Version 1 (modified by kradhakrishnan, 5 years ago) (diff) |
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P3.18 Large spatial scale instrument and telescope flat field
- Phase : 3
- Status : Draft
- Category : Nighttime testing (functionality and operability) (C4)
- Recurrence : before every night observations (valid for all observing modes). 2/day for CI (BB filter only).
- Duration : 1 hour(s)
Description
- Flat field taken during twilight
Prerequisites
- Authorize SHARK-NIR on the SX side.
- Atmospheric conditions: AO working conditions.
- Bad pixel map, Background or Dark.
Procedure
- This calibration is performed by sky observation combined with pointing scan in order to record a flat (that include telescope large scale transmission variations) on the detector.
- Single integration times for a given setup, using various flux level with natural light with no coronagraph.
Success criteria
- Width of flux distribution: 3.10-2
Notes
- Same as activity 7.5 in AD4
LBTO support
- Support from LBTI/LBTO?
Associated SHARK-NIR personnel
- JF, LM, MdP
Date performed and by whom