https://pfspipe.ipmu.jp/jira This file is an XML representation of an issue en-us 8.3.4 803005 13-09-2019 https://pfspipe.ipmu.jp/jira/browse/INSTRM-1781 Instrument control development <p>Here is a test and check list for software updates before coming the engineering run (2022/11/14-20). Note that all the software should be tagged and implemented at the summit/Hilo system.</p> <ol> <li>AG name (<a href="https://pfspipe.ipmu.jp/jira/browse/DAMD-138" title="Add AGCC filename format" class="issue-link" data-issue-key="DAMD-138"><del>DAMD-138</del></a>, <a href="https://pfspipe.ipmu.jp/jira/browse/INSTRM-1764" title="Rename AGCC image files" class="issue-link" data-issue-key="INSTRM-1764"><del>INSTRM-1764</del></a>)</li> </ol> <ul> <li> <ul> <li>Take AG camera frame and check the name (Yan)</li> </ul> </li> </ul> <ol> <li>XML file <ul> <li>Check bits of masked cobras in modified xml file (Yan)</li> <li>Generate PfsDesign with new bit flags (Onodera)</li> </ul> </li> <li>RHL PFS scheme <ul> <li>Document <a href="https://pfspipe.ipmu.jp/jira/browse/INSTRM-1765" title="Document scheme for measuring cobra offset, brightness and PSF " class="issue-link" data-issue-key="INSTRM-1765"><del>INSTRM-1765</del></a> (Lupton)</li> </ul> </li> <li>opDB grouping <ul> <li>Test with 2+ frames with the same groupId (Le Fur)</li> </ul> </li> <li>opDB schema integrity <ul> <li>guidestars objId – test by loading PfsDesign/config (Onodera or Yabe)</li> <li>population by ASIAA – test by MCS frame (Karr) </li> </ul> </li> <li>SM1+SM3 operation <ul> <li>Can SM1 be operated independently of SM3 and concurrently (Le Fur, Loomis)</li> </ul> </li> <li>Optical Crosstalk <ul> <li>Regenerate coefficients (Le Fur, Price)</li> <li>Fix bug  on one side of detector <a href="https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1100" title="Optical cross-talk doesn&#39;t work on one side of detector" class="issue-link" data-issue-key="PIPE2D-1100"><del>PIPE2D-1100</del></a> (Lupton)</li> <li>Test? (Price)</li> </ul> </li> <li>OBJECT card contents <ul> <li>Look at the contents as data are taken (Loomis)</li> </ul> </li> <li>DRP CALIB (Note: SuNSS cannot be used for SM3) <ul> <li>SM3 DCB data – detectorMaps (b+r), fiberProfiles (Siddiqui)</li> </ul> </li> </ol> <p> </p> <p> After POpt2 installed (i.e. the beginning of the run), the following items can be tested:</p> <ol> <li>Cobra convergence</li> <li>Raster scan</li> <li>Full Boresight calculation (check population of the DB)</li> <li>Check population of agc_data flags column (Karr)</li> </ol> INSTRM-1781

Punch list to start the engineering run in November 2022

Task Normal Done Done Unassigned yuki.moritani EngRun Fri, 4 Nov 2022 17:17:10 +0000 Tue, 7 Feb 2023 22:35:34 +0000 Wed, 30 Nov 2022 13:05:23 +0000 0 2 <p>We need to add taking a full set of calibrations, reducing them, checking them, and ingesting them in the usual place</p> <p>Yes, but calibrations using pfilamp can be taken only after PFI is on the telescope. And we can take bias/dark before the run?</p> <p>I think my summary was confuging... this is the punch list mainly done "before" the run.</p> <p>Closing as November 2022 (Run 08) completed.</p> Development Rank 0|02qph7:03 Sprint 2DDRP-2023 A