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<item>
            <title>[SCIDB-93] prepare object lists from HSC PDR2 for a new survey simulation</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/SCIDB-93</link>
                <project id="10601" key="SCIDB">Science Database</project>
                    <description>&lt;p&gt;Prepare object lists from PDR2 following the selection criteria of each SSP survey components.&#160; Pass the lists to &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/secure/ViewProfile.jspa?name=kiyoto.yabe&quot; class=&quot;user-hover&quot; rel=&quot;kiyoto.yabe&quot;&gt;Kiyoto Yabe&lt;/a&gt; to run ETC (which is a separate ticket).&lt;/p&gt;</description>
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        <key id="14282">SCIDB-93</key>
            <summary>prepare object lists from HSC PDR2 for a new survey simulation</summary>
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                                    <resolution id="10000">Done</resolution>
                                        <assignee username="msyktnk">Masayuki Tanaka</assignee>
                                    <reporter username="msyktnk">Masayuki Tanaka</reporter>
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                <created>Thu, 26 Mar 2020 07:46:42 +0000</created>
                <updated>Tue, 30 Jun 2020 23:26:45 +0000</updated>
                            <resolved>Tue, 30 Jun 2020 23:26:45 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>1</watches>
                                                                <comments>
                            <comment id="17030" author="msyktnk" created="Tue, 14 Apr 2020 04:39:23 +0000"  >&lt;p&gt;I picked the UD_COSMOS field for the galaxy evolution survey.&#160; For the cosmology and archaeology surveys, I picked VVDS because it is relatively large and reasonably square-shaped as of PDR2.&#160; The target selection criteria are the same as v2.&#160; I spent some time thinking about input spectra to simulate, but I chose to take an easy path, which is to use only one star forming and one quiescent galaxy spectra as we did in v2, just for now.&#160; The number of objects increased quite a bit and the compute time for ETC is now a concern.&#160; For our purpose, we do not necessarily have to simulate all objects, and we will reduce objects to keep the compute time within a reasonable amount of time.&#160;&#160; The first version of the catalogs have been sent to Yabe-kun.&lt;/p&gt;</comment>
                            <comment id="17417" author="msyktnk" created="Tue, 30 Jun 2020 23:26:36 +0000"  >&lt;p&gt;A minor fix was made and a revised catalog was sent to Yabe-kun for production.&lt;/p&gt;</comment>
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