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<ri:Resource created="2018-05-15T17:20:58Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>HI-selected Lyman limit systems metallicities</title><shortName>J/ApJ/833/283</shortName><identifier>ivo://CDS.VizieR/J/ApJ/833/283</identifier><altIdentifier>doi:10.26093/cds/vizier.18330283</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lehner N.</name></creator><creator><name>O'Meara J.M.</name></creator><creator><name>Howk J.C.</name></creator><creator><name>Prochaska J.X.</name></creator><creator><name>Fumagalli M.</name></creator><date role="Updated">2018-09-18T15:28:21Z</date><date role="Created">2018-05-15T17:20:58Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>quasars</subject><subject>redshifted</subject><subject>chemical-abundances</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>h-i-line-emission</subject><subject>visible-astronomy</subject><description>We present the first results from our KODIAQ Z survey aimed at determining the metallicity distribution and physical properties of the z&gt;~2 partial and full Lyman limit systems (pLLSs and LLSs; 16.2&lt;=logN_HI_&lt;19), which are probed of the interface regions between the intergalactic medium (IGM) and galaxies. We study 31 HI-selected pLLSs and LLSs at 2.3&lt;z&lt;3.3 observed with Keck/HIRES in absorption against background QSOs. We compare the column densities of metal ions to HI and use photoionization models to assess the metallicity. The metallicity distribution of the pLLSs/LLSs at 2.3&lt;z&lt;3.3 is consistent with a unimodal distribution peaking at [X/H]~-2. The metallicity distribution of these absorbers therefore evolves markedly with z since at z&lt;~1 it is bimodal with peaks at [X/H]~-1.8 and -0.3. There is a substantial fraction (25%-41%) of pLLSs/LLSs with metallicities well below those of damped Ly{alpha} absorbers (DLAs) at any studied z from z&lt;~1 to z~2-4, implying reservoirs of metal-poor, cool, dense gas in the IGM/galaxy interface at all z. However, the gas probed by pLLSs and LLSs is rarely pristine, with a fraction of 3%-18% for pLLSs/LLSs with [X/H]&lt;=-3. We find C/{alpha} enhancement in several pLLSs and LLSs in the metallicity range -2&lt;~[X/H]&lt;~-0.5, where C/{alpha} is 2-5 times larger than observed in Galactic metal-poor stars or high-redshift DLAs at similar metallicities. This is likely caused by preferential ejection of carbon from metal-poor galaxies into their surroundings.</description><source format="bibcode">2016ApJ...833..283L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/833/283</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/596/768">J/ApJ/596/768 : Optical depths in 19 QSOs (Schaye+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/635/123">J/ApJ/635/123 : The SDSS-DR3 damped Ly{alpha} survey (Prochaska+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/137">J/ApJ/765/137 : HST survey for Lyman limit systems. 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