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<ri:Resource created="2025-12-22T12:41:14Z" status="active" updated="2026-03-02T06:25:50Z" 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>Re-classification of high-redshift QSOs</title><shortName>J/A+A/704/A343</shortName><identifier>ivo://CDS.VizieR/J/A+A/704/A343</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Meusinger H.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2025-12-22T12:41:14Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>galaxies</subject><subject>quasars</subject><subject>stellar-spectral-types</subject><subject>white-dwarf-stars</subject><subject>supernovae</subject><description>The discovery of outsiders in the form of unusual, rare, or even unknown object types is important as they can provide useful information about otherwise hidden physical phenomena and processes. The present study takes advantage of the fact that the automated spectroscopic pipeline of the Sloan Digital Sky Survey (SDSS) occasionally assigns uncommon spectra to high-redshift quasi-stellar objects (QSOs). This study presents an analysis of about 4000 spectra that are QSOs with redshifts z&gt;4.5 according to the spectroscopic pipeline of the Sloan Digital Sky Survey (SDSS) DR16. It turns out that, after excluding non-classifiable spectra of low quality and those from three special plates, only 26% are high-z QSOs, 50% are QSOs at lower redshifts, 16% are galaxies, and 8% are stars. A significant proportion of the latter three categories prove to be unusual and are re-assigned here to a variety of rare spectral types. The results of the re-evaluation are summarised in the catalogue.</description><source format="bibcode">2025A&amp;A...704A.343M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/704/A343</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/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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