wiki:docs/CommissioningPlan/P3.9

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).