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<ri:Resource created="2024-03-01T11:03:44Z" status="active" updated="2025-09-09T14:15:03Z" 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 Clusters from SCUSS</title><shortName>J/PASP/132/B4101</shortName><identifier>ivo://CDS.VizieR/J/PASP/132/B4101</identifier><altIdentifier>doi:10.26093/cds/vizier.61333101</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gao J.</name></creator><creator><name>Zou H.</name></creator><creator><name>Zhou X.</name></creator><creator><name>Kong X.</name></creator><date role="Updated">2025-09-09T14:15:03Z</date><date role="Created">2024-03-01T11:03:44Z</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>galaxy-clusters</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><description>This paper presents the identification of galaxy clusters from the photometric redshift catalog based on three imaging surveys of SCUSS, Sloan Digital Sky Survey, and unWISE. By applying a fast clustering algorithm, we obtain a total of 19610 clusters in the redshift range of 0.05&lt;z&lt;0.65 over a sky area of about 3700 deg^2^ in the south Galactic gap. Monte Carlo simulations show that the false detection rate is about 8.9%. The redshift uncertainty is estimated to be about 0.013. The mass and richness of detected clusters are derived through the calibration based on the measurements of X-ray emission and Sunyaev-Zel'dovich effect. The median mass is 1.2x10^14^M_{sun}_.</description><source format="bibcode">2020PASP..132b4101G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/132/B4101</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/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/862/12">J/ApJ/862/12 : Photometric Redshift Catalog (SCUSS, SDSS, WISE) (Gao+, 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