Changes between Version 29 and Version 30 of docs/CommissioningPlan/P2.6

Timestamp:

10/31/22 14:23:37 (2 years ago)

Author:

mbergomi

Comment:

--

docs/CommissioningPlan/P2.6

@@ -5 +5 @@
 - **Category**  :       Daytime testing (functionality and operability) (C3)
 - **Recurrence**        :       after instrument installation at telescope platform
-- **Duration**  :       1/2 day
+- **Duration**  :       1 day
 
 **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") 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.
-- Before or after the previous test, we will also perform a short test (about 30 mins long) to find the center of the field. 
+- 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.
+- 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.
+- 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.
 
 **Procedure for the Tip-Tilt internal fast loop test**
 - Use ARGOS light source (to be used only at zenith) and direct light towards SHARK-NIR.
 - Close the SOUL AO loop to have the best ASM shape. Keep the ASM static with the best shape.
+Test A1.
 - Close the SHARK-NIR internal tip-tilt loop.
-- Take 10mins of data at the CRED2 (at loop frame rate) and SCICAM.
-- Introduce 0.5" seeing at the ASM and close the loop.
+- Take 10mins of data at the CRED2 (at loop frame rate) and SCICAM at 500 Hz.
+- Introduce 0.5" seeing at the ASM and close the loop at 500 hz.
 - Close the SHARK-NIR internal tip-tilt loop.
+
+Test A2.
+Repeat test A1 with 1000Hz.
+
+Test B1.
 - Take 10mins of data at the CRED2 and SCICAM.
 - Introduce 0.8" seeing at the ASM and close the loop.
 - Close the SHARK-NIR internal tip-tilt loop.
 - Take 10mins of data at the CRED2 and SCICAM.
-- Repeat the above steps for the selected brightness of the Argos light source
+
+Test B2.
+Repeat test A1 with 1000Hz.
+
+Test C.
+- Repeat the above steps of test B for the differnet selected brightness of the Argos light source (TBC which magnitudes, noting that max brightness should be mag 9th in R band)
 
 **Procedure for finding the field center**
@@ -39 +51 @@
 - The center of field estimated.
 
-**Notes**
-- For the SN team: know in advance how many minutes of data can be downloaded from CRED2 or the ring-buffer size.
-
 **LBTO support**
 - Authorize SHARK-NIR