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    <title>PFS-JIRA</title>
    <link>https://pfspipe.ipmu.jp/jira</link>
    <description>This file is an XML representation of an issue</description>
    <language>en-us</language>    <build-info>
        <version>8.3.4</version>
        <build-number>803005</build-number>
        <build-date>13-09-2019</build-date>
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<item>
            <title>[PIPE2D-1053] Make a full fluxmodeldata package</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/PIPE2D-1053</link>
                <project id="10002" key="PIPE2D">DRP 2-D Pipeline</project>
                    <description>&lt;p&gt;In &lt;a href=&quot;https://pfspipe.ipmu.jp/jira/browse/PIPE2D-920&quot; title=&quot;How to put the large set of the AMBRE model templates in github for flux calibration&quot; class=&quot;issue-link&quot; data-issue-key=&quot;PIPE2D-920&quot;&gt;&lt;del&gt;PIPE2D-920&lt;/del&gt;&lt;/a&gt;, we made what we call &quot;6k fluxmodeldata&quot;, which contained ~ 6,000 spectra from AMBRE synthetic spectra. We now have to make &quot;60k fluxmodeldata&quot;: ~60,000 spectra with their parameters on the finer grid that Yamashita-san&apos;s plan requires.&lt;/p&gt;

&lt;p&gt;1. We have to extend the format of &lt;tt&gt;broadband/photometries.fits&lt;/tt&gt; so that its user can distinguish the spectra in the 6k package from the other interpolated spectra.&lt;/p&gt;

&lt;p&gt;2. We have to make a 60k package. We may include in it a file that indicates the hyperparameters used in interpolating the spectra.&lt;/p&gt;

&lt;p&gt;3. We have to modify &lt;tt&gt;makeFluxModelInterpolator.py&lt;/tt&gt; so that it will be aware of the new format of &lt;tt&gt;broadband/photometries.fits&lt;/tt&gt;, and it will make &lt;tt&gt;interpolator.pickle&lt;/tt&gt; only from the 6k spectra. I think we should not include &lt;tt&gt;interpolator.pickle&lt;/tt&gt; in the package but each user should run &lt;tt&gt;makeFluxModelInterpolator.py&lt;/tt&gt; to make it, because the pickle depends on scipy&apos;s version.&lt;/p&gt;

&lt;p&gt;I will make the first version of 60k package with the hyperparameters already known to work reasonably. I think I can find better hyperparameters by estimating the goodness of hyperparameters with cross validation, but that will be another issue.&lt;/p&gt;</description>
                <environment></environment>
        <key id="22816">PIPE2D-1053</key>
            <summary>Make a full fluxmodeldata package</summary>
                <type id="3" iconUrl="https://pfspipe.ipmu.jp/jira/secure/viewavatar?size=xsmall&amp;avatarId=10518&amp;avatarType=issuetype">Task</type>
                                            <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>
                    <statusCategory id="3" key="done" colorName="green"/>
                                    <resolution id="10000">Done</resolution>
                                        <assignee username="sogo.mineo">sogo.mineo</assignee>
                                    <reporter username="sogo.mineo">sogo.mineo</reporter>
                        <labels>
                            <label>flux-calibration</label>
                            <label>model-templates</label>
                    </labels>
                <created>Thu, 9 Jun 2022 06:23:46 +0000</created>
                <updated>Fri, 24 Jun 2022 01:21:54 +0000</updated>
                            <resolved>Fri, 24 Jun 2022 01:21:54 +0000</resolved>
                                                                        <due></due>
                            <votes>0</votes>
                                    <watches>2</watches>
                                                                <comments>
                            <comment id="31071" author="sogo.mineo" created="Wed, 22 Jun 2022 06:04:50 +0000"  >&lt;p&gt;Full package is available here: &lt;a href=&quot;https://hscdata.mtk.nao.ac.jp/hsc_bin_dist/pfs/fluxmodeldata-ambre-20220518-full.tar.xz&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;https://hscdata.mtk.nao.ac.jp/hsc_bin_dist/pfs/fluxmodeldata-ambre-20220518-full.tar.xz&lt;/a&gt;&lt;/p&gt;

&lt;p&gt; &lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/15215/15215_out_fluxmodel_6750_g_any_z_-3.00_a_0.8.gif&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/span&gt;&lt;br/&gt;
Change of appearance of the interpolated flux with respect to log(g).&lt;/p&gt;

&lt;p&gt; &lt;span class=&quot;image-wrap&quot; style=&quot;&quot;&gt;&lt;img src=&quot;https://pfspipe.ipmu.jp/jira/secure/attachment/15216/15216_out_fluxmodel_any_g_3.50_z_-3.00_a_0.8.gif&quot; style=&quot;border: 0px solid black&quot; /&gt;&lt;/span&gt; &lt;br/&gt;
Change of appearance of the interpolated flux with respect to Teff.&lt;/p&gt;

&lt;p&gt;Judging merely from these two animations, I guess the interpolation was successful.&lt;/p&gt;

&lt;p&gt;If you simply replace the small package with this one, drp_stella will probably suffer from short of memory. I have yet to revise drp_stella before closing this issue.&lt;/p&gt;</comment>
                            <comment id="31072" author="sogo.mineo" created="Thu, 23 Jun 2022 07:39:05 +0000"  >&lt;p&gt;Could you review this PR (drp_stella)?&lt;/p&gt;</comment>
                            <comment id="31076" author="sogo.mineo" created="Fri, 24 Jun 2022 01:21:54 +0000"  >&lt;p&gt;Merged. Thanks for the review.&lt;/p&gt;</comment>
                    </comments>
                    <attachments>
                            <attachment id="15215" name="out_fluxmodel_6750_g_any_z_-3.00_a_0.8.gif" size="196825" author="sogo.mineo" created="Wed, 22 Jun 2022 05:59:55 +0000"/>
                            <attachment id="15216" name="out_fluxmodel_any_g_3.50_z_-3.00_a_0.8.gif" size="646999" author="sogo.mineo" created="Wed, 22 Jun 2022 06:02:06 +0000"/>
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