wiki:docs/CommissioningPlan/P3.4

Version 4 (modified by kradhakrishnan, 4 years ago) (diff)

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P3.4 Telescope control – focal plane geometry estimation

  • Phase : 3
  • Status : Draft
  • Category : Nighttime testing (functionality and operability) (C4)
  • Recurrence : once at commissioning
  • Duration : 1 night

Description

  • For the correct telescope mode for SHARK-NIR, find the offset direction & magnitude (for the field-stabilized mode), verify the proper image orientation, pixel scale, field of view, and distortion at the SCICAM. Note that this may be performed with and without AO running.

Prerequisites

  • Atmospheric conditions: should be able to see bight stars on sky (preferably close to zenith?).
  • Authorize SHARK-NIR on the SX side.
  • Suitable binary or astrometric targets.
  • AO running for part of the test.

Procedure

  1. Procedure for image orientation
    • Select a filter
    • Place the de-rotator in the nominal "zero" position.
    • Issue a preset to move to a bright star (but not too bright to saturate)
    • Center the star in the science channel
    • Issue a pure elevation offset to the TCS of ca. 5” and verify expected motion direction on the SCICAM
    • Return to the on-axis position and repeat with a pure azimuth motion.
    • Issue a preset to move to a suitable astrometric binary (typically 5-8 arcsec separation) and center one star in the science channel.
    • Based on the published coordinates of the binary, issue the appropriate offset to center the other star.
  2. Procedure for pixel scale/ plate scale
    • Select a filter
    • Issue a preset to move to a suitable astrometric binary to measure pixel scale (typically 5-8 arcsec separation)
    • Center the binary in the upper half of the SCICAM and take several frames. Average these frames
    • Move the binary to the lower half of the SCICAM and repeat.
    • Use the difference image (optionally flat-fielded) to verify the expected pixel scale. This gives two measures.
    • Repeat this for other filters.

Success criteria

  • The image orientation is as expected. The pixel scale and field of view of the SCICAM are as expected.

Notes LBTO support

  • Support from telescope operator (if needed).
  • Presence of John Hill usually helps while collimating for the first time.

Associated SHARK-NIR personnel

Date performed and by whom