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/PIPE2D-366 DRP 2-D Pipeline <p>Identify which absorption features are sensitive to stellar atmosphere parameters for F-stars.</p> <p>A short report of the features to be used and how they were determined should be provided.</p> <p>The absorption features should be written to a persistent file that can be subsequently loaded into the 2D DRP pipeline for flux calibration. The format needs to be decided. The location would be determined by <a href="https://pfspipe.ipmu.jp/jira/secure/ViewProfile.jspa?name=kiyoto.yabe" class="user-hover" rel="kiyoto.yabe">Kiyoto Yabe</a>.</p> PIPE2D-366

Identify absorption features

Task Normal Done Done Masayuki Tanaka hassan flux-calibration model-templates Tue, 19 Feb 2019 17:28:02 +0000 Fri, 23 Dec 2022 06:20:33 +0000 Fri, 23 Dec 2022 06:20:33 +0000 0 3 <p>The location of this file isn't important as it'll be loaded as a butler object. We do need to get it into the datamodel, and come up with a way of storing it "permanently" away from the live code/data, and potentially versioning it. Using git seems reasonable here, but we still have to sort out the details &#8211; and I agree that <a href="https://pfspipe.ipmu.jp/jira/secure/ViewProfile.jspa?name=kiyoto.yabe" class="user-hover" rel="kiyoto.yabe">Kiyoto Yabe</a> would be a good person.</p> <p>This ticket is obsolete and superseded by <a href="https://pfspipe.ipmu.jp/jira/browse/PIPE2D-647" title="Spectral stellar typing for flux calibration" class="issue-link" data-issue-key="PIPE2D-647"><del>PIPE2D-647</del></a>.</p> Blocks INFRA-242 Development Rank 0|02qptg:f Story Points 6.0