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<ri:Resource created="2026-09-03T14:52:04Z" status="active" updated="2026-09-09T00:00:00Z" 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>New redshift 1.6&lt;z&lt;4.2 of QUBRICS QSOs</title><shortName>J/MNRAS/522/2019</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/522/2019</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cristiani S.</name></creator><creator><name>Porru M.</name></creator><creator><name>Guarneri F.</name></creator><creator><name>Calderone G.</name></creator><creator><name>Boutsia K.</name></creator><creator><name>Grazian A.,Cupani G.</name></creator><creator><name>D'Odorico V.</name></creator><creator><name>Fontanot F.</name></creator><creator><name>Martins C.J.A.P.</name></creator><creator><name>Marques C.M.J.,Maitra S.</name></creator><creator><name>Trost A.</name></creator><date role="Updated">2026-09-03T13:54:36Z</date><date role="Created">2026-09-03T14:52:04Z</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>surveys</subject><subject>quasars</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>astrometry</subject><subject>spectroscopy</subject><description>The QUBRICS (QUasars as BRIght beacons for Cosmology in the Southern hemisphere) survey aims at constructing a sample of the brightest quasars with z~&gt;2.5, observable with facilities in the Southern Hemisphere. 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A Golden Sample of seven quasars is presented that makes it possible to carry out this experiment in about 1500 h of observation in 25 yr, using the ANDES spectrograph at the 39m ELT, a significant improvement with respect to previous estimates.</description><source format="bibcode">2023MNRAS.522.2019C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/522/2019</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/J/MNRAS/511/572">J/MNRAS/511/572 : High-redshift Ultraluminous QSOs with SMSS DR3</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/482/3458">J/MNRAS/482/3458 : UVES Spectral Quasar Absorption Database DR1 (Murphy+,2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/887/268">J/ApJ/887/268 : Bright QSOs in Southern Hemisphere (QUBRICS)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/871/258">J/ApJ/871/258 : ELQS in SDSS. 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