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<item>
            <title>[PIPE2D-1075] Standard stars for September 2022 engineering run</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1075</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;Prepare a target list of standard stars for the September 2022 Eng Run. The target list is composed of faint DA white dwarf standards and CalSpec stars as well as the last runs.&#160;&lt;/p&gt;</description>
                <environment></environment>
        <key id="22933">PIPE2D-1075</key>
            <summary>Standard stars for September 2022 engineering run</summary>
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                                    <resolution id="10000">Done</resolution>
                                        <assignee username="takuji.yamashita">Takuji Yamashita</assignee>
                                    <reporter username="takuji.yamashita">Takuji Yamashita</reporter>
                        <labels>
                            <label>EngRun</label>
                            <label>flux-calibration</label>
                    </labels>
                <created>Thu, 8 Sep 2022 01:46:27 +0000</created>
                <updated>Fri, 4 Nov 2022 05:43:38 +0000</updated>
                            <resolved>Mon, 3 Oct 2022 13:42:08 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>4</watches>
                                                                <comments>
                            <comment id="31292" author="takuji.yamashita" created="Thu, 8 Sep 2022 01:52:28 +0000"  >&lt;p&gt;The new target list of standard stars for the September Eng Run contains&#160;6 DA white dwarfs selected from Narayan et al. (2019) which are 18-20 mag stars, and 2 F-stars from CalSpec which are 9 mag and 16 mag stars. These stars will&#160;be used for the raster scan test but the data can also be used for the flux calibration test.&#160;Their coordinate information was fetched from Gaia DR3 and the photometries were from PS1 DR2 or APASS DR10.&#160;I sent the list to Moritani-san. I have no order of priority from a point of view of flux calibration.&#160;&lt;/p&gt;

&lt;p&gt;I have made the same comment here:&lt;/p&gt;

&lt;p&gt;&lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1022?focusedCommentId=31291&amp;amp;page=com.atlassian.jira.plugin.system.issuetabpanels:comment-tabpanel#comment-31291&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1022?focusedCommentId=31291&amp;amp;page=com.atlassian.jira.plugin.system.issuetabpanels:comment-tabpanel#comment-31291&lt;/a&gt;&lt;/p&gt;</comment>
                            <comment id="31528" author="hassan" created="Mon, 3 Oct 2022 13:42:08 +0000"  >&lt;p&gt;&lt;tt&gt;pfsDesigns&lt;/tt&gt; for the Sep 2022 eng run have been created successfully.&lt;/p&gt;</comment>
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