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<ri:Resource created="2013-01-10T14:38:11Z" 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>New 2.2&lt;z&lt;3 quasars from SDSS and UKIDSS</title><shortName>J/AJ/142/78</shortName><identifier>ivo://CDS.VizieR/J/AJ/142/78</identifier><altIdentifier>doi:10.26093/cds/vizier.51420078</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wu X.-B.</name></creator><creator><name>Wang R.</name></creator><creator><name>Schmidt K.B.</name></creator><creator><name>Bian F.</name></creator><creator><name>Jiang L.</name></creator><creator><name>Fan X.</name></creator><date role="Updated">2018-01-05T08:57:11Z</date><date role="Created">2013-01-10T14:38:11Z</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>active-galactic-nuclei</subject><subject>redshifted</subject><subject>infrared-photometry</subject><description>The identification of quasars in the redshift range 2.2&lt;z&lt;3 is known to be very inefficient because the optical colors of such quasars are indistinguishable from those of stars. Recent studies have proposed using optical variability or near-infrared (near-IR) colors to improve the identification of the missing quasars in this redshift range. Here we present a case study combining both methods. We select a sample of 70 quasar candidates from variables in Sloan Digital Sky Survey (SDSS) Stripe 82, which are non-ultraviolet excess sources and have UKIDSS near-IR public data. They are clearly separated into two parts on the Y-K/g-z color-color diagram, and 59 of them meet or lie close to a newly proposed Y-K/g-z selection criterion for z&lt;4 quasars. Of these 59 sources, 44 were previously identified as quasars in SDSS DR7, and 35 of them are quasars at 2.2&lt;z&lt;3. We present spectroscopic observations of 14 of 15 remaining quasar candidates using the Bok 2.3m telescope and the MMT 6.5m telescope, and successfully identify all of them as new quasars at z=2.36-2.88. We also apply this method to a sample of 643 variable quasar candidates with SDSS-UKIDSS nine-band photometric data selected from 1875 new quasar candidates in SDSS Stripe 82 given by Butler &amp; Bloom (2011AJ....141...93B) based on the time-series selections, and find that 188 of them are probably new quasars with photometric redshifts at 2.2&lt;z&lt;3. Our results indicate that the combination of optical variability and optical/near-IR colors is probably the most efficient way to find 2.2&lt;z&lt;3 quasars and is very helpful for constructing a complete quasar sample. We discuss its implications for ongoing and upcoming large optical and near-IR sky surveys.</description><source format="bibcode">2011AJ....142...78W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/78</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/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/314">I/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource>http://www.sdss.org : SDSS Home 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