Changes between Version 12 and Version 13 of docs/CommissioningPlan/P3.10

Timestamp:

02/26/21 12:22:45 (4 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P3.10

@@ -17 +17 @@
 •       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.
+* Check the phase diversity NCPA approach using Wollaston prism + DI-DBI (already calibrated). Take images at SCICAM.
+* Measure the phase diversity NCPA approach using Wollaston prism + DI-DBI  and using real star (need to do on the spot, but script exists). Take images at SCICAM.
+* Digression: If the PSF after applying the calibrated NCPA is bad, we could close the SHARK-NIR shutter (can have the SOUL-AO running parallel) and do a quick internal NCPA measurement (either till the NCPA modal coefficients or until the new shape on ALPAO-DM). Confirm that the alignment of SHARK-NIR is still good.
 * Check the pupil position inserting the pupil lens.
 * 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.