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<ri:Resource created="2021-06-25T15:52:00Z" 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>Strongly lensed quasars in SDSS</title><shortName>J/MNRAS/477/L70</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/477/L70</identifier><altIdentifier>doi:10.26093/cds/vizier.74779070</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Williams P.R.</name></creator><creator><name>Agnello A.</name></creator><creator><name>Treu T.</name></creator><creator><name>Abramson L.E.</name></creator><creator><name>Anguita T.,Apostolovski Y.</name></creator><creator><name>Chen G.C.-F.</name></creator><creator><name>Fassnacht C.D.</name></creator><creator><name>Hsueh J.W.</name></creator><creator><name>Lemaux B.C.,Motta V.</name></creator><creator><name>Oldham L.</name></creator><creator><name>Rojas K.</name></creator><creator><name>Rusu C.E.</name></creator><creator><name>Shajib A.J.</name></creator><creator><name>Wang X.</name></creator><date role="Updated">2024-08-18T20:19:35Z</date><date role="Created">2021-06-25T15:52:00Z</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>gravitational-lensing</subject><subject>redshifted</subject><description>We present the discovery of three quasar lenses in the Sloan Digital Sky Survey, selected using two novel photometry-based selection techniques. The J0941+0518 system, with two point sources separated by 5.46 arcsec on either side of a galaxy, has source and lens redshifts 1.54 and 0.343. Images of J2257+2349 show two point sources separated by 1.67 arcsec on either side of an E/S0 galaxy. The extracted spectra show two images of the same quasar at z_s_=2.10. SDSS J1640+1045 has two quasar spectra at z_s_=1.70 and fits to the SDSS and Pan-STARRS images confirm the presence of a galaxy between the two point sources. We observed 56 photometrically selected lens candidates in this follow-up campaign, confirming three new lenses, re-discovering one known lens, and ruling out 36 candidates, with 16 still inconclusive. 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