Details
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Type:
Story
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Status: Done
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Resolution: Done
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Fix Version/s: None
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Component/s: pipe_analysis
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Labels:None
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Story Points:7
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Epic Link:
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Sprint:DRP F19-5, DRP F19-6 (Nov), DRP S20-2 (Jan), DRP S20-3 (Feb), DRP S20-5 (Apr), DRP S20-6 (May), DRP F20-1 (June), DRP F20-2 (July), DRP F20-3 (Aug), DRP F20-5 (Oct), DRP S21a (Dec Jan)
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Team:Data Release Production
Description
Participation in several recent focussed sprints (namely the Per-CCD Astrometry sprint, DM-19943) inspired several additions and updates to the the `pipe_analysis` scripts. This ticket is to implement those features, including:
- overplotting the WCSs on the visit level sky plots computed at different processing stages (including raw/initial/sfm/ubercal)
- plotting the coadd image as a background to the sky plots (in particular to allow for differencing of coadds produced by different processing runs in the compareCoaddAnalysis.py script, but can also be useful as a "quick look" at the image as a persisted png)
- allow for sky plots to have units of RA/Dec and/or "pixels" (focal plane or tract)
- add directional arrows on the visit-level focal plane "pixel" plots
- extra accommodations for non-HSC cameras (DECam, cfht, lsst/DC2)
The updates suggested above were implemented on the ticket branch and served their purpose in the DM-19943 sprint. The branch wasn't merged to master, and need not be since the pipe_analysis repo is in the process of being retired and replaced with analysis_drp, but it can still be used for inspiration for development of analysis_drp if deemed useful for general QAing. Marking as done (but decreasing the SPs a bit).