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<item>
            <title>[REDMINE1D-39] [RM-6154] Apply Milkyway ISM dust extinction</title>
                <link>https://pfspipe.ipmu.jp/jira/browse/REDMINE1D-39</link>
                <project id="11002" key="REDMINE1D">1D Redmine </project>
                    <description>&lt;p&gt;&lt;em&gt;&lt;font color=&quot;#505f79&quot;&gt; Created on 2020-11-27 18:06:21 by Didier Vibert. % Done: 20&lt;/font&gt;&lt;/em&gt;&lt;/p&gt;


&lt;p&gt;applying the ism for stars proved to be usefull&lt;/p&gt;

&lt;p&gt;should we apply a local dust extinction for galaxies to ? then it has to be applied in obsframe&lt;/p&gt;</description>
                <environment></environment>
        <key id="16743">REDMINE1D-39</key>
            <summary>[RM-6154] Apply Milkyway ISM dust extinction</summary>
                <type id="3" iconUrl="https://pfspipe.ipmu.jp/jira/secure/viewavatar?size=xsmall&amp;avatarId=10518&amp;avatarType=issuetype">Task</type>
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                                    <resolution id="-1">Unresolved</resolution>
                                        <assignee username="r2j.migrate">Redmine-Jira Migtation</assignee>
                                    <reporter username="r2j.migrate">Redmine-Jira Migtation</reporter>
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                <created>Fri, 4 Jun 2021 01:20:23 +0000</created>
                <updated>Tue, 13 Jun 2023 06:11:49 +0000</updated>
                                                                                <due></due>
                            <votes>0</votes>
                                    <watches>2</watches>
                                                                <comments>
                            <comment id="32972" author="yuki.moritani" created="Tue, 13 Jun 2023 06:11:42 +0000"  >&lt;p&gt;Comment by Didier Vibert on 2021-06-28 09:26:16:&lt;br/&gt;
r&#233;cup&#233;rer la carte, question coordonn&#233;es source dispo ? &lt;/p&gt;
</comment>
                            <comment id="32973" author="yuki.moritani" created="Tue, 13 Jun 2023 06:11:46 +0000"  >&lt;p&gt;Comment by Vincent Le Brun on 2021-06-29 09:28:23:&lt;br/&gt;
The extinction map from  Planck is here :&lt;br/&gt;
&lt;a href=&quot;http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=HFI_CompMap_ThermalDustModel_2048_R1.20.fits&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;http://pla.esac.esa.int/pla/aio/product-action?MAP.MAP_ID=HFI_CompMap_ThermalDustModel_2048_R1.20.fits&lt;/a&gt;&lt;br/&gt;
E(B-V) is in column  3&lt;br/&gt;
Coordonn&#233;es are available from  HEALPIX reference system&lt;br/&gt;
&lt;a href=&quot;https://sourceforge.net/projects/healpix/&quot; class=&quot;external-link&quot; rel=&quot;nofollow&quot;&gt;https://sourceforge.net/projects/healpix/&lt;/a&gt;&lt;br/&gt;
There are routines that make the link between coordinates and pixel/row number. &lt;br/&gt;
This should be implemented in AMAZED and (at least) the Euclid pipeline. The correction on the continuum is the same as in the ISM fit but at redshift 0.&lt;br/&gt;
The correction should be optional, as simulated data might not be affected by MW extinction&lt;/p&gt;</comment>
                            <comment id="32974" author="yuki.moritani" created="Tue, 13 Jun 2023 06:11:47 +0000"  >&lt;p&gt;Comment by Vincent Le Brun on 2021-12-15 21:23:43:&lt;br/&gt;
&#224; discuter en planif.&lt;/p&gt;</comment>
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