wiki:docs/CommissioningPlan/P3.4

Version 16 (modified by elcarolo, 3 years ago) (diff)

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P3.4 Pupil alignment

  • Phase : 3
  • Status : Draft
  • Category : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
  • Recurrence : before every observing target (CI, LSS), starting from commissioning.
  • Duration : 2 hours

Description

  • Alignment of the internal pupil image with apodizer (at PP1) or Lyot stop (at PP2) in the coronagraphic mode

Prerequisites

  • Bad pixel map, Background or Dark, Flat-field, detector RON

Procedure

  • The position of the first tip-tilt mirror (IN_TT) is optimized in order to have the first pupil image centered with the apodizer/Lyot stop. This is obtained comparing the pupil image, formed on the SCICAM, with the image of the apodizer, received on the SCICAM using the calibration fiber as a source.

Templates

  • SHARKNIR_gen_tec_PupilApoAlignment (realased)
  • SHARKNIR_gen_tec_PupilLyotAlignment (realased)

Success criteria

  • Expected accuracy: 0.25% of pupil image diameter ~17arcsec of the TTM ~1.5pixel SCICAM ~30μm at the level of the SCICAM.

Notes

  • Same as activity 8.2 in AD4
  • Template: SHARKNIR_gen_tec_PupilAlignment

LBTO support

  • AO support

Date performed and by whom