Changes between Version 24 and Version 25 of docs/CommissioningPlan/P2.6
- Timestamp:
- 09/28/22 09:25:35 (2 years ago)
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docs/CommissioningPlan/P2.6
v24 v25 8 8 9 9 **Description** 10 - To verify the SHARK-NIR internal fast tip-tilt loop (using CRED1 and SHARK-NIR ALPAO DM) using the ARGOS light source (only at zenith) for various seeing conditions simulated at the ASM. This test will verify if the correction of the fast tip-tilt loop is affected by residual of the turbulence, for stardifferent magnitudes.10 - To verify the SHARK-NIR internal fast tip-tilt loop (using CRED1 and SHARK-NIR ALPAO DM) using the ARGOS light source (only at zenith) for various seeing conditions 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. 11 11 12 12 **Prerequisites** … … 17 17 - Close the SOUL AO loop to have the best ASM shape. Keep the ASM static with the best shape. 18 18 - Close the SHARK-NIR internal tip-tilt loop. 19 - Take 10mins of data at the CRED2 and SCICAM.19 - Take 10mins of data at the CRED2 (at loop frame rate) and SCICAM. 20 20 - Introduce 0.5" seeing at the ASM and close the loop. 21 21 - Close the SHARK-NIR internal tip-tilt loop.