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<ri:Resource created="2019-07-31T14:28:32Z" 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>MARD-Y3 catalog</title><shortName>J/MNRAS/488/739</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/488/739</identifier><altIdentifier>doi:10.26093/cds/vizier.74880739</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Klein M.</name></creator><creator><name>Grandis S.</name></creator><creator><name>Mohr J.J.</name></creator><creator><name>Paulus M.</name></creator><creator><name>Abbott T.M.C.</name></creator><creator><name>Annis J.,Avila S.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Brooks D.</name></creator><creator><name>Buckley-Geer E.</name></creator><creator><name>Carnero Rosell A.,Carrasco Kind M.</name></creator><creator><name>Carretero J.</name></creator><creator><name>Castander F.J.</name></creator><creator><name>Cunha C.E.</name></creator><creator><name>D'Andrea C.B.,da Costa L.N.</name></creator><creator><name>De Vicente J.</name></creator><creator><name>Desai S.</name></creator><creator><name>Diehl H.T.</name></creator><creator><name>Dietrich J.P.</name></creator><creator><name>Doel P.,Evrard A.E.</name></creator><creator><name>Flaugher B.</name></creator><creator><name>Fosalba P.</name></creator><creator><name>Frieman J.</name></creator><creator><name>Garcia-Bellido J.,Gaztanaga E.</name></creator><creator><name>Giles P.A.</name></creator><creator><name>Gruen D.</name></creator><creator><name>Gruendl R.A.</name></creator><creator><name>Gschwend J.</name></creator><creator><name>Gutierrez G.,Hartley W.G.</name></creator><creator><name>Hollowood D.L.</name></creator><creator><name>Honscheid K.</name></creator><creator><name>Hoyle B.</name></creator><creator><name>James D.J.,Jeltema T.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Kuropatkin N.</name></creator><creator><name>Lima M.</name></creator><creator><name>Maia M.A.G.</name></creator><creator><name>March M.,Marshall J.L.</name></creator><creator><name>Menanteau F.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Ogando R.L.C.</name></creator><creator><name>Plazas A.A.,Romer A.K.</name></creator><creator><name>Roodman A.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Scarpine V.</name></creator><creator><name>Schindler R.</name></creator><creator><name>Serrano S.,Sevilla-Noarbe I.</name></creator><creator><name>Smith M.</name></creator><creator><name>Smith R.C.</name></creator><creator><name>Soares-Santos M.</name></creator><creator><name>Sobreira F.,Suchyta E.</name></creator><creator><name>Swanson M.E.C.</name></creator><creator><name>Tarle G.</name></creator><creator><name>Thomas D.</name></creator><creator><name>Vikram V.,DES Collaboration</name></creator><date role="Updated">2025-05-15T20:14:35Z</date><date role="Created">2019-07-31T14:28:32Z</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>x-ray-sources</subject><subject>redshifted</subject><description>We present the MARD-Y3 catalogue of between 1086 and 2171 galaxy clusters (52 per cent and 65 per cent new) produced using multicomponent matched filter (MCMF) follow-up in 5000 deg^2^ of DES-Y3 optical data of the ~20000 overlapping ROSAT All-Sky Survey source catalogue (2RXS) X-ray sources. Optical counterparts are identified as peaks in galaxy richness as a function of redshift along the line of sight towards each 2RXS source within a search region informed by an X-ray prior. All peaks are assigned a probability fcont of being a random superposition. The clusters lie at 0.02&lt;z&lt;1.1 with more than 100 clusters at z&gt;0.5. Residual contamination is 2.6 per cent and 9.6 per cent for the cuts adopted here. For each cluster we present the optical centre, redshift, rest frame X-ray luminosity, M500 mass, coincidence with NWAY infrared sources, and estimators of dynamical state. About ~2 per cent of MARD-Y3 clusters have multiple possible counterparts, the photo-z's are high quality with {sigma}{DELTA}z/(1+z)=0.0046, and ~1 per cent of clusters exhibit evidence of X-ray luminosity boosting from emission by cluster active galactic nuclei. Comparison with other catalogues (MCXC, RM, SPT-SZ, Planck) is performed to test consistency of richness, luminosity, and mass estimates. We measure the MARD-Y3 X-ray luminosity function and compare it to the expectation from a fiducial cosmology and externally calibrated luminosity- and richness-mass relations. Agreement is good, providing evidence that MARD-Y3 has low contamination and can be understood as a simple two step selection - X-ray and then optical - of an underlying cluster population described by the halo mass function.</description><source format="bibcode">2019MNRAS.488..739K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/488/739</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/J/A+A/588/A103">J/A+A/588/A103 : Second ROSAT all-sky survey (2RXS) source 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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>LFCRL</name><description>(raw) luminosity of best counter part (LUM_LFCR)</description><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LFCM500corr</name><description>Corrected M500 of best counter part (M500_LFCR_CORR)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Name</name><description>Name, MARDJHHMMSS.s+DDMMSS (NAME)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>RAJ2000</name><description>X-ray right ascension (J2000) from 2RXS (RA_DEG)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>X-ray declination (J2000) from 2RXS (DEC_DEG)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>ExpTime</name><description>RASS exposure time (EXPOSURE)</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Cts</name><description>X-ray source counts (CTS)</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Cts</name><description>Error on counts (CERR)</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CRate</name><description>X-ray count rate (RATE)</description><unit>ct/s</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_CRate</name><description>Error on the rate (ERATE)</description><unit>ct/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ext</name><description>X-ray extend [PIX] (EXT)</description><unit>pix</unit><ucd>instr.fov;instr.pixel</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ext</name><description>Error on extend (EXTERR)</description><unit>pix</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ExtML</name><description>Extend likelihood (EXT_ML)</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExiML</name><description>Existence likelihood (EXI_ML)</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zP1</name><description>Redshift P1 (Z_P1)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zP2</name><description>? Redshift P2 (Z_P2)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>zP3</name><description>? Redshift P3 (Z_P3)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LambdaP1</name><description>Richness P1 (LAMBDA_P1)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LambdaP2</name><description>? Richness P2 (LAMBDA_P2)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LambdaP3</name><description>? Richness P3 (LAMBDA_P3)</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAP1deg</name><description>? Optical right ascension of P1 (J2000) (RA_P1)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>RAP2deg</name><description>? Optical right ascension of P2 (J2000) (RA_P2)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>RAP3deg</name><description>? Optical right ascension of P3 (J2000) (RA_P3)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEP1deg</name><description>? Optical declination of P1 (J2000) (DEC_P1)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>DEP2deg</name><description>? Optical declination of P2 (J2000) (DEC_P2)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>DEP3deg</name><description>? Optical declination of P3 (J2000) (DEC_P3)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>fMult</name><description>[0/1] 1 for multiple detection in X-rays, 0 else (MULTIPLE_FLAG)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>P1Lcorr</name><description>Corrected luminosity P1 (LUM_P1_CORR)</description><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>P2Lcorr</name><description>? Corrected luminosity P2 (LUM_P2_CORR)</description><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>P3Lcorr</name><description>? Corrected luminosity P3 (LUM_P3_CORR)</description><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>P1M500corr</name><description>Corrected mass M_500 P1 (M500_P1_CORR)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>P2M500corr</name><description>? Corrected mass M_500 P2 (M500_P2_CORR)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>P3M500corr</name><description>? Corrected mass M_500 P3 (M500_P3_CORR)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LambdaP1</name><description>Error on richness P1 (E_LAMBDA_P1)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LambdaP2</name><description>? Error on richness P2 (E_LAMBDA_P2)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LambdaP3</name><description>? Error on richness P3 (E_LAMBDA_P3)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LambdaLFCR</name><description>Error on richness for best counter part (E_LAMBDA_LFCR)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LambdaLFCR</name><description>Richness of best counter part (LAMBDA_LFCR)</description><ucd>meta.id.part;src.class.richness;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FcontP1</name><description>Probability f_cont_ of being a random superposition for P1 (F_CONT_R_P1)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FcontP2</name><description>? Probability f_cont_ of being a random superposition for P2 (F_CONT_R_P2)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FcontP3</name><description>? Probability f_cont_ of being a random superposition for P3 (F_CONT_R_P3)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>zLFCR</name><description>Redshift of best counter part (Z_LFCR)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FcontLFCR</name><description>Probability f_cont_ of being a random superposition of best counter part (F_CONT_LFCR)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LFCM500</name><description>(raw) M500 of best counter part (M500_LFCR)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LFCRLcorr</name><description>Corrected luminosity of best counter part (LUM_LFCR_CORR)</description><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RALFCRdeg</name><description>? RA (optical) of best counter part (J2000) (RA_LFCR)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DELFCRdeg</name><description>? DEC (optical) of best counter part (J2000) (DEC_LFCR)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>DsigLFCR</name><description>? Distance from mean scaling for WISE matches (D_SIG_LFCR)</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DfcLFCR</name><description>Difference lowest to second lowest f_cont (DFC_LFCR)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>2RXS</name><description>Display the 2RXS data (Boller et al. 2916, Cat. J/A+A/588/A103</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>