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        <build-number>803005</build-number>
        <build-date>13-09-2019</build-date>
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<item>
            <title>[PIPE2D-1277] Master FLUXSTD catalog</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1277</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;There are a few different versions of the FLUXSTD catalogs that we have used in our engineering runs. There is room for improvements in the latest version and this epic is a master ticket for the next (and hopefully final) version of the FLUXSTD catalog. The catalogs so far are summarized in&lt;br/&gt;
 &lt;a href=&quot;https://github.com/Subaru-PFS/drp_fstar_photo/blob/main/doc/catalog.md&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;https://github.com/Subaru-PFS/drp_fstar_photo/blob/main/doc/catalog.md&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;Based on a discussion with Ishigaki-san, the current version is based on the Gaia DR3 and PS1 DR2 matched catalog. The catalog is stored in a local DB in Mitaka. The SQL script at the link above gives the selection function, but in short: gMeanPSFMag&amp;lt;21 and gMeanPSFMag&amp;gt;13.5 are the primary constraints. The comparisons with SEGUE included the y-band photometry, but Ishigaki-san told me that faint objects are missing the y-band photometry (need to check why) and most stars are classified without the y-band. We need to understand this because the y-band is useful (z/y-bands straddle the Paschen break).&lt;/p&gt;

&lt;p&gt;Also, no flag cuts have been applied. We should apply, at minimum, qualityFlag &amp;amp; objInfoFlag == GOOD. There may be other flags to apply and we need to look into it. We should also remove bad stars; we may remove red stars (after the Galactic extinction correction is applied). The original catalog has about 2 million objects and the compute time is about 3 seconds per object.&lt;/p&gt;

&lt;p&gt;Another thing we need to understand is how brutus behaves when we exceed a specified memory limit. Ishigaki-san says it uses fewer models without any log output.&lt;/p&gt;</description>
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        <key id="23774">PIPE2D-1277</key>
            <summary>Master FLUXSTD catalog</summary>
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                                    <resolution id="-1">Unresolved</resolution>
                                        <assignee username="msyktnk">Masayuki Tanaka</assignee>
                                    <reporter username="msyktnk">Masayuki Tanaka</reporter>
                        <labels>
                            <label>FLUXSTD</label>
                    </labels>
                <created>Fri, 4 Aug 2023 01:26:25 +0000</created>
                <updated>Wed, 20 Dec 2023 06:41:19 +0000</updated>
                                                                                <due></due>
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                                    <watches>5</watches>
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