Changes between Version 2 and Version 3 of docs/CommissioningPlan/P4.9

Timestamp:

02/01/21 15:36:29 (4 years ago)

Author:

dmesa

Comment:

--

docs/CommissioningPlan/P4.9

@@ -24 +24 @@
 **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.
+        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**