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<item>
            <title>[DAMD-83] Consider use of PSF fluxes as well as fiber fluxes for spectrophotometry</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/DAMD-83</link>
                <project id="10400" key="DAMD">Data Model</project>
                    <description>&lt;p&gt;&lt;a href=&quot;https://pfspipe.ipmu.jp/jira/secure/ViewProfile.jspa?name=msyktnk&quot; class=&quot;user-hover&quot; rel=&quot;msyktnk&quot;&gt;Masayuki Tanaka&lt;/a&gt; points out that for stars we should be tying the spectrophotometry to the psf fluxes rather than the fibre flux.   The fibre fluxes are seeing-corrected, but not corrected to a large (ideally infinite) radius, so while they &lt;b&gt;might&lt;/b&gt; provide acceptable colours they will not provide acceptable total photometry.   Please add &lt;tt&gt;psfFlux&lt;/tt&gt; measurements to the &lt;tt&gt;pfsDesign&lt;/tt&gt; file.&lt;/p&gt;</description>
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        <key id="14633">DAMD-83</key>
            <summary>Consider use of PSF fluxes as well as fiber fluxes for spectrophotometry</summary>
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                                            <priority id="10000" iconUrl="https://pfspipe.ipmu.jp/jira/images/icons/priorities/medium.svg">Normal</priority>
                        <status id="10002" iconUrl="https://pfspipe.ipmu.jp/jira/images/icons/statuses/generic.png" description="The issue is resolved, reviewed, and merged">Done</status>
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                                    <resolution id="10000">Done</resolution>
                                        <assignee username="hassan">hassan</assignee>
                                    <reporter username="rhl">rhl</reporter>
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                <created>Fri, 17 Jul 2020 18:12:24 +0000</created>
                <updated>Mon, 4 Jan 2021 20:23:05 +0000</updated>
                            <resolved>Wed, 18 Nov 2020 23:34:35 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>4</watches>
                                                                <comments>
                            <comment id="17448" author="msyktnk" created="Mon, 20 Jul 2020 00:57:24 +0000"  >&lt;p&gt;As you say, let&apos;s use fluxes (nJy) instead of magnitudes. &lt;del&gt;In addition, we need flux uncertainties.&lt;/del&gt; (the uncertainties are covered in &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/DAMD-84&quot; title=&quot;Add photometric errors to the pfsDesign and pfsObject files&quot; class=&quot;issue-link&quot; data-issue-key=&quot;DAMD-84&quot;&gt;&lt;del&gt;DAMD-84&lt;/del&gt;&lt;/a&gt;).&#160; These fluxes should not be corrected for the Galactic extinction. We will &apos;apply&apos; the Galactic extinction in the flux calibration (we infer the intrinsic spectral shape of a specphot std from the stellar typing using photometry and absorption lines, and then apply the Galactic extinction to it to make the &apos;expected&apos; spectrum that we observe).&#160; I wonder if it would be useful to have a fiducial E(B-V) in pfsDesign...?&#160; There is a few Galactic extinction maps in the market and I do not know which one is most popular these days.&lt;/p&gt;</comment>
                            <comment id="18021" author="hassan" created="Wed, 4 Nov 2020 02:47:09 +0000"  >&lt;p&gt;As agreed in the 2D DRP technical telecon 2020-10-26, addressing &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/DAMD-33&quot; title=&quot;Do we need total mag as well as fiber mag?&quot; class=&quot;issue-link&quot; data-issue-key=&quot;DAMD-33&quot;&gt;&lt;del&gt;DAMD-33&lt;/del&gt;&lt;/a&gt; (introduce totalFlux) and &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/DAMD-84&quot; title=&quot;Add photometric errors to the pfsDesign and pfsObject files&quot; class=&quot;issue-link&quot; data-issue-key=&quot;DAMD-84&quot;&gt;&lt;del&gt;DAMD-84&lt;/del&gt;&lt;/a&gt; (add photometric errors) in this same ticket.&lt;/p&gt;</comment>
                            <comment id="18057" author="hassan" created="Wed, 18 Nov 2020 23:34:35 +0000"  >&lt;p&gt;Merged to master.&lt;/p&gt;</comment>
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            <issuekey id="14634">DAMD-84</issuekey>
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            <issuekey id="12603">DAMD-33</issuekey>
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