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-852 DRP 2-D Pipeline <p>Write a code to derive a probability distribution function from broad-band SED fitting of a standard star, and implement it to the flux calibration part in 2DDRP Pipeline. A draft of the code was provided from Takuji Yamashita.</p> PIPE2D-852

Code implementation of broad-band SED fitting for flux calibration

Task Normal Done Done sogo.mineo sogo.mineo flux-calibration Thu, 17 Jun 2021 04:47:10 +0000 Thu, 15 Jul 2021 05:54:19 +0000 Wed, 7 Jul 2021 01:42:33 +0000 0 5 <p>I opened two pull requests for this issue:</p> <p><a href="https://github.com/Subaru-PFS/drp_stella/pull/204" class="external-link" rel="nofollow">https://github.com/Subaru-PFS/drp_stella/pull/204</a><br/> <a href="https://github.com/Subaru-PFS/drp_pfs_data/pull/13" class="external-link" rel="nofollow">https://github.com/Subaru-PFS/drp_pfs_data/pull/13</a></p> <p>Could you review them?</p> <p>FitBroadbandSEDTask introduced by these changes will be a subtask of Yamashita-san's flux calibration. This task is given several fiber fluxes and returns probabilities for various SEDs. Yamashita-san's flux calibration will take these probabilities into account in order to determine the best SED for observed spectra.</p> <p>Thanks for review. Merged to master.</p> Blocks PIPE2D-371 Development Epic Link PIPE2D-303 Rank 0|zzs8a8: Reviewers price