is used to display spatial offsets of the source frames as a function of time. This curve is used to check the precision of a telescope mount. The offsets are relative to the reference frame, they are computed separately in X and Y direction.
Making a track-list
(1) The list of available data sets is displayed here.
The actual data set is shown here.
Click the “Save” button (3) to save the light curve to the file.
See also