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<ri:Resource created="2023-10-20T11:18:04Z" 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>SZ galaxy clusters from the ACTPol</title><shortName>J/ApJS/235/20</shortName><identifier>ivo://CDS.VizieR/J/ApJS/235/20</identifier><altIdentifier>doi:10.26093/cds/vizier.22350020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hilton M.</name></creator><creator><name>Hasselfield M.</name></creator><creator><name>Sifon C.</name></creator><creator><name>Battaglia N.</name></creator><creator><name>Aiola S.</name></creator><creator><name>Bharadwaj V.,Bond J.R.</name></creator><creator><name>Choi S.K.</name></creator><creator><name>Crichton D.</name></creator><creator><name>Datta R.</name></creator><creator><name>Devlin M.J.</name></creator><creator><name>Dunkley J.,Dunner R.</name></creator><creator><name>Gallardo P.A.</name></creator><creator><name>Gralla M.</name></creator><creator><name>Hincks A.D.</name></creator><creator><name>Ho S.-P.P.</name></creator><creator><name>Hubmayr J.,Huffenberger K.M.</name></creator><creator><name>Hughes J.P.</name></creator><creator><name>Koopman B.J.</name></creator><creator><name>Kosowsky A.</name></creator><creator><name>Louis T.,Madhavacheril M.S.</name></creator><creator><name>Marriage T.A.</name></creator><creator><name>Maurin L.</name></creator><creator><name>McMahon J.</name></creator><creator><name>Miyatake H.,Moodley K.</name></creator><creator><name>Naess S.</name></creator><creator><name>Nati F.</name></creator><creator><name>Newburgh L.</name></creator><creator><name>Niemack M.D.</name></creator><creator><name>Oguri M.,Page L.A.</name></creator><creator><name>Partridge B.</name></creator><creator><name>Schmitt B.L.</name></creator><creator><name>Sievers J.</name></creator><creator><name>Spergel D.N.,Staggs S.T.</name></creator><creator><name>Trac H.</name></creator><creator><name>van Engelen A.</name></creator><creator><name>Vavagiakis E.M.</name></creator><creator><name>Wollack E.J.</name></creator><date role="Updated">2023-12-11T20:11:43Z</date><date role="Created">2023-10-20T11:18:04Z</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>astronomical-object-identification</subject><subject>radio-sources</subject><subject>visible-astronomy</subject><description>We present a catalog of 182 galaxy clusters detected through the Sunyaev-Zel'dovich (SZ) effect by the Atacama Cosmology Telescope in a contiguous 987.5deg^2^ field. The clusters were detected as SZ decrements by applying a matched filter to 148GHz maps that combine the original ACT equatorial survey with data from the first two observing seasons using the ACTPol receiver. Optical/IR confirmation and redshift measurements come from a combination of large public surveys and our own follow-up observations. Where necessary, we measured photometric redshifts for clusters using a pipeline that achieves accuracy {Delta}z/(1+z)=0.015 when tested on Sloan Digital Sky Survey data. Under the assumption that clusters can be described by the so-called universal pressure profile (UPP) and its associated mass scaling law, the full signal-to-noise ratio &gt; 4 sample spans the mass range 1.6&lt;M_500c_^UPP^/10^14^M_{sun}_&lt;9.1, with median M_500c_^UPP^=3.1x10^14^M_{sun}_. The sample covers the redshift range 0.1&lt;z&lt;1.4 (median z=0.49), and 28 clusters are new discoveries (median z=0.80). We compare our catalog with other overlapping cluster samples selected using the SZ, optical, and X-ray wavelengths. We find that the ratio of the UPP-based SZ mass to richness-based weak-lensing mass is &lt;M_500c_^UPP^&gt;/&lt;M_500c_^{lambda}WL^&gt;=0.68+/-0.11. After applying this calibration, the mass distribution for clusters with M_500c_&gt;4x10^14^M_{sun}_ is consistent with the number of such clusters found in the South Pole Telescope SZ survey.</description><source format="bibcode">2018ApJS..235...20H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/235/20</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/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/103">VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/359">II/359 : The VISTA Hemisphere Survey (VHS) catalog DR4.1 (McMahon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/367">II/367 : The VISTA Hemisphere Survey (VHS) catalog DR5 (McMahon+, 2020)</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/J/MNRAS/274/75">J/MNRAS/274/75 : z of ROSAT X-ray brightest clusters (Crawford+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/129/435">J/ApJS/129/435 : NORAS galaxy cluster survey. 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(1=match) (RMMatch)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AName</name><description>Closest match listed on NED</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>RABdeg</name><description>BCG right ascension (J2000) (BCG_RADeg)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG declination (J2000) (BCG_decDeg)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>z</name><description>[0.1/1.4] "Best" redshift of the cluster</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_z</name><description>[0.02/0.15]? zphot uncertainty (zErr)</description><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_z</name><description>Note on z: "spec" (147 occurrences) or "phot" (35 occurrences) (zType)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>r_z</name><description>Reference on z (zSource) (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>delSDSS</name><description>[0.6/21.4]? zCluster density contrast statistic using SDSS photometry, {delta}SDSS (deltaSDSS) (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_delSDSS</name><description>[0.1/3.5]? delSDSS uncertainty (deltaSDSS_err)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>delS82</name><description>[1/78]? zCluster density contrast statistic using S82 photometry, {delta}S82 (deltaS82) (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_delS82</name><description>[0.1/32]? delS82 uncertainty (deltaS82_err)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>delCFHT</name><description>[0.7/14]? zCluster density contrast statistic using CFHTLenS photometry, {delta}CFHT (deltaCFHT) (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_delCFHT</name><description>[0.04/0.6]? delCFHT uncertainty (deltaCFHT_err)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>delSOAR</name><description>[2.8/36]? zCluster density contrast statistic using APO/SOAR photometry, {delta}SOAR (deltaSOAR) (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_delSOAR</name><description>[0.5/4]? delSOAR uncertainty (deltaSOAR_err)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M500cUPP</name><description>[1.6/9.1] Mass measured with respect to the critical density at the cluster redshift; corrected for the bias due to the steepness of the halo mass function (3)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500cUPP</name><description>[0.3/1.7] Positive 1-sigma error on M500cUPP (M500cUPP_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500cUPP</name><description>[0.2/1.4] Negative 1-sigma error on M500cUPP (M500cUPP_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500cUnc</name><description>[1.8/10.5] Mass measured with respect to the critical density at the cluster redshift; uncorrected (3)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500cUnc</name><description>[0.39/2.1] Positive 1-sigma error on M500cUnc (M500cUnc_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>[0.3/1.7] Negative 1-sigma error on M500cUnc (M500cUnc_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M200mUPP</name><description>[2.8/16.1] Mass measured with respect to the mean density at the cluster redshift; corrected for the bias due to the steepness of the halo mass function (3)(4)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M200mUPP</name><description>[0.5/3.2] Positive 1-sigma error on M200mUPP (M200mUPP_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M200mUPP</name><description>[0.4/2.7] Negative 1-sigma error on M200mUPP (M200mUPP_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M200mUnc</name><description>[3/18.5] Mass measured with respect to the mean density at the cluster redshift; uncorrected (3)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M200mUnc</name><description>[0.6/4] Positive 1-sigma error on M200mUnc (M200mUnc_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>[0.5/3.3] Negative 1-sigma error on M200mUnc (M200mUnc_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500cCal</name><description>[2.4/13.4] M_500c_^UPP^ rescaled rescaled by the richness-based weak-lensing mass calibration factor of 1/0.68 (see Section 6.1) (3)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_M500cCal</name><description>[0.6/3.1] Positive 1-sigma error on M500cCal (M500cCal_errPlus)</description><unit>1e+14solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M500cCal</name><description>[0.5/3] Negative 1-sigma error on M500cCal (M500cCal_errMinus)</description><unit>1e+14solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>