Changes between Version 30 and Version 31 of docs/CommissioningPlan/P2.6

Timestamp:

10/31/22 14:49:41 (2 years ago)

Author:

mbergomi

Comment:

--

docs/CommissioningPlan/P2.6

@@ -8 +8 @@
 
 **Description**
-- To verify the SHARK-NIR internal fast tip-tilt loop (using CRED2 and SHARK-NIR ALPAO DM) using the ARGOS light source (only at zenith) for various seeing conditions (0.5", 0.8" [or larger, if possible]) simulated at the ASM. This test will verify if the correction of the fast tip-tilt loop is affected by the residual turbulence for star at different magnitudes.
+- To verify the SHARK-NIR internal fast tip-tilt loop (using CRED2 and SHARK-NIR ALPAO DM) using the ARGOS light source (only at zenith) for various seeing conditions (0.5", 0.8" [or larger, if possible]) simulated at the ASM. This test will verify if the correction of the fast tip-tilt loop is affected by the residual turbulence for star at different magnitudes. In Padova just tip-tilt was injected and it was injected on the DM mirror used also for its correction.
 - Before or after the previous test, we will also perform a short test (about 30 mins long) to find the center of the field while derotating. 
 
 **Prerequisites**
-- Knowledge of Argos light source magnitude and the possibility of tuning its brightness (more info pending from LBTO, jenny?). 
-- For the SN team: know in advance how many minutes of data can be downloaded from CRED2 or the ring-buffer size. Confirm 10 mins are ok.
+- Knowledge of Argos light source magnitude and the possibility of tuning its brightness (more info pending from LBTO, jenny?).  In alternative we can change magnitude with our ND filters.
+- For the SN team: know in advance how many minutes of data can be downloaded from CRED2 or the ring-buffer size. At least barycenter position should be saved, in a format compatible with statistical analyses. Confirm if 10 mins are ok.
 
 **Procedure for the Tip-Tilt internal fast loop test**
@@ -48 +48 @@
 
 **Success criteria**
-- SHARK-NIR fast tip-tilt loop works efficiently within the requirements in all the seeing conditions.
+- SHARK-NIR fast tip-tilt loop works efficiently within the requirements in all the seeing conditions and magnitudes (comparison between open-close loop variation with different  injected turbulence).
 - The center of field estimated.