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-1821 Instrument control development <p>In order to fit the templates to the PSFs in the AG camera, the agccActor and centroiding routine need</p> <ul> <li>dZ: the offset in focus compared to the focus in autoguider. This can be calculated from the database if the value of m2_pos3 for a focussed autoguider is known.</li> <li>the reference positions of the stars in the focussed image</li> <li>the template themselves</li> </ul> <p>The first two items could be obtained from agc_exposure if the agc_exposure_id for the reference image is known.</p> <p>The third item could be stored in pfs_instdata (and, if necessary, updated in the same way as other calibration files).  </p> INSTRM-1821

Propogate template fitting information to agccActor

Task Normal Won't Fix Won't Fix chyan karr EngRun Fri, 9 Dec 2022 13:38:43 +0000 Tue, 3 Jan 2023 20:58:11 +0000 Tue, 3 Jan 2023 20:58:11 +0000 0 1 <p>Chi-Hung and I had a chat and have come up with a solution. </p> <ul> <li>add a keyword to the AGCC expose command which tells the code that this is a reference image. </li> <li>if the keyword is set, the positions determined from sep will be saved as part of the cParms dictionary, and will be the reference points until the expose command is called with the keyword again.</li> </ul> <p>It is planned to correct the AG focus for the upcoming Feb 2023 Run 10.</p> Blocks INSTRM-1817 Development Rank 0|zzsvhf: Sprint PreEngRun09Dec