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  1. PFS observation processing/procedure
  2. OBSPROC-33

Review the pfsDesign generation script in 2022Nov run and plan for 2022Dec run

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    • Type: Task
    • Status: Done (View Workflow)
    • Priority: Normal
    • Resolution: Done
    • Component/s: None
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      Description

      • What we noticed during the 2022Nov run and will be fixed for the next run
        • general
        • script
          • Also, maybe we should fit the `EUPS` mechanism so that we can switch to different versions, but need to check if this is possible.
          • brokenFiber and brokenCobra should be separated in fiberStatus (see DAMD-143)
        • fiber allocation
          • Do we need to control the calibrators (sky and fluxstds) not to be closed to bright fibers? 
        • targetDB
          • targets
            • `target` table has columns for epoch and proper motion but pfsDesign datamodel not (see DAMD-137).
            • filterNames should follow the rule of fluxCalibration:
              • HSC: {g,r_old,r2,i_old,i2,z,y}_hsc
              • PS1: {g,r,i,z,y}_ps1
              • Gaia: {bp,rp,g}_gaia
              • SDSS: {u,g,r,i,z}_sdss
          • sky objects 
            • `cat_id` is not propagated to pfsDesign (see OBSPROC-34) --> done
            • We couldn't utilized the file of mapping between tract information and target coordinates
            • We should think about more on how to make sky targets in a field with diffuse feature and very high target density (such as M31).
        • gaiaDB

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          relates to

          Task - A task that needs to be done. PIPE2D-1110 Make match filterName between pfsConfig and flux calibration

          • Normal - Normal priorities
          • Done

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              • Assignee:
                Unassigned
                Reporter:
                kiyoto.yabe Kiyoto Yabe
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                • Created:
                  Updated:
                  Resolved: