<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://pwiki.pic.es/index.php?action=history&amp;feed=atom&amp;title=High_redshift_galaxies</id>
	<title>High redshift galaxies - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://pwiki.pic.es/index.php?action=history&amp;feed=atom&amp;title=High_redshift_galaxies"/>
	<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High_redshift_galaxies&amp;action=history"/>
	<updated>2026-05-15T15:05:55Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.35.14</generator>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=High_redshift_galaxies&amp;diff=834&amp;oldid=prev</id>
		<title>Jcarrete: /* Version 1.0 */</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High_redshift_galaxies&amp;diff=834&amp;oldid=prev"/>
		<updated>2020-07-23T16:37:08Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Version 1.0&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 16:37, 23 July 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l66&quot; &gt;Line 66:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 66:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;     SELECT * FROM jcarrete.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;     SELECT * FROM jcarrete.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;     WHERE id IS NOT NULL;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;     WHERE id IS NOT NULL;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;== Version 1.1 ==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;I decide to add a new column in order to have the sedname as a integer values rather than as a string value:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;I decide to add a new column in order to have the sedname as a integer values rather than as a string value:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=High_redshift_galaxies&amp;diff=833&amp;oldid=prev</id>
		<title>Jcarrete: Created page with &quot;== Version 1.0 ==  Catalog provided by Rebecca and Pascal: https://euclid.roe.ac.uk/projects/puswg/wiki/Galaxies  It is a &quot;.txt&quot; file.  I remove the header and copy it into hd...&quot;</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High_redshift_galaxies&amp;diff=833&amp;oldid=prev"/>
		<updated>2020-07-23T16:36:42Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;== Version 1.0 ==  Catalog provided by Rebecca and Pascal: https://euclid.roe.ac.uk/projects/puswg/wiki/Galaxies  It is a &amp;quot;.txt&amp;quot; file.  I remove the header and copy it into hd...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Version 1.0 ==&lt;br /&gt;
&lt;br /&gt;
Catalog provided by Rebecca and Pascal: https://euclid.roe.ac.uk/projects/puswg/wiki/Galaxies&lt;br /&gt;
&lt;br /&gt;
It is a &amp;quot;.txt&amp;quot; file.&lt;br /&gt;
&lt;br /&gt;
I remove the header and copy it into hdfs:&lt;br /&gt;
&lt;br /&gt;
    tail -n+2 /cephfs/pic.es/astro/scratch/jcarrete/sandbox/Euclid/High_redshift_galaxies/Euclid_SC8_simcat_LBGs_DPL_16sqdegs_v1.txt | hdfs dfs -copyFromLocal - /user/jcarrete/data/euclid/high_z_galaxies/v1.0/Euclid_SC8_simcat_LBGs_DPL_16sqdegs_v1.csv&lt;br /&gt;
&lt;br /&gt;
I create the external table:&lt;br /&gt;
&lt;br /&gt;
    CREATE EXTERNAL TABLE jcarrete.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0(&lt;br /&gt;
    id bigint COMMENT 'unique galaxy identifier',&lt;br /&gt;
    `type` string COMMENT 'type (LBG for all objects)',&lt;br /&gt;
    z float COMMENT 'Redshift (in the range [6-12])',&lt;br /&gt;
    abs_muv float COMMENT 'absolute magnitude at 1500 angstroms',&lt;br /&gt;
    sedname string COMMENT 'Spectral Energy Distribution name (among 76, 38 without UV lines, 38 with UV lines, corresponding to a given UV slope)',&lt;br /&gt;
    rhalf_kpc float COMMENT 'half light radius (in physical kpc)',&lt;br /&gt;
    rhalf_arcsec float COMMENT 'half light radius (in arcsec)',&lt;br /&gt;
    muv float COMMENT 'for information only, observed magnitude at rest-frame 1500',&lt;br /&gt;
    beta float COMMENT 'for information only, used to assign an SED'&lt;br /&gt;
    )&lt;br /&gt;
    ROW FORMAT SERDE &lt;br /&gt;
      'org.apache.hadoop.hive.serde2.lazy.LazySimpleSerDe' &lt;br /&gt;
    WITH SERDEPROPERTIES ( &lt;br /&gt;
      'field.delim'=' ', &lt;br /&gt;
      'serialization.format'=' ') &lt;br /&gt;
    STORED AS INPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.mapred.TextInputFormat' &lt;br /&gt;
    OUTPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.HiveIgnoreKeyTextOutputFormat'&lt;br /&gt;
    LOCATION&lt;br /&gt;
      'hdfs://AntNest/user/jcarrete/data/euclid/high_z_galaxies/v1.0' &lt;br /&gt;
    ;&lt;br /&gt;
&lt;br /&gt;
I create the ORC table:&lt;br /&gt;
&lt;br /&gt;
    CREATE TABLE euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0_c(&lt;br /&gt;
    id bigint COMMENT 'unique galaxy identifier',&lt;br /&gt;
    `type` string COMMENT 'type (LBG for all objects)',&lt;br /&gt;
    z float COMMENT 'Redshift (in the range [6-12])',&lt;br /&gt;
    abs_muv float COMMENT 'absolute magnitude at 1500 angstroms',&lt;br /&gt;
    sedname string COMMENT 'Spectral Energy Distribution name (among 76, 38 without UV lines, 38 with UV lines, corresponding to a given UV slope)',&lt;br /&gt;
    rhalf_kpc float COMMENT 'half light radius (in physical kpc)',&lt;br /&gt;
    rhalf_arcsec float COMMENT 'half light radius (in arcsec)',&lt;br /&gt;
    muv float COMMENT 'for information only, observed magnitude at rest-frame 1500',&lt;br /&gt;
    beta float COMMENT 'for information only, used to assign an SED'&lt;br /&gt;
    )&lt;br /&gt;
    CLUSTERED BY ( &lt;br /&gt;
      id) &lt;br /&gt;
    SORTED BY ( &lt;br /&gt;
      id ASC) &lt;br /&gt;
    INTO 4 BUCKETS&lt;br /&gt;
    ROW FORMAT SERDE &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcSerde' &lt;br /&gt;
    STORED AS INPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcInputFormat' &lt;br /&gt;
    OUTPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcOutputFormat'&lt;br /&gt;
    ;&lt;br /&gt;
&lt;br /&gt;
Then I covert the data:&lt;br /&gt;
&lt;br /&gt;
    INSERT OVERWRITE TABLE cosmohub. euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0_c&lt;br /&gt;
    SELECT * FROM jcarrete.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0&lt;br /&gt;
    WHERE id IS NOT NULL;&lt;br /&gt;
&lt;br /&gt;
I decide to add a new column in order to have the sedname as a integer values rather than as a string value:&lt;br /&gt;
&lt;br /&gt;
    CREATE TABLE euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_1_c(&lt;br /&gt;
    id bigint COMMENT 'unique galaxy identifier',&lt;br /&gt;
    `type` string COMMENT 'type (LBG for all objects)',&lt;br /&gt;
    z float COMMENT 'Redshift (in the range [6-12])',&lt;br /&gt;
    abs_muv float COMMENT 'absolute magnitude at 1500 angstroms',&lt;br /&gt;
    sedname string COMMENT 'Spectral Energy Distribution name (among 76, 38 without UV lines, 38 with UV lines, corresponding to a given UV slope)',&lt;br /&gt;
    sedname_int int COMMENT 'sedname as integer (from 0 to 75, from 0 to 37 without UV lines, from 38 to 75 with UV lines)',&lt;br /&gt;
    rhalf_kpc float COMMENT 'half light radius (in physical kpc)',&lt;br /&gt;
    rhalf_arcsec float COMMENT 'half light radius (in arcsec)',&lt;br /&gt;
    muv float COMMENT 'for information only, observed magnitude at rest-frame 1500',&lt;br /&gt;
    beta float COMMENT 'for information only, used to assign an SED'&lt;br /&gt;
    )&lt;br /&gt;
    CLUSTERED BY ( &lt;br /&gt;
      id) &lt;br /&gt;
    SORTED BY ( &lt;br /&gt;
      id ASC) &lt;br /&gt;
    INTO 4 BUCKETS&lt;br /&gt;
    ROW FORMAT SERDE &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcSerde' &lt;br /&gt;
    STORED AS INPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcInputFormat' &lt;br /&gt;
    OUTPUTFORMAT &lt;br /&gt;
      'org.apache.hadoop.hive.ql.io.orc.OrcOutputFormat'&lt;br /&gt;
    ;&lt;br /&gt;
&lt;br /&gt;
This is the command to convert sedname into sedname_int:&lt;br /&gt;
&lt;br /&gt;
    INSERT OVERWRITE TABLE cosmohub.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_1_c&lt;br /&gt;
    SELECT id, `type`,z, abs_muv, sedname, &lt;br /&gt;
    CASE WHEN sedname = 'beta_1.25.dat' THEN 0&lt;br /&gt;
    WHEN sedname = 'beta_1.30.dat' THEN 1&lt;br /&gt;
    WHEN sedname = 'beta_1.35.dat' THEN 2&lt;br /&gt;
    WHEN sedname = 'beta_1.40.dat' THEN 3&lt;br /&gt;
    WHEN sedname = 'beta_1.45.dat' THEN 4&lt;br /&gt;
    WHEN sedname = 'beta_1.50.dat' THEN 5&lt;br /&gt;
    WHEN sedname = 'beta_1.55.dat' THEN 6&lt;br /&gt;
    WHEN sedname = 'beta_1.60.dat' THEN 7&lt;br /&gt;
    WHEN sedname = 'beta_1.65.dat' THEN 8&lt;br /&gt;
    WHEN sedname = 'beta_1.70.dat' THEN 9&lt;br /&gt;
    WHEN sedname = 'beta_1.75.dat' THEN 10&lt;br /&gt;
    WHEN sedname = 'beta_1.80.dat' THEN 11&lt;br /&gt;
    WHEN sedname = 'beta_1.85.dat' THEN 12&lt;br /&gt;
    WHEN sedname = 'beta_1.90.dat' THEN 13&lt;br /&gt;
    WHEN sedname = 'beta_1.95.dat' THEN 14&lt;br /&gt;
    WHEN sedname = 'beta_2.00.dat' THEN 15&lt;br /&gt;
    WHEN sedname = 'beta_2.05.dat' THEN 16&lt;br /&gt;
    WHEN sedname = 'beta_2.10.dat' THEN 17&lt;br /&gt;
    WHEN sedname = 'beta_2.15.dat' THEN 18&lt;br /&gt;
    WHEN sedname = 'beta_2.20.dat' THEN 19&lt;br /&gt;
    WHEN sedname = 'beta_2.25.dat' THEN 20&lt;br /&gt;
    WHEN sedname = 'beta_2.30.dat' THEN 21&lt;br /&gt;
    WHEN sedname = 'beta_2.35.dat' THEN 22&lt;br /&gt;
    WHEN sedname = 'beta_2.40.dat' THEN 23&lt;br /&gt;
    WHEN sedname = 'beta_2.45.dat' THEN 24&lt;br /&gt;
    WHEN sedname = 'beta_2.50.dat' THEN 25&lt;br /&gt;
    WHEN sedname = 'beta_2.55.dat' THEN 26&lt;br /&gt;
    WHEN sedname = 'beta_2.60.dat' THEN 27&lt;br /&gt;
    WHEN sedname = 'beta_2.65.dat' THEN 28&lt;br /&gt;
    WHEN sedname = 'beta_2.70.dat' THEN 29&lt;br /&gt;
    WHEN sedname = 'beta_2.75.dat' THEN 30&lt;br /&gt;
    WHEN sedname = 'beta_2.80.dat' THEN 31&lt;br /&gt;
    WHEN sedname = 'beta_2.85.dat' THEN 32&lt;br /&gt;
    WHEN sedname = 'beta_2.90.dat' THEN 33&lt;br /&gt;
    WHEN sedname = 'beta_2.95.dat' THEN 34&lt;br /&gt;
    WHEN sedname = 'beta_3.00.dat' THEN 35&lt;br /&gt;
    WHEN sedname = 'beta_3.05.dat' THEN 36&lt;br /&gt;
    WHEN sedname = 'beta_3.10.dat' THEN 37&lt;br /&gt;
    WHEN sedname = 'beta_1.25_wUVLines.dat' THEN 38&lt;br /&gt;
    WHEN sedname = 'beta_1.30_wUVLines.dat' THEN 39&lt;br /&gt;
    WHEN sedname = 'beta_1.35_wUVLines.dat' THEN 40&lt;br /&gt;
    WHEN sedname = 'beta_1.40_wUVLines.dat' THEN 41&lt;br /&gt;
    WHEN sedname = 'beta_1.45_wUVLines.dat' THEN 42&lt;br /&gt;
    WHEN sedname = 'beta_1.50_wUVLines.dat' THEN 43&lt;br /&gt;
    WHEN sedname = 'beta_1.55_wUVLines.dat' THEN 44&lt;br /&gt;
    WHEN sedname = 'beta_1.60_wUVLines.dat' THEN 45&lt;br /&gt;
    WHEN sedname = 'beta_1.65_wUVLines.dat' THEN 46&lt;br /&gt;
    WHEN sedname = 'beta_1.70_wUVLines.dat' THEN 47&lt;br /&gt;
    WHEN sedname = 'beta_1.75_wUVLines.dat' THEN 48&lt;br /&gt;
    WHEN sedname = 'beta_1.80_wUVLines.dat' THEN 49&lt;br /&gt;
    WHEN sedname = 'beta_1.85_wUVLines.dat' THEN 50&lt;br /&gt;
    WHEN sedname = 'beta_1.90_wUVLines.dat' THEN 51&lt;br /&gt;
    WHEN sedname = 'beta_1.95_wUVLines.dat' THEN 52&lt;br /&gt;
    WHEN sedname = 'beta_2.00_wUVLines.dat' THEN 53&lt;br /&gt;
    WHEN sedname = 'beta_2.05_wUVLines.dat' THEN 54&lt;br /&gt;
    WHEN sedname = 'beta_2.10_wUVLines.dat' THEN 55&lt;br /&gt;
    WHEN sedname = 'beta_2.15_wUVLines.dat' THEN 56&lt;br /&gt;
    WHEN sedname = 'beta_2.20_wUVLines.dat' THEN 57&lt;br /&gt;
    WHEN sedname = 'beta_2.25_wUVLines.dat' THEN 58&lt;br /&gt;
    WHEN sedname = 'beta_2.30_wUVLines.dat' THEN 59&lt;br /&gt;
    WHEN sedname = 'beta_2.35_wUVLines.dat' THEN 60&lt;br /&gt;
    WHEN sedname = 'beta_2.40_wUVLines.dat' THEN 61&lt;br /&gt;
    WHEN sedname = 'beta_2.45_wUVLines.dat' THEN 62&lt;br /&gt;
    WHEN sedname = 'beta_2.50_wUVLines.dat' THEN 63&lt;br /&gt;
    WHEN sedname = 'beta_2.55_wUVLines.dat' THEN 64&lt;br /&gt;
    WHEN sedname = 'beta_2.60_wUVLines.dat' THEN 65&lt;br /&gt;
    WHEN sedname = 'beta_2.65_wUVLines.dat' THEN 66&lt;br /&gt;
    WHEN sedname = 'beta_2.70_wUVLines.dat' THEN 67&lt;br /&gt;
    WHEN sedname = 'beta_2.75_wUVLines.dat' THEN 68&lt;br /&gt;
    WHEN sedname = 'beta_2.80_wUVLines.dat' THEN 69&lt;br /&gt;
    WHEN sedname = 'beta_2.85_wUVLines.dat' THEN 70&lt;br /&gt;
    WHEN sedname = 'beta_2.90_wUVLines.dat' THEN 71&lt;br /&gt;
    WHEN sedname = 'beta_2.95_wUVLines.dat' THEN 72&lt;br /&gt;
    WHEN sedname = 'beta_3.00_wUVLines.dat' THEN 73&lt;br /&gt;
    WHEN sedname = 'beta_3.05_wUVLines.dat' THEN 74&lt;br /&gt;
    WHEN sedname = 'beta_3.10_wUVLines.dat' THEN 75&lt;br /&gt;
    END as sedname_int,&lt;br /&gt;
    rhalf_kpc, rhalf_arcsec, muv, beta&lt;br /&gt;
    FROM jcarrete.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_0&lt;br /&gt;
    WHERE id IS NOT NULL;&lt;br /&gt;
&lt;br /&gt;
    ANALYZE TABLE cosmohub.euclid_sc8_simcat_lbgs_dpl_16_sqdegs_v1_1_c COMPUTE STATISTICS FOR COLUMNS;&lt;br /&gt;
&lt;br /&gt;
Then I create the catalog in CosmoHub.&lt;/div&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
</feed>