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<ri:Resource created="2025-11-12T14:23:01Z" status="active" updated="2026-07-02T12:00:39Z" 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>Galaxy-galaxy strong lens cand. from DELVE</title><shortName>J/ApJ/954/68</shortName><identifier>ivo://CDS.VizieR/J/ApJ/954/68</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xt-24</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zaborowski E.A.</name></creator><creator><name>Drlica-Wagner A.</name></creator><creator><name>Ashmead F.</name></creator><creator><name>Wu J.F.</name></creator><creator><name>Morgan R.,Bom C.R.</name></creator><creator><name>Shajib A.J.</name></creator><creator><name>Birrer S.</name></creator><creator><name>Cerny W.</name></creator><creator><name>Buckley-Geer E.J.,Mutlu-Pakdil B.</name></creator><creator><name>Ferguson P.S.</name></creator><creator><name>Glazebrook K.</name></creator><creator><name>Lozano S.J.G.</name></creator><creator><name>Gordon Y.,Martinez M.</name></creator><creator><name>Manwadkar V.</name></creator><creator><name>O'Donnell J.</name></creator><creator><name>Poh J.</name></creator><creator><name>Riley A.</name></creator><creator><name>Sakowska J.D.,Santana-Silva L.</name></creator><creator><name>Santiago B.X.</name></creator><creator><name>Sluse D.</name></creator><creator><name>Tan C.Y.</name></creator><creator><name>Tollerud E.J.,Verma A.</name></creator><creator><name>Carballo-Bello J.A.</name></creator><creator><name>Choi Y.</name></creator><creator><name>James D.J.</name></creator><creator><name>Kuropatkin N.,Martinez-Vazquez C.E.</name></creator><creator><name>Nidever D.L.</name></creator><creator><name>Castellon J.L.N.</name></creator><creator><name>Noel N.E.D.,Olsen K.A.G.</name></creator><creator><name>Pace A.B.</name></creator><creator><name>Mau S.</name></creator><creator><name>Yanny B.</name></creator><creator><name>Zenteno A.</name></creator><creator><name>Abbott T.M.C.,Aguena M.</name></creator><creator><name>Alves O.</name></creator><creator><name>Andrade-Oliveira F.</name></creator><creator><name>Bocquet S.</name></creator><creator><name>Brooks D.,Burke D.L.</name></creator><creator><name>Carnero Rosell A.</name></creator><creator><name>Carrasco Kind M.</name></creator><creator><name>Carretero J.,Castander F.J.</name></creator><creator><name>Conselice C.J.</name></creator><creator><name>Costanzi M.</name></creator><creator><name>Pereira M.E.S.,De Vicente J.</name></creator><creator><name>Desai S.</name></creator><creator><name>Dietrich J.P.</name></creator><creator><name>Doel P.</name></creator><creator><name>Everett S.</name></creator><creator><name>Ferrero I.,Flaugher B.</name></creator><creator><name>Friedel D.</name></creator><creator><name>Frieman J.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Gruen D.,Gruendl R.A.</name></creator><creator><name>Gutierrez G.</name></creator><creator><name>Hinton S.R.</name></creator><creator><name>Hollowood D.L.</name></creator><creator><name>Honscheid K.,Kuehn K.</name></creator><creator><name>Lin H.</name></creator><creator><name>Marshall J.L.</name></creator><creator><name>Melchior P.</name></creator><creator><name>Mena-Fernandez J.,Menanteau F.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Palmese A.</name></creator><creator><name>Paz-Chinchon F.</name></creator><creator><name>Pieres A.,Malagon A.A.P.</name></creator><creator><name>Prat J.</name></creator><creator><name>Rodriguez-Monroy M.</name></creator><creator><name>Romer A.K.</name></creator><creator><name>Sanchez E.,Scarpine V.</name></creator><creator><name>Sevilla-Noarbe I.</name></creator><creator><name>Smith M.</name></creator><creator><name>Suchyta E.</name></creator><creator><name>To C.,Weaverdyck N.</name></creator><creator><name>DELVE &amp; DES Collaborations</name></creator><date role="Updated">2026-07-02T12:00:39Z</date><date role="Created">2025-11-12T14:23:01Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>surveys</subject><description>We perform a search for galaxy-galaxy strong lens systems using a convolutional neural network (CNN) applied to imaging data from the first public data release of the DECam Local Volume Exploration Survey, which contains ~520 million astronomical sources covering ~4000deg2 of the southern sky to a 5{sigma} point-source depth of g=24.3, r=23.9, i=23.3, and z=22.8mag. Following the methodology of similar searches using Dark Energy Camera data, we apply color and magnitude cuts to select a catalog of ~11 million extended astronomical sources. After scoring with our CNN, the highest-scoring 50000 images were visually inspected and assigned a score on a scale from 0 (not a lens) to 3 (very probable lens). We present a list of 581 strong lens candidates, 562 of which are previously unreported. We categorize our candidates using their human-assigned scores, resulting in 55 Grade A candidates, 149 Grade B candidates, and 377 Grade C candidates. We additionally highlight eight potential quadruply lensed quasars from this sample. Due to the location of our search footprint in the northern Galactic cap (b&gt;10deg) and southern celestial hemisphere (decl.&lt;0deg), our candidate list has little overlap with other existing ground-based searches. Where our search footprint does overlap with other searches, we find a significant number of high-quality candidates that were previously unidentified, indicating a degree of orthogonality in our methodology. We report properties of our candidates including apparent magnitude and Einstein radius estimated from the image separation.</description><source format="bibcode">2023ApJ...954...68Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/954/68</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/II/371">II/371 : The Dark Energy Survey (DES): Data Release 2 (Abbott+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/964">J/ApJ/682/964 : Sloan lens ACS survey. V. 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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>Lens candidate identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>m_ID</name><description>Number of sources for this lens</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Rating</name><description>[0.3/2.6] Mean final rating</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Grade</name><description>Grade (A=high-confidence candidate) (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Type</name><description>Object type; Lens or source (2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>rE</name><description>[0.86/9.9]? 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