Version 8 (modified by elcarolo, 3 years ago) (diff) |
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P3.9 NCPA working and performance & checking for pupil shifts
- Phase : 3
- Status : Draft
- Category : Nighttime testing (functionality and operability) (C5) + Nighttime testing for performance (C7)
- Recurrence : once at commissioning
- Duration : 3 nights
Description
- Evaluate the NCPA working and performance using the baseline approach, phase-diversity approach using the Wollaston prism & dual-band imaging, and measurement of NCPA using SHARK-NIR internal calibration sources.
Prerequisites
- Atmospheric conditions: TBD
- Authorize SHARK-NIR on the SX side.
- AO is working.
- Target(s) at different Zenith distances with different magnitudes.
- lookup tables of already calibrated NCPA measurements.
Procedure
- Acquire a star of a given magnitude, start SOUL-AO, followed by the internal-TT loop.
- 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 (already calibrated). Take images at SCICAM.
- 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) to confirm that the alignment of SHARK-NIR is still good. This would mean that the NCPA already calibrated is not good enough!
- 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.
- Check the pupil position by inserting the pupil lens.
- Repeat for a different star (of various magnitudes and for a different telescope elevation). It is also good to do this for other seeing conditions.
Templates
- SHARKNIR_di_cal_NCPA (not released)
Success criteria
- NCPA estimated and applied on the ASM / ALPAO DM.
- Cross-check the NCPA performances with the daytime activity P2.6.
- The total residual after NCPA correction should be <30nm.
Notes
LBTO support
- AO support
Date performed and by whom
comment
- perform for 5 cases e.g. Rmag 8, 10, 10, 12, 14. These five cases where the star has different mag and at different zenith angles over different nights (so different seeing).