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P4.6

-                      v4
+                      v5
 **Procedure**
+•       ?
+•       After pre-set and acquisition of the target we will run on flux calibration template with the star off-centered from the coronagraph (short templete - few minutes). To this a centering
+        observation follows with the Fourier mode on the DM allowing the creation of four satellite spots (around 5% of the target brightness). Also this template is short.
+        We then perform the scientific coronagraphic observation using pupil stabilized observing mode. This observation should be taken during the passage of the star to the meridian to maximize
+        the rotation of the FOV and allow to implement ADI. This part should be long at least 1:20-1:30 hours. The observation is closed running again centering and flux calibration with the same
+        modalities adopeted at the beginning of the observations.
 **Notes**