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	<id>https://pwiki.pic.es/index.php?action=history&amp;feed=atom&amp;title=High-z_QSOs</id>
	<title>High-z QSOs - 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-z_QSOs"/>
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	<updated>2026-04-20T15:08:13Z</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-z_QSOs&amp;diff=906&amp;oldid=prev</id>
		<title>Jcarrete at 22:37, 25 February 2021</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=906&amp;oldid=prev"/>
		<updated>2021-02-25T22:37:17Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;a href=&quot;//pwiki.pic.es/index.php?title=High-z_QSOs&amp;amp;diff=906&amp;amp;oldid=901&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=901&amp;oldid=prev</id>
		<title>Jcarrete at 09:54, 2 February 2021</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=901&amp;oldid=prev"/>
		<updated>2021-02-02T09:54:47Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;a href=&quot;//pwiki.pic.es/index.php?title=High-z_QSOs&amp;amp;diff=901&amp;amp;oldid=893&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=893&amp;oldid=prev</id>
		<title>Jcarrete at 15:59, 18 January 2021</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=893&amp;oldid=prev"/>
		<updated>2021-01-18T15:59:15Z</updated>

		<summary type="html">&lt;p&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;
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				&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 15:59, 18 January 2021&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-l647&quot; &gt;Line 647:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 647:&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;     {&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;     {&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;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;         &amp;quot;sql&amp;quot;: &amp;quot;SELECT CAST(unique_id AS bigint) AS SOURCE_ID,  \nCAST(-1 AS &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;float&lt;/del&gt;) AS HALO_ID, \nCAST(kind AS smallint) AS KIND,  \nCAST(ra AS double) AS RA,  \nCAST(`dec` AS double) AS `DEC`,  \nCAST(ra_mag AS double) AS RA_MAG,  \nCAST(dec_mag AS double) AS DEC_MAG,  \nCAST(z AS float) AS Z_OBS,  \nCAST(m1450 AS float) AS REF_MAG_ABS,  \nCAST(m1450 AS float) AS REF_MAG,  \nCAST(-1 AS float) AS BULGE_FRACTION,  \nCAST(-1 AS float) AS BULGE_R50,  \nCAST(-1 AS float) AS DISK_R50,  \nCAST(-1 AS float) AS BULGE_NSERSIC,  \nCAST(-1 AS float) AS BULGE_AXIS_RATIO,  \nCAST(-1 AS float) AS INCLINATION_ANGLE,  \nCAST(-1 AS float) AS DISK_ANGLE,  \nCAST(kappa AS float) AS KAPPA,  \nCAST(gamma1 AS float) AS GAMMA1,  \nCAST(gamma2 AS float) AS GAMMA2,  \nCAST(template_int AS float) AS SED_TEMPLATE,  \nCAST(0 AS smallint) AS EXT_LAW,  \nCAST(-1 AS float) AS EBV,  \nCAST(-1 AS float) AS HALPHA_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS HBETA_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS O2_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS O3_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS N2_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS S2_LOGFLAM_EXT_MAG,  \nCAST(mw_extinction AS float) AS AV,\nCAST(euclid_vis*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_VIS_MAG,  \nCAST(euclid_nisp_y*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Y_NISP_MAG,  \nCAST(euclid_nisp_j*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_J_NISP_MAG,  \nCAST(euclid_nisp_h*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_H_NISP_MAG,  \nCAST(blanco_decam_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_DECAM_MAG,  \nCAST(blanco_decam_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_DECAM_MAG,  \nCAST(blanco_decam_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_DECAM_MAG,  \nCAST(blanco_decam_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_DECAM_MAG,  \nCAST(cfht_megacam_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_MEGACAM_MAG,  \nCAST(cfht_megacam_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_MEGACAM_MAG,  \nCAST(jst_jpcam_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_JPCAM_MAG,  \nCAST(pan_starrs_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_PANSTARRS_MAG,  \nCAST(pan_starrs_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_PANSTARRS_MAG,  \nCAST(subaru_hsc_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_HSC_MAG,  \nCAST(gaia_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float)  AS TU_FNU_G_GAIA_MAG,  \nCAST(gaia_bp*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_BP_GAIA_MAG,  \nCAST(gaia_rp*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_RP_GAIA_MAG,  \nCAST(lsst_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_LSST_MAG,  \nCAST(lsst_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_LSST_MAG,  \nCAST(lsst_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_LSST_MAG,  \nCAST(lsst_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_LSST_MAG,  \nCAST(lsst_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_LSST_MAG,  \nCAST(lsst_y*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Y_LSST_MAG,  \nCAST(kids_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_KIDS_MAG,  \nCAST(kids_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_KIDS_MAG,  \nCAST(kids_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_KIDS_MAG,  \nCAST(kids_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_KIDS_MAG,  \nCAST(2mass_j*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_J_2MASS_MAG,  \nCAST(2mass_h*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_H_2MASS_MAG,  \nCAST(2mass_ks*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_KS_2MASS_MAG  \nFROM cosmohub.flagship_mock_1_10_4_qso_s  \nWHERE SHIFTRIGHT(hpix_29_nest, (29-5)*2) = 2063&amp;quot;&lt;/div&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;         &amp;quot;sql&amp;quot;: &amp;quot;SELECT CAST(unique_id AS bigint) AS SOURCE_ID,  \nCAST(-1 AS &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;bigint&lt;/ins&gt;) AS HALO_ID, \nCAST(kind AS smallint) AS KIND,  \nCAST(ra AS double) AS RA,  \nCAST(`dec` AS double) AS `DEC`,  \nCAST(ra_mag AS double) AS RA_MAG,  \nCAST(dec_mag AS double) AS DEC_MAG,  \nCAST(z AS float) AS Z_OBS,  \nCAST(m1450 AS float) AS REF_MAG_ABS,  \nCAST(m1450 AS float) AS REF_MAG,  \nCAST(-1 AS float) AS BULGE_FRACTION,  \nCAST(-1 AS float) AS BULGE_R50,  \nCAST(-1 AS float) AS DISK_R50,  \nCAST(-1 AS float) AS BULGE_NSERSIC,  \nCAST(-1 AS float) AS BULGE_AXIS_RATIO,  \nCAST(-1 AS float) AS INCLINATION_ANGLE,  \nCAST(-1 AS float) AS DISK_ANGLE,  \nCAST(kappa AS float) AS KAPPA,  \nCAST(gamma1 AS float) AS GAMMA1,  \nCAST(gamma2 AS float) AS GAMMA2,  \nCAST(template_int AS float) AS SED_TEMPLATE,  \nCAST(0 AS smallint) AS EXT_LAW,  \nCAST(-1 AS float) AS EBV,  \nCAST(-1 AS float) AS HALPHA_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS HBETA_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS O2_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS O3_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS N2_LOGFLAM_EXT_MAG,  \nCAST(-1 AS float) AS S2_LOGFLAM_EXT_MAG,  \nCAST(mw_extinction AS float) AS AV,\nCAST(euclid_vis*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_VIS_MAG,  \nCAST(euclid_nisp_y*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Y_NISP_MAG,  \nCAST(euclid_nisp_j*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_J_NISP_MAG,  \nCAST(euclid_nisp_h*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_H_NISP_MAG,  \nCAST(blanco_decam_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_DECAM_MAG,  \nCAST(blanco_decam_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_DECAM_MAG,  \nCAST(blanco_decam_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_DECAM_MAG,  \nCAST(blanco_decam_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_DECAM_MAG,  \nCAST(cfht_megacam_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_MEGACAM_MAG,  \nCAST(cfht_megacam_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_MEGACAM_MAG,  \nCAST(jst_jpcam_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_JPCAM_MAG,  \nCAST(pan_starrs_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_PANSTARRS_MAG,  \nCAST(pan_starrs_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_PANSTARRS_MAG,  \nCAST(subaru_hsc_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_HSC_MAG,  \nCAST(gaia_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float)  AS TU_FNU_G_GAIA_MAG,  \nCAST(gaia_bp*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_BP_GAIA_MAG,  \nCAST(gaia_rp*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_RP_GAIA_MAG,  \nCAST(lsst_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_LSST_MAG,  \nCAST(lsst_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_LSST_MAG,  \nCAST(lsst_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_LSST_MAG,  \nCAST(lsst_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_LSST_MAG,  \nCAST(lsst_z*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Z_LSST_MAG,  \nCAST(lsst_y*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_Y_LSST_MAG,  \nCAST(kids_u*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_U_KIDS_MAG,  \nCAST(kids_g*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_G_KIDS_MAG,  \nCAST(kids_r*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_R_KIDS_MAG,  \nCAST(kids_i*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_I_KIDS_MAG,  \nCAST(2mass_j*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_J_2MASS_MAG,  \nCAST(2mass_h*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_H_2MASS_MAG,  \nCAST(2mass_ks*1.e23*(1/((1 - kappa)*(1 - kappa) - gamma1*gamma1 - gamma2*gamma2))  AS float) AS TU_FNU_KS_2MASS_MAG  \nFROM cosmohub.flagship_mock_1_10_4_qso_s  \nWHERE SHIFTRIGHT(hpix_29_nest, (29-5)*2) = 2063&amp;quot;&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;         }&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;         }&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-z_QSOs&amp;diff=888&amp;oldid=prev</id>
		<title>Jcarrete at 16:26, 15 January 2021</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=888&amp;oldid=prev"/>
		<updated>2021-01-15T16:26:05Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;a href=&quot;//pwiki.pic.es/index.php?title=High-z_QSOs&amp;amp;diff=888&amp;amp;oldid=813&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
	<entry>
		<id>https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=813&amp;oldid=prev</id>
		<title>Jcarrete: Created page with &quot;Information in Euclid Redmine:  https://euclid.roe.ac.uk/projects/puswg/wiki/Quasars/      CREATE TABLE full_H25cut_Hcol_v1_0_c(     `id` bigint COMMENT 'ID',     `type` strin...&quot;</title>
		<link rel="alternate" type="text/html" href="https://pwiki.pic.es/index.php?title=High-z_QSOs&amp;diff=813&amp;oldid=prev"/>
		<updated>2020-06-30T22:06:39Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;Information in Euclid Redmine:  https://euclid.roe.ac.uk/projects/puswg/wiki/Quasars/      CREATE TABLE full_H25cut_Hcol_v1_0_c(     `id` bigint COMMENT &amp;#039;ID&amp;#039;,     `type` strin...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;Information in Euclid Redmine:&lt;br /&gt;
&lt;br /&gt;
https://euclid.roe.ac.uk/projects/puswg/wiki/Quasars/&lt;br /&gt;
&lt;br /&gt;
    CREATE TABLE full_H25cut_Hcol_v1_0_c(&lt;br /&gt;
    `id` bigint COMMENT 'ID',&lt;br /&gt;
    `type` string COMMENT 'type (QSO for all objects)',&lt;br /&gt;
    `z` float COMMENT 'redshift (z). Redshifts are in the range [6-15]',&lt;br /&gt;
    `m1450` float COMMENT 'absolute magnitude at 1450 angstroms (M1450)',&lt;br /&gt;
    `template` string COMMENT 'spectral template name (among 21)',&lt;br /&gt;
    `h` float COMMENT 'approximate H-band magnitude for information only. This was computed for applying the magnitude cut'&lt;br /&gt;
    )&lt;br /&gt;
    CLUSTERED BY (&lt;br /&gt;
    id&lt;br /&gt;
    )&lt;br /&gt;
    SORTED BY ( &lt;br /&gt;
    id ASC&lt;br /&gt;
    ) &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;
    INSERT OVERWRITE TABLE cosmohub.full_H25cut_Hcol_v1_0_c&lt;br /&gt;
    SELECT `id`, `type`, `z`,`m1450`, `template`, `h`&lt;br /&gt;
    FROM tallada.full_H25cut_Hcol;  &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
    ANALYZE TABLE cosmohub.full_H25cut_Hcol_v1_0_c COMPUTE STATISTICS FOR COLUMNS;&lt;br /&gt;
&lt;br /&gt;
--------------&lt;br /&gt;
&lt;br /&gt;
    CREATE TABLE full_H25cut_Hcol_v1_1_c(&lt;br /&gt;
    `id` bigint COMMENT 'ID',&lt;br /&gt;
    `type` string COMMENT 'type (QSO for all objects)',&lt;br /&gt;
    `z` float COMMENT 'redshift (z). Redshifts are in the range [6-15]',&lt;br /&gt;
    `m1450` float COMMENT 'absolute magnitude at 1450 angstroms (M1450)',&lt;br /&gt;
    `template` string COMMENT 'spectral template name (among 21)',&lt;br /&gt;
    `template_int` int COMMENT 'spectral template as integer (from 0 to 20)',&lt;br /&gt;
    `h` float COMMENT 'approximate H-band magnitude for information only. This was computed for applying the magnitude cut'&lt;br /&gt;
    )&lt;br /&gt;
    CLUSTERED BY (&lt;br /&gt;
    id&lt;br /&gt;
    )&lt;br /&gt;
    SORTED BY ( &lt;br /&gt;
    id ASC&lt;br /&gt;
    ) &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;
&lt;br /&gt;
    INSERT OVERWRITE TABLE cosmohub.full_H25cut_Hcol_v1_1_c&lt;br /&gt;
    SELECT `id`, `type`, `z`,`m1450`, `template`,&lt;br /&gt;
    CASE WHEN template = 'Banados_avg_Harris' THEN 0 &lt;br /&gt;
     WHEN template = 'Banados_avg_Selsing' THEN 1&lt;br /&gt;
     WHEN template = 'Banados_avg_Vandenberk' THEN 2&lt;br /&gt;
     WHEN template = 'Banados_hlya_Harris' THEN 3&lt;br /&gt;
     WHEN template = 'Banados_hlya_Selsing' THEN 4&lt;br /&gt;
     WHEN template = 'Banados_hlya_Vandenberk' THEN 5&lt;br /&gt;
     WHEN template = 'Banados_llya_Harris' THEN 6&lt;br /&gt;
     WHEN template = 'Banados_llya_Selsing' THEN 7&lt;br /&gt;
     WHEN template = 'Banados_llya_Vandenberk' THEN 8&lt;br /&gt;
     WHEN template = 'Hewett_l0_cb' THEN 9&lt;br /&gt;
     WHEN template = 'Hewett_l0_cr' THEN 10&lt;br /&gt;
     WHEN template = 'Hewett_l0_cs' THEN 11&lt;br /&gt;
     WHEN template = 'Hewett_ld_cb' THEN 12&lt;br /&gt;
     WHEN template = 'Hewett_ld_cr' THEN 13&lt;br /&gt;
     WHEN template = 'Hewett_ld_cs' THEN 14&lt;br /&gt;
     WHEN template = 'Hewett_lh_cb' THEN 15&lt;br /&gt;
     WHEN template = 'Hewett_lh_cr' THEN 16&lt;br /&gt;
     WHEN template = 'Hewett_lh_cs' THEN 17&lt;br /&gt;
     WHEN template = 'Hewett_ls_cb' THEN 18&lt;br /&gt;
     WHEN template = 'Hewett_ls_cr' THEN 19&lt;br /&gt;
     WHEN template = 'Hewett_ls_cs' THEN 20&lt;br /&gt;
    END as template_int,&lt;br /&gt;
    `h`&lt;br /&gt;
    FROM tallada.full_H25cut_Hcol;  &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
    ANALYZE TABLE cosmohub.full_H25cut_Hcol_v1_1_c COMPUTE STATISTICS FOR COLUMNS;&lt;/div&gt;</summary>
		<author><name>Jcarrete</name></author>
	</entry>
</feed>