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        <build-date>13-09-2019</build-date>
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<item>
            <title>[PIPE2D-384] Estimate density of F-stars as a fn of (RA, Dec)</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-384</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;To get a feel for how many spectrophotometric standards we have across the HSC footprint, we collect stars from the HSC database and apply magnitude + color cuts to select F-stars and estimate their spatial density.&#160; The density is of course dependent on the cuts we apply, but it would be useful to get a feel at this point and also to setup a machinery to estimate the stellar density for a given set of mag + color cuts.&lt;/p&gt;

&lt;p&gt;&#160;&lt;/p&gt;

&lt;p&gt;&#160;&lt;/p&gt;</description>
                <environment></environment>
        <key id="13405">PIPE2D-384</key>
            <summary>Estimate density of F-stars as a fn of (RA, Dec)</summary>
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                                            <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>
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                                    <resolution id="10000">Done</resolution>
                                        <assignee username="takuji.yamashita">Takuji Yamashita</assignee>
                                    <reporter username="msyktnk">Masayuki Tanaka</reporter>
                        <labels>
                            <label>flux-calibration</label>
                    </labels>
                <created>Thu, 7 Mar 2019 06:47:49 +0000</created>
                <updated>Wed, 18 Sep 2019 12:43:24 +0000</updated>
                            <resolved>Tue, 17 Sep 2019 02:43:53 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>2</watches>
                                                                <comments>
                            <comment id="15366" author="takuji.yamashita" created="Fri, 26 Apr 2019 12:29:45 +0000"  >&lt;p&gt;Using the &#8220;crude&#8221; selection defined at &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-383&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;PIPE2D-383&lt;/a&gt; and the HSC objects with g &amp;lt; 23 at &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-382&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;PIPE2D-382&lt;/a&gt;, F star candidates are selected and their density maps are created at each survey field. The figure is an example of the density maps. (A high density at R.A. ~ 31 deg is due to a star cluster. )&lt;/p&gt;

&lt;p&gt;&lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;a id=&quot;11929_thumb&quot; href=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/11929/11929_HSCFstar_DensityMap_pW02_20190426.png&quot; title=&quot;HSCFstar_DensityMap_pW02_20190426.png&quot; file-preview-type=&quot;image&quot; file-preview-id=&quot;11929&quot; file-preview-title=&quot;HSCFstar_DensityMap_pW02_20190426.png&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/thumbnail/11929/_thumb_11929.png&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/a&gt;&lt;/span&gt;&lt;/p&gt;</comment>
                            <comment id="16079" author="takuji.yamashita" created="Tue, 17 Sep 2019 02:43:53 +0000"  >&lt;p&gt;The methodology to estimate the spatial density of the selected F-stars was studied. We will re-make the density map using an updated selection criteria for F-stars.&lt;/p&gt;</comment>
                    </comments>
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                                                                <inwardlinks description="relates to">
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            <issuekey id="13355">PIPE2D-361</issuekey>
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                <attachments>
                            <attachment id="11929" name="HSCFstar_DensityMap_pW02_20190426.png" size="39512" author="takuji.yamashita" created="Fri, 26 Apr 2019 12:27:34 +0000"/>
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