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-991 DRP 2-D Pipeline <p>A synthetic broadband photometry table of AMBRE model templates is used for broadband SED fitting in flux calibration. This table is generated from the model template set on the user side. I provide a code to make the table in the drp_fstar repository. </p> PIPE2D-991

Code to make a synthetic broadband photometry table of AMBRE

Task Normal Done Done Takuji Yamashita Takuji Yamashita model-templates Mon, 28 Feb 2022 02:14:25 +0000 Fri, 3 Jun 2022 07:37:04 +0000 Fri, 3 Jun 2022 07:37:04 +0000 0 3 <p>Because the size of this table is small, we provide it together with an AMBRE model template set. The current model set and the broad-band flux table are provided in <a href="https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1044" class="external-link" rel="nofollow">PIPE2D-1044</a>. So, I will close this ticket.</p> <p>This work is included in <a href="https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1044" title="Flux models for flux calibration must have wavelengths in vacuum" class="issue-link" data-issue-key="PIPE2D-1044"><del>PIPE2D-1044</del></a>. </p> Development Epic Link PIPE2D-303 Rank 0|zzst73: Reviewers hassan