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<ri:Resource created="2003-02-13T23:25:54Z" status="active" updated="2026-03-17T20:08:11Z" 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>Damped Lyman alpha absorption of QSOs</title><shortName>J/other/PASA/19.</shortName><identifier>ivo://CDS.VizieR/J/other/PASA/19.455</identifier><altIdentifier>doi:10.26093/cds/vizier/ds/bjkeff</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Curran S.J.</name></creator><creator><name>Webb J.K.</name></creator><creator><name>Murphy M.T.</name></creator><creator><name>Bandiera R.</name></creator><creator><name>Corbelli E.</name></creator><creator><name>Flambaum V.V.</name></creator><date role="Updated">2026-03-17T20:08:11Z</date><date role="Created">2003-02-13T23:25:54Z</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>radio-sources</subject><subject>radio-astronomy</subject><description>We present a catalogue of the 322 damped Lyman alpha absorbers taken from the literature. All damped Lyman alpha absorbers are included, with no selection on redshift or quasar magnitude. Of these, 123 are candidates and await confirmation using high resolution spectroscopy. For all 322 objects we catalogue the radio properties of the background quasars, when known. Around 60 quasars have radio flux densities above 0.1Jy and approximately half of these have optical magnitudes brighter than V=18. This compilation should prove useful in several areas of extragalactic/cosmological research.</description><source format="bibcode">2002PASA...19..455C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PASA/19.455</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/VII/224">VII/224 : Quasars and Active Galactic Nuclei (10th Ed.) 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>QSO name (When more than one zabs, the name is repeated)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType><flag>primary</flag></column><column><name>n_Name</name><description>[*] note detailed in "notes.dat" file</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>? Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DEJ2000</name><description>? Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>Pos</name><description>[SN] When no position: S: See section 2; N: Not published</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>zem</name><description>? Emission redshift of the quasar</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zabs</name><description>? Redshift of the Lyman{alpha} absorber</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>l_logNHI</name><description>[&gt;&lt;= ] Limit flag on logNHI</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>logNHI</name><description>? Columm density of the Lyman{alpha} absorber</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_logNHI</name><description>Reference for logNHI, in refnhi.dat</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>n_logNHI</name><description>[*W] Note on logNHI (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vmag</name><description>? V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_S0.4GHz</name><description>[~] Limit flag on S0.4GHz</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S0.4GHz</name><description>? Radio flux density at 0.44, 0.37 or 0.41GHz (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.200-400MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_S0.4GHz</name><description>[X] Note on S0.4GHz (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>r_S0.4GHz</name><description>Reference for S0.4GHz, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>S0.4GHzb</name><description>? Second radio flux density at 0.4GHz value</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.200-400MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_S0.4GHzb</name><description>Reference for S0.4GHzb, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_S1.4GHz</name><description>[&lt;~] Limit flag on 1.4GHz</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S1.4GHz</name><description>? Radio flux density at 1.4GHz</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_S1.4GHz</name><description>Reference for S1.4GHz, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>S1.4GHzb</name><description>? 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Radio flux density at 2.7GHz</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_S2.7GHz</name><description>[X] Note on S2.7GHz (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>r_S2.7GHz</name><description>Reference for S2.7GHz, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>l_S5.0GHz</name><description>[&lt;~ ] Limit flag on S5.0GHz</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>S5.0GHz</name><description>? Radio flux density at 5.0GHz</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_S5.0GHz</name><description>[X] Note on S5.0GHz (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>r_S5.0GHz</name><description>Reference for S5.0GHz, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>S5.0GHzb</name><description>? Second radio flux density at 5.0GHz value</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_S5.0GHzb</name><description>Note on S5.0GHzb, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>l_S1</name><description>[&lt;~ ] Limit flag on S1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>S1</name><description>? Radio flux density at "Freq1"</description><unit>Jy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Freq1</name><description>? 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Value of the Freq2 radio line</description><unit>GHz</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_S2</name><description>Notes on S2, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>l_S3</name><description>[~ ] Limit flag on S3</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>S3</name><description>? Radio flux density at "Freq3"</description><unit>Jy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Freq3</name><description>? Value of the Freq3 radio line</description><unit>GHz</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_S3</name><description>Notes on S3, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>S4</name><description>? Radio flux density at "Freq4"</description><unit>Jy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Freq4</name><description>? Value of the Freq4 radio line</description><unit>GHz</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_S4</name><description>[x] Reference for S4, in refflux.dat file</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/other/PASA/19.455/table2</name><description>The radio-loud DLAs in which H I absorption has been searched</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Quasar name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>l_tau</name><description>Limit flag on tau</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>tau</name><description>Optical depth of the H I line, with 3{sigma} limits</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_tau</name><description>[,-] Set of values, or range</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>tau2</name><description>? Other value or upper limit of tau</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logNHI</name><description>HI column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S</name><description>Approximate flux density at z_abs_</description><unit>Jy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sp+Index</name><description>? Spectral index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Notes</name><description>Notes (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType></column></table><table><name>J/other/PASA/19.455/refnhi</name><description>Damped Lyman alpha absorption references</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>Code for the references</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="31*">char</dataType></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="120*">char</dataType></column></table><table><name>J/other/PASA/19.455/notes</name><description>Individual notes</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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