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        <build-number>803005</build-number>
        <build-date>13-09-2019</build-date>
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<item>
            <title>[PIPE2D-942] Do we see bright blue spots at double their original wavelength, i.e., in red</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-942</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;We are looking into the possible reasons for the larger than expected&lt;img class=&quot;emoticon&quot; src=&quot;https://pfspipe.ipmu.jp/jira/images/icons/emoticons/help_16.png&quot; height=&quot;16&quot; width=&quot;16&quot; align=&quot;absmiddle&quot; alt=&quot;&quot; border=&quot;0&quot;/&gt; drop in observed flux on the blue detector. As one possible diagnostic, look if there is any hint of bright blue arclines being observed at double their original wavelength in red.&#160;&lt;/p&gt;

&lt;p&gt;The code is at:&#160;&lt;/p&gt;
&lt;div class=&quot;code panel&quot; style=&quot;border-width: 1px;&quot;&gt;&lt;div class=&quot;codeContent panelContent&quot;&gt;
&lt;pre class=&quot;code-java&quot;&gt;
/home/ncaplar/Pipeline_notebooks/PIPE2D-942 (blue spots seen in red).ipynb&lt;/pre&gt;
&lt;/div&gt;&lt;/div&gt;</description>
                <environment></environment>
        <key id="18336">PIPE2D-942</key>
            <summary>Do we see bright blue spots at double their original wavelength, i.e., in red</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="ncaplar">ncaplar</assignee>
                                    <reporter username="ncaplar">ncaplar</reporter>
                        <labels>
                    </labels>
                <created>Wed, 10 Nov 2021 19:28:53 +0000</created>
                <updated>Wed, 8 Dec 2021 15:04:08 +0000</updated>
                            <resolved>Thu, 18 Nov 2021 21:41:02 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>2</watches>
                                                                <comments>
                            <comment id="25018" author="ncaplar" created="Thu, 11 Nov 2021 02:40:25 +0000"  >&lt;p&gt;have selected the brightest HgCd (60 seconds exposure) available from PFI. We have to use HgCd because other lamps do not have basically any lines below 490nm, which is the upper limit for this analysis. As such I can operate only with calexp images (&lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-935&quot; title=&quot;Support HgCd and other multi and single element sources&quot; class=&quot;issue-link&quot; data-issue-key=&quot;PIPE2D-935&quot;&gt;&lt;del&gt;PIPE2D-935&lt;/del&gt;&lt;/a&gt;). I have attached two figures&lt;/p&gt;

&lt;p&gt;1. blue_arm.png showing the spots at the blue end of blue arm. Both of these lines are quite strong (see the bar on the images).&lt;br/&gt;
 2. red_arm.png shows the cutouts of the calexp file at the wavelengths of the spots in the blue arm multiplied by 2. I do not see any appreciable contribution to the flux from the ghosts.&#160; &lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;a id=&quot;14468_thumb&quot; href=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/14468/14468_red_arm.png&quot; title=&quot;red_arm.png&quot; file-preview-type=&quot;image&quot; file-preview-id=&quot;14468&quot; file-preview-title=&quot;red_arm.png&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/thumbnail/14467/_thumb_14467.png&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/a&gt;&lt;/span&gt;&lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;a id=&quot;14468_thumb&quot; href=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/14468/14468_red_arm.png&quot; title=&quot;red_arm.png&quot; file-preview-type=&quot;image&quot; file-preview-id=&quot;14468&quot; file-preview-title=&quot;red_arm.png&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/thumbnail/14468/_thumb_14468.png&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/a&gt;&lt;/span&gt;&lt;/p&gt;</comment>
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                                            <outwardlinks description="relates to">
                                        <issuelink>
            <issuekey id="22531">INSTRM-1470</issuekey>
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                <attachments>
                            <attachment id="14467" name="blue_arm.png" size="50205" author="ncaplar" created="Thu, 11 Nov 2021 02:36:40 +0000"/>
                            <attachment id="14468" name="red_arm.png" size="133827" author="ncaplar" created="Thu, 11 Nov 2021 02:36:41 +0000"/>
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