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<ri:Resource created="2014-12-01T09:58:49Z" 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>HST survey for Lyman limit systems. II.</title><shortName>J/ApJ/765/137</shortName><identifier>ivo://CDS.VizieR/J/ApJ/765/137</identifier><altIdentifier>doi:10.26093/cds/vizier.17650137</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>O'Meara J.M.</name></creator><creator><name>Prochaska J.X.</name></creator><creator><name>Worseck G.</name></creator><creator><name>Chen H.-W.</name></creator><creator><name>Madau P.</name></creator><date role="Updated">2017-06-27T06:37:49Z</date><date role="Created">2014-12-01T09:58:49Z</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>visible-astronomy</subject><subject>sloan-photometry</subject><subject>redshifted</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>surveys</subject><description>We present the first science results from our Hubble Space Telescope survey for Lyman limit absorption systems (LLS) using the low dispersion spectroscopic modes of the Advanced Camera for Surveys and the Wide Field Camera 3. Through an analysis of 71 quasars, we determine the incidence frequency of LLS per unit redshift and per unit path length, l(z) and l(X), respectively, over the redshift range 1&lt;z&lt;2.6, and find a weighted mean of l(X)=0.29+/-0.05 for 2.0&lt;z&lt;2.5 through a joint analysis of our sample and that of Ribaudo et al. (2011, J/ApJ/736/42). Through stacked spectrum analysis, we determine a median (mean) value of the mean free path to ionizing radiation at z=2.4 of {lambda}^912^_mfp_=243(252)h^-1^_72_Mpc, with an error on the mean value of +/-43h^-1^_72_Mpc. We also re-evaluate the estimates of {lambda}^912^_mfp_ from Prochaska et al. (2010, J/ApJ/718/392) and place constraints on the evolution of {lambda}^912^_mfp_ with redshift, including an estimate of the "breakthrough" redshift of z=1.6. Consistent with results at higher z, we find that a significant fraction of the opacity for absorption of ionizing photons comes from systems with N_HI_&lt;=10^17.5^cm^-2^ with a value for the total Lyman opacity of {tau}^Lyman^_eff_=0.40+/-0.15. Finally, we determine that at minimum, a 5-parameter (4 power law) model is needed to describe the column density distribution function f(N_HI_,X) at z~2.4, find that f(N_HI_,X) undergoes no significant change in shape between z~2.4 and z~3.7, and provide our best fit model for f(N_HI_,X).</description><source format="bibcode">2013ApJ...765..137O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/765/137</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 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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/AJ/131/2766">J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/427">J/A+A/458/427 : Lyman alpha absorbers in 0.5&lt;z&lt;1.9 QSOs (Janknecht+, 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/MNRAS/335/555">J/MNRAS/335/555 : Lyman-alpha forest of 5 QSOs (Kim+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/373/757">J/A+A/373/757 : Lyman-Alpha Forest of 3 QSOs (Kim+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/475/469">J/ApJ/475/469 : Composite HST Spectrum of Quasars (Zheng+ 1997)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home page</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/765/137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/765/137</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/765/137</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/765/137</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/765/137</mirrorURL><mirrorURL 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