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Type: Task
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Status: Done (View Workflow)
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Priority: Normal
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Resolution: Done
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Affects Version/s: None
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Fix Version/s: None
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Component/s: None
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Labels:
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Sprint:EngRun16May
Please make a plan with priority for the data acquisition in May 2024 run (run16).
The calibration data taken regularly among the run:
https://sumire.pbworks.com/w/page/156874332/Calibration%20Data%20from%20Run%2016
- masterBiases
- masterDarkes
- Bootstrap?
- Check detectorMap using IIS (see also
PIPE2D-1426)
- Check detectorMap using IIS (see also
- Arc/Trace to make detectorMap
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- (What YM heard by Kiyoto is) Shortest exposure it enough for each lamp
(longer exposure looked saturated), and 3 frames (instead of 5 frames) are enough. - i.e., w/ brn, 10s Ar, 45s Xe, 10s Ne, 70s Kr, 45s HgCd, 45s Trace
w/ bmn, 10s Ar, 45s Xe, 10s Ne, 45s Kr, 45s Trace
- (What YM heard by Kiyoto is) Shortest exposure it enough for each lamp
- Trace to make fiberProfile
- Take one ditheredFlat for mod4 group1, having mod16 trace.
- Using mod16 trace, check if extraction is reasonable
- Using ditheredFlat, make one profile and compare?
- If extraction is not good, take the other three groups.
--> it turns our that we should take new fiberProfiles (because of thermal cycle of the cameras)
- Take one ditheredFlat for mod4 group1, having mod16 trace.
Other data (to understand instrument)
- Quartz data to study InR dependency (
PIPE2D-1283) - Quartz data to monitor fiber-to-fiber throughput variation.
- Twilight
- At different rotator angle. Quartz data is needed at the same rotator angle.
- All-sky field
- All-F-star field
- Else?
- relates to
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PIPE2D-1426 Plan for QA check of calibration in May 2024 run
- Done