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<item>
            <title>[PIPE2D-650] Apply the SDSS LSF to AMBRE templates</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-650</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;Apply the SDSS line spread function (LSF) to the AMBRE model templates in order to accurately compare between an SDSS spectrum and the best fit AMBRE model template.&lt;/p&gt;</description>
                <environment></environment>
        <key id="15009">PIPE2D-650</key>
            <summary>Apply the SDSS LSF to AMBRE templates</summary>
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                    <statusCategory id="3" key="done" colorName="green"/>
                                    <resolution id="10000">Done</resolution>
                                        <assignee username="msyktnk">Masayuki Tanaka</assignee>
                                    <reporter username="takuji.yamashita">Takuji Yamashita</reporter>
                        <labels>
                            <label>flux-calibration</label>
                            <label>model-templates</label>
                    </labels>
                <created>Wed, 4 Nov 2020 05:38:10 +0000</created>
                <updated>Fri, 14 Jul 2023 06:17:26 +0000</updated>
                            <resolved>Fri, 14 Jul 2023 06:17:25 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>3</watches>
                                                                <comments>
                            <comment id="34014" author="msyktnk" created="Fri, 14 Jul 2023 06:17:17 +0000"  >&lt;p&gt;I suspect this ticket was originally intended as a prior task to &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-651&quot; title=&quot;Spectral fitting of SDSS spectra for flux calibration&quot; class=&quot;issue-link&quot; data-issue-key=&quot;PIPE2D-651&quot;&gt;PIPE2D-651&lt;/a&gt;, but LSF convolution is an obvious step in the stellar typing (at least in the current algorithm) and I do not think it deserves a stand-alone ticket. Closing.&lt;/p&gt;</comment>
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