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<ri:Resource created="2022-02-18T10:14:46Z" 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>Ghostly damped Ly{alpha} systems in SDSS DR14</title><shortName>J/ApJ/901/123</shortName><identifier>ivo://CDS.VizieR/J/ApJ/901/123</identifier><altIdentifier>doi:10.26093/cds/vizier.19010123</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fathivavsari H.</name></creator><date role="Updated">2022-08-25T11:42:14Z</date><date role="Created">2022-02-18T10:14:46Z</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>spectroscopy</subject><subject>redshifted</subject><subject>intergalactic-medium</subject><description>We report the discovery of 59 new ghostly absorbers from the Sloan Digital Sky Survey Data Release 14. These absorbers, with z_abs_~z_QSO_, reveal no Ly{alpha} absorption, and they are mainly identified through the detection of strong metal absorption lines in the spectra. The number of such previously known systems is 30. The new systems are found with the aid of machine-learning algorithms. The spectra of 41 (out of total of 89) absorbers also cover the Ly{beta} spectral region. By fitting the damping wings of the Ly{beta} absorption in the stacked spectrum of 21 (out of 41) absorbers with relatively stronger Ly{beta} absorption, we measured an HI column density of log N(HI)=21.50. This column density is 0.5dex higher than that of the previous work. We also found that the metal absorption lines in the stacked spectrum of the 21 ghostly absorbers with stronger Ly{beta} absorption have similar properties as those in the stacked spectrum of the remaining systems. This circumstantial evidence strongly suggests that the majority of our ghostly absorbers are indeed DLAs.</description><source format="bibcode">2020ApJ...901..123F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/901/123</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/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/286">VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/508/200">J/ApJ/508/200 : QSO low-z Ly{alpha} absorbers (Tripp+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/524/536">J/ApJ/524/536 : Nearby Ly{alpha} quasar absorbers (Impey+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/116/622">J/PASP/116/622 : SDSS damped Ly{alpha} survey: DR1 (Prochaska+, 2004)</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/A+A/547/L1">J/A+A/547/L1 : SDSS-III DR9 DLA catalogue (Noterdaeme+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/449/1536">J/MNRAS/449/1536 : New damped Ly{alpha} absorbers (Turnshek+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/1850">J/MNRAS/472/1850 : Detecting damped Ly{alpha} absorbers (Garnett+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/477/5625">J/MNRAS/477/5625 : SDSSDR12 eclipsing damped Lya systems (Fathivavsari+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/888/85">J/ApJ/888/85 : Ghostly strong Lya abs. in SDSS DR12 (Fathivavsari, 2020)</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/901/123</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/901/123</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/901/123</mirrorURL></interface></capability><capability><interface 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