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<ri:Resource created="2021-05-28T13:57:11Z" status="active" updated="2025-06-13T15:25:00Z" 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>Sunyaev-Zel'dovich galaxy clusters surveyed by ACT</title><shortName>J/ApJS/253/3</shortName><identifier>ivo://CDS.VizieR/J/ApJS/253/3</identifier><altIdentifier>doi:10.26093/cds/vizier.22530003</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hilton M.</name></creator><creator><name>Sifon C.</name></creator><creator><name>Naess S.</name></creator><creator><name>Madhavacheril M.</name></creator><creator><name>Oguri M.</name></creator><creator><name>Rozo E.,Rykoff E.</name></creator><creator><name>Abbott T.M.C.</name></creator><creator><name>Adhikari S.</name></creator><creator><name>Aguena M.</name></creator><creator><name>Aiola S.</name></creator><creator><name>Allam S.,Amodeo S.</name></creator><creator><name>Amon A.</name></creator><creator><name>Annis J.</name></creator><creator><name>Ansarinejad B.</name></creator><creator><name>Aros-Bunster C.,Austermann J.E.</name></creator><creator><name>Avila S.</name></creator><creator><name>Bacon D.</name></creator><creator><name>Battaglia N.</name></creator><creator><name>Beall J.A.</name></creator><creator><name>Becker D.T.,Bernstein G.M.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Bhandarkar T.</name></creator><creator><name>Bhargava S.</name></creator><creator><name>Bond J.R.</name></creator><creator><name>Brooks D.,Burke D.L.</name></creator><creator><name>Calabrese E.</name></creator><creator><name>Carrasco Kind M.</name></creator><creator><name>Carretero J.</name></creator><creator><name>Choi S.K.,Choi A.</name></creator><creator><name>Conselice C.</name></creator><creator><name>da Costa L.N.</name></creator><creator><name>Costanzi M.</name></creator><creator><name>Crichton D.,Crowley K.T.</name></creator><creator><name>Dunner R.</name></creator><creator><name>Denison E.V.</name></creator><creator><name>Devlin M.J.</name></creator><creator><name>Dicker S.R.</name></creator><creator><name>Diehl H.T.,Dietrich J.P.</name></creator><creator><name>Doel P.</name></creator><creator><name>Duff S.M.</name></creator><creator><name>Duivenvoorden A.J.</name></creator><creator><name>Dunkley J.,Everett S.</name></creator><creator><name>Ferraro S.</name></creator><creator><name>Ferrero I.</name></creator><creator><name>Ferte A.</name></creator><creator><name>Flaugher B.</name></creator><creator><name>Frieman J.,Gallardo P.A.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Gaztanaga E.</name></creator><creator><name>Gerdes D.W.</name></creator><creator><name>Giles P.,Golec J.E.</name></creator><creator><name>Gralla M.B.</name></creator><creator><name>Grandis S.</name></creator><creator><name>Gruen D.</name></creator><creator><name>Gruendl R.A.</name></creator><creator><name>Gschwend J.,Gutierrez G.</name></creator><creator><name>Han D.</name></creator><creator><name>Hartley W.G.</name></creator><creator><name>Hasselfield M.</name></creator><creator><name>Hill J.C.</name></creator><creator><name>Hilton G.C.,Hincks A.D.</name></creator><creator><name>Hinton S.R.</name></creator><creator><name>Ho S.-P.P.</name></creator><creator><name>Honscheid K.</name></creator><creator><name>Hoyle B.</name></creator><creator><name>Hubmayr J.,Huffenberger K.M.</name></creator><creator><name>Hughes J.P.</name></creator><creator><name>Jaelani A.T.</name></creator><creator><name>Jain B.</name></creator><creator><name>James D.J.,Jeltema T.</name></creator><creator><name>Kent S.</name></creator><creator><name>Knowles K.</name></creator><creator><name>Koopman B.J.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Lahav O.</name></creator><creator><name>Lima M.,Lin Y.-T.</name></creator><creator><name>Lokken M.</name></creator><creator><name>Loubser S.I.</name></creator><creator><name>MacCrann N.</name></creator><creator><name>Maia M.A.G.</name></creator><creator><name>Marriage T.A.,Martin J.</name></creator><creator><name>McMahon J.</name></creator><creator><name>Melchior P.</name></creator><creator><name>Menanteau F.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Miyatake H.,Moodley K.</name></creator><creator><name>Morgan R.</name></creator><creator><name>Mroczkowski T.</name></creator><creator><name>Nati F.</name></creator><creator><name>Newburgh L.B.</name></creator><creator><name>Niemack M.D.,Nishizawa A.J.</name></creator><creator><name>Ogando R.L.C.</name></creator><creator><name>Orlowski-Scherer J.</name></creator><creator><name>Page L.A.</name></creator><creator><name>Palmese A.,Partridge B.</name></creator><creator><name>Paz-Chinchon F.</name></creator><creator><name>Phakathi P.</name></creator><creator><name>Plazas A.A.</name></creator><creator><name>Robertson N.C.,Romer A.K.</name></creator><creator><name>Carnero Rosell A.</name></creator><creator><name>Salatino M.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Schaan E.,Schillaci A.</name></creator><creator><name>Sehgal N.</name></creator><creator><name>Serrano S.</name></creator><creator><name>Shin T.</name></creator><creator><name>Simon S.M.</name></creator><creator><name>Smith M.,Soares-Santos M.</name></creator><creator><name>Spergel D.N.</name></creator><creator><name>Staggs S.T.</name></creator><creator><name>Storer E.R.</name></creator><creator><name>Suchyta E.,Swanson M.E.C.</name></creator><creator><name>Tarle G.</name></creator><creator><name>Thomas D.</name></creator><creator><name>To C.</name></creator><creator><name>Trac H.</name></creator><creator><name>Ullom J.N.</name></creator><creator><name>Vale L.R.,Van Lanen J.</name></creator><creator><name>Vavagiakis E.M.</name></creator><creator><name>De Vicente J.</name></creator><creator><name>Wilkinson R.D.</name></creator><creator><name>Wollack E.J.,Xu Z.</name></creator><creator><name>Zhang Y.</name></creator><date role="Updated">2023-09-05T07:53:48Z</date><date role="Created">2021-05-28T13:57:11Z</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>galaxy-clusters</subject><subject>redshifted</subject><subject>radio-sources</subject><subject>visible-astronomy</subject><subject>gravitational-lensing</subject><description>We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio &gt;4 in 13211deg^2^ of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multifrequency matched filter to 98 and 150GHz maps constructed from ACT observations obtained from 2008 to 2018 and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04&lt;z&lt;1.91 (median z=0.52). The catalog contains 222 z&gt;1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ signal versus mass-scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M_500c_&gt;3.8x10^14^M_{sun}_, evaluated at z=0.5, for clusters detected at signal-to-noise ratio &gt;5 in maps filtered at an angular scale of 2.4'. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ signal mass-scaling relation, such as the Dark Energy Survey (4566deg^2^), the Hyper Suprime-Cam Subaru Strategic Program (469deg^2^), and the Kilo Degree Survey (825deg^2^). We highlight some noteworthy objects in the sample, including potentially projected systems, clusters with strong lensing features, clusters with active central galaxies or star formation, and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10Gyr.</description><source format="bibcode">2021ApJS..253....3H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/253/3</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/110">VII/110 : Rich Clusters of Galaxies (Abell+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/177">VII/177 : Redshifts and Velocity Dispersions for Abell Clusters (Struble+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/203">VII/203 : Las Campanas Redshift Survey (Shectman+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/91">VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)</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/II/343">II/343 : VIKING catalogue data release 2 (Edge+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/347">II/347 : KiDS-ESO-DR3 multi-band source catalog (de Jong+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/357">II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/269/151">J/MNRAS/269/151 : APM cluster redshift survey (Dalton+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/274/75">J/MNRAS/274/75 : Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/502/558">J/ApJ/502/558 : Catalog of ROSAT galaxy clusters (Vikhlinin+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/514/148">J/ApJ/514/148 : ROSAT survey of bright galaxies clusters (De Grandi+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/129/435">J/ApJS/129/435 : NORAS galaxy cluster survey. 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47360 47362 47364-47365 47390 47427 47430 47435 47438-47439 47446 47450 47459-47460 47463 47465 47470 47482 47509 47580 48076 48130 48171 48174 48199 48254 48258 48272 48344 48346 48375 48396 48405 48423 48431 48445 48454 48479 48498 48510 48576 48583 48605-48606 48622 48639 48684 48688 48692 48737 48741 48963 48966 48970 48974 48977 48979 49009 49012 49025 49077 49104 49145 49147</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/253/3?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/253/3/clusters</name><description>Cluster catalog</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ACT-CL</name><description>Cluster name (JHHMM.m+DDMM) (name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>primary</flag></column><column><name>HSC</name><description>[0/1] Flag indicating if the cluster falls within the HSC-SSP S19A footprint (footprint_HSCs19a) (7)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KiDS</name><description>[0/1] Flag indicating if the cluster falls within the KiDS DR4 footprint (footprint_KiDSDR4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>delta</name><description>[-0.2/24.1]? Density contrast statistic ({delta}) measured at the zCluster photometric redshift (zCluster_delta)</description><ucd>phys.density;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_delta</name><description>[0.08/3.3]? Delta uncertainty (zCluster_errDelta)</description><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Source</name><description>Photometry used for zCluster measurements (see Section 3.1.4) (zCluster_source) (8)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000) of the SZ detection by ACT</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-60/20.5] Declination in decimal degrees (J2000) of the SZ detection by ACT</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SNR</name><description>[4/54] Signal-to-noise ratio, optimized over all filter scales</description><ucd>stat.snr;instr.filter</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>y0</name><description>[0.2/13.2] Central Comptonization parameter measured using the optimal matched filter template (i.e., the one that maximizes S/N) (y_c)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_y0</name><description>[0.05/0.7] Y0 uncertainty (err_y_c)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNR2.4</name><description>[2.8/54] Signal-to-noise ratio at the reference 2.4' filter scale (fixed_SNR)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fy0</name><description>[0.2/6] Central Comptonization parameter measured at the reference 2.4' filter scale (fixed_y_c)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_fy0</name><description>[0.07/0.3] Fy0 uncertainty (fixed_err_y_c)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ftemp</name><description>Name of the matched filter template resulting in the highest S/N detection of this cluster (template)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Tile</name><description>Name of the ACT map tile (typically with dimensions 10degx5deg) in which the cluster was found (tileName)</description><ucd>obs.image</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>z</name><description>[0.03/2] Adopted redshift for the cluster (redshift)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_z</name><description>[0/0.21] z uncertainty (only for photometric redshifts) (redshiftErr)</description><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_z</name><description>Redshift type (spec=spectroscopic (1649 occurrences) or phot=photometric (2546 occurrences)) (redshiftType)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_z</name><description>Reference on z (redshiftSource) (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>M500c</name><description>[1/13.5] Cluster mass estimate (M_500c_) within a spherical radius that encloses an average density equal to 500 times the critical density at the cluster redshift (2)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500c</name><description>[0.2/3] M500c positive uncertainty (M500c_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500c</name><description>M500c negative uncertainty (M500c_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500cC</name><description>[1.4/19] Rescaled M_500c_ (M500cCal) (3)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500cC</name><description>[0.4/4.5] M500cC positive uncertainty (M500cCal_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500cC</name><description>M500cC negative uncertainty (M500cCal_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M200m</name><description>[1.9/25.5] M_200_ with respect to the mean density (M200m) (4)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M200m</name><description>[0.4/6.2] M200m positive uncertainty (M200m_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M200m</name><description>M200m negative uncertainty (M200m_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500cUnc</name><description>[1.2/16.3] Uncorrected M_500c_ (M500cUncorr) (5)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500cUnc</name><description>[0.3/4.4] M500cUnc positive uncertainty (M500cUncorr_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500cUnc</name><description>M500cUnc negative uncertainty (M500cUncorr_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M200mUnc</name><description>[2.2/31] Uncorrected M_200_ (M200mUncorr) (6)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M200mUnc</name><description>[0.5/9.3] M200mUnc positive uncertainty (M200mUncorr_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M200mUnc</name><description>M200mUnc negative uncertainty (M200mUncorr_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DES</name><description>[0/1] Flag indicating if the cluster falls within the DES Y3 footprint (footprint_DESY3)</description><ucd>meta.code</ucd></column><column><name>redM</name><description>[0/1] Flag indicating cross-match with a redMaPPer-detected cluster in the SDSS footprint (Rykoff+ 2014, J/ApJ/785/104) (RM)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lamSDSS</name><description>[20/300]? Optical richness ({lambda}) measurement for the redMaPPer algorithm in the SDSS footprint (RM_LAMBDA)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_lamSDSS</name><description>[1.7/32]? LambdaSDSS uncertainty (RM_LAMBDA_ERR)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>redMDES</name><description>[0/1] Flag indicating cross-match with a redMaPPer-detected cluster in the DES Y3 footprint (RMDESY3) (9)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lamDES</name><description>[20/248]? Optical richness ({lambda}) measurement for the redMaPPer algorithm in the DES Y3 footprint (RMDESY3_LAMBDA_CHISQ)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_lamDES</name><description>[1.4/179]? LambdaDES uncertainty (RMDESY3_LAMBDA_CHISQ_E)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CAMIRA</name><description>[0/1] Flag indicating cross-match with a CAMIRA-detected cluster in the HSCSSP S19A footprint (CAMIRA) (10)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ncamira</name><description>[10.4/118]? Optical richness measurement for the CAMIRA algorithm in the HSCSSP S19A footprint (CAMIRA_N_mem)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAOdeg</name><description>? Alternative optically right ascension (J2000) from a heterogeneous collection of measurements (opt_RADeg)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEOdeg</name><description>? Alternative optically declination (J2000) from a heterogeneous collection of measurements (opt_decDeg)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>r_Optpos</name><description>Reference of the alternative optical position (opt_positionSource) (11)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Notes</name><description>Notes (12)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>knownLens</name><description>Name(s) of known strong gravitational lenses within 2Mpc projected distance of this cluster</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="42*">char</dataType></column><column><name>r_knownLens</name><description>Reference(s) on knownLens (knownLensRefCode) (13)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Warnings</name><description>Warning message related to the redshift measurement for this cluster (e.g., possible projected system)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="93*">char</dataType></column><column><name>Mult</name><description>indicates that the cluster is in a pair or group of clusters (link to Table 4)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJS/253/3/multsys</name><description>Systems of multiple SZ sources (Table 4)</description><column><name>ACT-CL</name><description>Cluster name (JHHMM.m+DDMM) (name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>ACT-CL3</name><description>3rd ACT-CL cluster name (JHHMM.m+DDMM)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>ACT-CL4</name><description>4th ACT-CL cluster name (JHHMM.m+DDMM)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>RAJ2000</name><description>Mean right ascension (J2000) (meanRADeg)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Mean declination (J2000) (meanDecDeg)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>[0.04/1.2] Mean redshift (meanRedshift)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NCl</name><description>[2/4] Number of clusters in group (numClusters)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Tile</name><description>Tile name (tileName)</description><ucd>obs.image</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ACT-CL2</name><description>2nd ACT-CL cluster name (JHHMM.m+DDMM)</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>SepMpc</name><description>[0.37/10] Maximum projected separation between the components in Mpc (maxSeparationMpc)</description><unit>Mpc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SepArcmin</name><description>[1.5/89.3] Maximum projected separation between the components in arcmin (maxSeparationArcmin)</description><unit>arcmin</unit><ucd>pos.angDistance;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Phot</name><description>[0/1] 1=objects with photometric redshifts (includesPhotoRedshift)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>