Changes between Version 4 and Version 5 of docs/CommissioningPlan/P3.10

Timestamp:

01/21/21 19:34:12 (4 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P3.10

@@ -15 +15 @@
 
 **Procedure**
-•       Acquire star of given magnitude. Start SOUL-AO.
-* Check the working and performance of the NCPA baseline approach. Take images at SCICAM.
-* Check the phase diversity approach using Wollaston prism + DI-DBI. Take images at SCICAM.
-* Check the phase diversity approach (using the internal calibration source). Take images at SCICAM.
-* Repeat for a different star (of different magnitudes and for different elevation of the telescope)
+•       Acquire star of a given magnitude. Start SOUL-AO.
+* Check the working and performance of the NCPA (already calibrated) baseline approach. Take images at SCICAM.
+* Check the phase diversity NCPA approach using Wollaston prism + DI-DBI (need to do on the spot, but script exists). Take images at SCICAM.
+* Check the phase diversity approach using the internal calibration source (already calibrated). Take images at SCICAM.
+* Repeat for a different star (of different magnitudes and for a different elevation of the telescope). It is also good to do this for different seeing conditions.
 
 **Success criteria**