The making of the observations is described in the technical notes n°3, n°4 and n°5. The result of an observation is, most of time, under the form of a succession of images dated in UTC. One will then have to determine the light flux of the occulted or eclipsed satellite on each image and to plot a light curve of the flux against the time showing the variation of the light flux during the events (cf. the technical note n°5).

As an example, we will provide here soon images in fits format to be analyzed. You will be able to plot the corresponding light curve and make the same with your own observations. Images may be recorded in several formats: fits or video movies in avi. If you are not able to analyze your data, please send your files of images to phemu@imcce.fr together with a report of the observation to be made on the special form.