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<ri:Resource created="2021-07-19T08:38:07Z" 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 strong Lya absorbers in SDSS DR12</title><shortName>J/ApJ/888/85</shortName><identifier>ivo://CDS.VizieR/J/ApJ/888/85</identifier><altIdentifier>doi:10.26093/cds/vizier.18880085</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fathivavsari H.</name></creator><date role="Updated">2021-10-25T10:15:53Z</date><date role="Created">2021-07-19T08:38:07Z</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>intergalactic-medium</subject><subject>redshifted</subject><description>We have searched the Sloan Digital Sky Survey Data Release 12 for ghostly strong Ly{alpha} (DLA) systems. These systems, located at the redshift of the quasars, show strong absorption from low-ionization atomic species but reveal no HI Ly{alpha} absorption. Our search has, for the first time, resulted in a sample of 30 homogeneously selected ghostly absorbers with z_QSO_&gt;2.0. Thirteen of the ghostly absorbers exhibit absorption from other HI Lyman series lines. The lack of Ly{alpha} absorption in these absorbers is consistent with them being dense and compact with projected sizes smaller than the broad-line region of the background quasar. Although uncertain, the estimated median HI column density of these absorbers is logN(HI)~21.0. We compare the properties of ghostly absorbers with those of eclipsing DLAs that are high-column-density absorbers, located within 1500km/s of the quasar emission redshift and showing strong Ly{alpha} emission in their DLA trough. We discover an apparent sequence in the observed properties of these DLAs, with ghostly absorbers showing wider HI kinematics, stronger absorptions from high-ionization species, CII and SiII excited states, and a higher level of dust extinction. Since we estimate that all these absorbers have similar metallicities, logZ/Z_{sun}_~-1.0, we conclude that ghostly absorbers are part of the same population as eclipsing DLAs, except that they are denser and located closer to the central active galactic nuclei.</description><source format="bibcode">2020ApJ...888...85F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/888/85</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/279">VII/279 : SDSS quasar catalog: twelfth data release (Paris+, 2017)</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/MNRAS/354/L31">J/MNRAS/354/L31 : SDSS DR2 QSO and DLA properties (Murphy+, 2004)</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/PASP/118/1077">J/PASP/118/1077 : Metal-strong damped Ly{alpha} systems (Herbert-Fort+, 2006)</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/663/320">J/ApJ/663/320 : IR-through-UV extinction curve (Fitzpatrick+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/392/998">J/MNRAS/392/998 : Damped Lyman{alpha} systems (Ellison+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/2302">J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)</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/other/ApSS/353.347">J/other/ApSS/353.347 : 398-710nm Sun spectral atlases (Fathivavsari+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/203">J/AJ/149/203 : Reddening of ~35000 quasars from SDSS (Krawczyk+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/462/3285">J/MNRAS/462/3285 : XQ-100. 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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>SDSS</name><description>SDSS name (HHMMSS.ss+DDMMSS.s; J2000)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>zQSO</name><description>[2.038/3.39] Quasar emission redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zabs</name><description>[2.035/3.387] Ghostly absorber absorption redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logNHI</name><description>[20.3/21.8]? Logarithm of HI column density (1)</description><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FeII1</name><description>[39/2373]? Rest equivalent width (in m{AA}) of the FeII{lambda}1608 absorption line</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FeII2</name><description>[674/4319]? Rest equivalent width (in m{AA}) of the FeII{lambda}2382 absorption line</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FeII3</name><description>[569/5869]? Rest equivalent width (in m{AA}) of the FeII{lambda}2600 absorption line</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AlII</name><description>[278/3278]? Rest equivalent width (in m{AA}) of the AlII{lambda}1670 absorption line</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MgII</name><description>[1562/4414]? Rest equivalent width (in m{AA}) of the MgII{lambda}2796 absorption line</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CII</name><description>[1001/5105]? 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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>ID</name><description>SDSS Plate-MJD-Fiber identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>z</name><description>[2.04/5.47] Quasar spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>S1</name><description>Member of the S-1 subsample? (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>S2</name><description>Member of the S-2 subsample? (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>S3</name><description>Member of the S-3 subsample? (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>S4</name><description>Member of the S-4 subsample? (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>S5</name><description>Member of the S-5 subsample? (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Ghost</name><description>Member of the ghostly absorbers?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>DR16Q</name><description>Display data from the SDSS-DR16Q catalog (VII/289) within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Sp</name><description>Interactive spectrum from SDSS-DR14</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from SDSS-DR14 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>_DE</name><description>Position from SDSS-DR14 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column></table></schema></tableset></ri:Resource>