Changes between Version 5 and Version 6 of docs/CommissioningPlan/P4.6

Timestamp:

02/01/21 15:06:48 (4 years ago)

Author:

dmesa

Comment:

--

docs/CommissioningPlan/P4.6

@@ -23 +23 @@
 
 **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
+•       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