Version 4 (modified by kradhakrishnan, 3 years ago) (diff) |
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P3.0 Large spatial scale instrument and telescope flat field
- Phase : 3
- Status : Draft
- Category : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
- Recurrence : before every night observations (valid for all observing modes). 2/day for CI (BB filter only).
- Duration : 2 hours
Description
- Flat field is 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 a pointing scan to record a flat (including telescope large scale transmission variations) on the detector.
- Single integration times for a given setup, using various flux levels with natural light with no coronagraph.
Templates
Success criteria
- Width of flux distribution: 3.10-2
Notes
- Same as activity 7.5 in AD4
LBTO support
- Dome open during twilight
Date performed and by whom