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<ri:Resource created="2016-05-27T12:22:12Z" status="active" updated="2025-06-13T15:25:00Z" 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>HST observations of QSOs with medium spectra</title><shortName>J/ApJ/818/113</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/113</identifier><altIdentifier>doi:10.26093/cds/vizier.18180113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neeleman M.</name></creator><creator><name>Prochaska J.X.</name></creator><creator><name>Ribaudo J.</name></creator><creator><name>Lehner N.</name></creator><creator><name>Howk J.C.</name></creator><creator><name>Rafelski M.,Kanekar N.</name></creator><date role="Updated">2022-10-05T07:44:20Z</date><date role="Created">2016-05-27T12:22:12Z</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>spectroscopy</subject><subject>ultraviolet-astronomy</subject><description>We use the Hubble Space Telescope (HST) archive of ultraviolet (UV) quasar spectroscopy to conduct the first blind survey for damped Ly{alpha} absorbers (DLAs) at low redshift (z&lt;1.6). Our statistical sample includes 463 quasars with spectral coverage spanning a total redshift path {Delta}z=123.3 or an absorption path {Delta}X=229.7. Within this survey path, we identify 4 DLAs defined as absorbers with HI column density N_HI_&gt;=10^20.3^/cm2, which implies an incidence per absorption length lDLA(X)=0.017_-0.008_^+0.014^ at a median survey path redshift of z=0.623. While our estimate of l_DLA_(X) is lower than earlier estimates at z~0 from HI 21cm emission studies, the results are consistent within the measurement uncertainties. Our data set is too small to properly sample the N_HI_ frequency distribution function f(N_HI_,X), but the observed distribution agrees with previous estimates at z&gt;2. Adopting the z&gt;2 shape of f(N_HI_, X), we infer an HI mass density at z~0.6 of {rho}_HI_^DLA^=0.25_-0.12_^+0.20^. This is significantly lower than previous estimates from targeted DLA surveys with the HST, but consistent with results from low-z HI 21cm observations, and suggests that the neutral gas density of the universe has been decreasing over the past 10Gyr.</description><source format="bibcode">2016ApJ...818..113N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/113</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/217">J/MNRAS/452/217 : HI cosmological mass density at z=5 (Crighton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/161">J/ApJ/779/161 : MgII absorbers in 0.4&lt;z&lt;2.3 SDSS QSOs (Seyffert+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/547/L1">J/A+A/547/L1 : SDSS-III DR9 DLA catalogue (Noterdaeme+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/89">J/ApJ/755/89 : Metallicities of damped Ly{alpha} systems (Rafelski+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/42">J/ApJ/736/42 : HST QSO Catalog (Ribaudo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/1087">J/A+A/505/1087 : DLAs in SDSS-DR7 (Noterdaeme+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/636/610">J/ApJ/636/610 : Damped Ly{alpha} systems at z&lt;1.65 (Rao+, 2006)</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/MNRAS/354/L31">J/MNRAS/354/L31 : SDSS DR2 QSO and DLA properties (Murphy+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/140/143">J/ApJS/140/143 : HST FOS spectral atlas (Bechtold+, 2002)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/818/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/818/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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