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	<title>Euclid mock production v1.8.1 - Revision history</title>
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	<updated>2026-04-20T15:09:43Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://pwiki.pic.es/index.php?title=Euclid_mock_production_v1.8.1&amp;diff=895&amp;oldid=prev</id>
		<title>Jcarrete at 11:03, 20 January 2021</title>
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		<updated>2021-01-20T11:03:37Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;a href=&quot;//pwiki.pic.es/index.php?title=Euclid_mock_production_v1.8.1&amp;amp;diff=895&amp;amp;oldid=455&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=Euclid_mock_production_v1.8.1&amp;diff=455&amp;oldid=prev</id>
		<title>Jcarrete: Created page with &quot;Goals:  * Test new pipeline with some improvements in the SciPIC algorithm. * The catalog is a 2 redshift bins, 0.4 &lt; z &lt; 0.6 and 0.9 &lt; z &lt; 1.1.  The catalog has been produced...&quot;</title>
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		<updated>2019-04-26T14:49:40Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;Goals:  * Test new pipeline with some improvements in the SciPIC algorithm. * The catalog is a 2 redshift bins, 0.4 &amp;lt; z &amp;lt; 0.6 and 0.9 &amp;lt; z &amp;lt; 1.1.  The catalog has been produced...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Goals: &lt;br /&gt;
* Test new pipeline with some improvements in the SciPIC algorithm.&lt;br /&gt;
* The catalog is a 2 redshift bins, 0.4 &amp;lt; z &amp;lt; 0.6 and 0.9 &amp;lt; z &amp;lt; 1.1.&lt;br /&gt;
&lt;br /&gt;
The catalog has been produced using notebook:&lt;br /&gt;
&lt;br /&gt;
&amp;gt; /hdfs/user/jcarrete/data/euclid/flagship_1_8_1/config/Euclid_mock_pipeline_production-v1.8.ipynb&lt;br /&gt;
&lt;br /&gt;
The commit used in SciPIC is 4b08560&lt;br /&gt;
&lt;br /&gt;
Some information about the changes:&lt;br /&gt;
&lt;br /&gt;
* Copy from 1.7.0 date(15/04/2019) but using the commit that includes the new NFW API (4b08560)&lt;br /&gt;
* I &amp;quot;copy-paste&amp;quot; the way fluxes are estimated in the SciPIC flux autovalidation.ipynb notebook from Pau.&lt;br /&gt;
* This version is the 1st try to integrate the NFW changes from Linda and the correct way of estimating the fluxes using the 1st octant of the new halo rockstar catalog.&lt;br /&gt;
* Changes:&lt;br /&gt;
** query to use the new rockstar dark matter halo catalog; the id for haloes changes: (bx, by, bz, id)&lt;br /&gt;
** API change to use the NFW from Linda&lt;br /&gt;
** file from Francisco mv to the scipic code: cp /software/astro/__to_delete__/src/castander/auxfiles/logflux_correction_hae_v1_3_1.csv /nfs/pic.es/user/j/jcarrete/src/mocks/scipic/mocks/fluxes/halpha_flux/logflux_correction_hae_v1_3_1.csv&lt;br /&gt;
** New binning emmission lines&lt;br /&gt;
** Changes in the way emission lines are called&lt;br /&gt;
** Changes in the auxilary files path: &amp;quot;/nfs/pic.es/user/j/jcarrete/scipic_files&amp;quot;&lt;br /&gt;
** I add a unique_gal_id using bx, by, bz and id&lt;/div&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
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