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        <build-number>803005</build-number>
        <build-date>13-09-2019</build-date>
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<item>
            <title>[PIPE2D-370] Derive flux calibration vector for a given standard </title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-370</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;Write a function that for a given flux calibration standard, derives the flux calibration vector for that standard.&lt;/p&gt;</description>
                <environment></environment>
        <key id="13367">PIPE2D-370</key>
            <summary>Derive flux calibration vector for a given standard </summary>
                <type id="3" iconUrl="https://pfspipe.ipmu.jp/jira/secure/viewavatar?size=xsmall&amp;avatarId=10518&amp;avatarType=issuetype">Task</type>
                                            <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>
                    <statusCategory id="3" key="done" colorName="green"/>
                                    <resolution id="10000">Done</resolution>
                                        <assignee username="takuji.yamashita">Takuji Yamashita</assignee>
                                    <reporter username="hassan">hassan</reporter>
                        <labels>
                            <label>flux-cal-vector</label>
                            <label>flux-calibration</label>
                    </labels>
                <created>Tue, 19 Feb 2019 19:41:37 +0000</created>
                <updated>Tue, 6 Jul 2021 04:52:12 +0000</updated>
                            <resolved>Tue, 6 Jul 2021 04:52:12 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>4</watches>
                                                                <comments>
                            <comment id="21644" author="takuji.yamashita" created="Tue, 6 Jul 2021 04:32:51 +0000"  >&lt;p&gt;This is a flux ratio of the best-fit model to the simulated spectrum. The flux of the best-fit model was scaled using the broad-band photometry (&lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-838&quot; title=&quot;Absolute scaling of the best-fit model spectrum&quot; class=&quot;issue-link&quot; data-issue-key=&quot;PIPE2D-838&quot;&gt;&lt;del&gt;PIPE2D-838&lt;/del&gt;&lt;/a&gt;). It is distributed around 1. There is a systematic offset in the blue part at ~400 nm. This comes from stellar typing. In this case, the simulated spectrum was generated at Teff=7000K, logg=4.5, &lt;span class=&quot;error&quot;&gt;&amp;#91;Fe/H&amp;#93;&lt;/span&gt;=0, &lt;span class=&quot;error&quot;&gt;&amp;#91;a/Fe&amp;#93;&lt;/span&gt;=0, while the best-fit parameters are Teff=7069K, logg=3.69, &lt;span class=&quot;error&quot;&gt;&amp;#91;Fe/H&amp;#93;&lt;/span&gt;=-1.5, &lt;span class=&quot;error&quot;&gt;&amp;#91;a/Fe&amp;#93;&lt;/span&gt;=0.6.&#160;&lt;/p&gt;

&lt;p&gt;&lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;a id=&quot;13945_thumb&quot; href=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/13945/13945_vector.png&quot; title=&quot;vector.png&quot; file-preview-type=&quot;image&quot; file-preview-id=&quot;13945&quot; file-preview-title=&quot;vector.png&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/thumbnail/13944/_thumb_13944.png&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/a&gt;&lt;/span&gt;&lt;/p&gt;</comment>
                            <comment id="21645" author="takuji.yamashita" created="Tue, 6 Jul 2021 04:36:25 +0000"  >&lt;p&gt;This is a resultant flux calibration vector of the above case. The flux calibration vector is a ratio of the best-fit model spectrum to the input spectrum. Here, the atmospheric absorption and the quartz flat were applied to the input spectrum.&#160;&lt;/p&gt;

&lt;p&gt;&lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;a id=&quot;13945_thumb&quot; href=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/13945/13945_vector.png&quot; title=&quot;vector.png&quot; file-preview-type=&quot;image&quot; file-preview-id=&quot;13945&quot; file-preview-title=&quot;vector.png&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/thumbnail/13945/_thumb_13945.png&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/a&gt;&lt;/span&gt;&lt;/p&gt;</comment>
                    </comments>
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                                        <issuelink>
            <issuekey id="13369">PIPE2D-371</issuekey>
        </issuelink>
            <issuelink>
            <issuekey id="13371">PIPE2D-373</issuekey>
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            <issuekey id="15609">PIPE2D-838</issuekey>
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                <attachments>
                            <attachment id="13944" name="flux_ratio.png" size="83474" author="takuji.yamashita" created="Tue, 6 Jul 2021 04:27:08 +0000"/>
                            <attachment id="13945" name="vector.png" size="40999" author="takuji.yamashita" created="Tue, 6 Jul 2021 04:27:10 +0000"/>
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