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<ri:Resource created="2026-05-28T08:42:47Z" status="active" updated="2026-07-07T00:00:00Z" 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>redMaPPer clusters with ident. substructure</title><shortName>J/A+A/710/A57</shortName><identifier>ivo://CDS.VizieR/J/A+A/710/A57</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tuomainen R.</name></creator><creator><name>Finoguenov A.</name></creator><creator><name>Comparat J.</name></creator><creator><name>Doubrawa L.</name></creator><date role="Updated">2026-05-28T07:43:42Z</date><date role="Created">2026-05-28T08:42:47Z</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>visible-astronomy</subject><subject>redshifted</subject><description>Numerical simulations of hierarchical structure formation predict that galaxy clusters retain significant dark matter substructure, a signature of their ongoing assembly. This substructure is traced by both the spatial distribution of member galaxies and perturbations in the hot intracluster medium. Merging events significantly impact the thermodynamic state of clusters, introducing scatter in observable mass scaling relations and thereby affecting their use as precision cosmology probes. We statistically quantified the prevalence and properties of substructure in optical galaxy clusters and directly investigated its impact on X-ray morphology and scaling relations, leveraging new data from the DECaLS Legacy Survey and the SRG/eROSITA all-sky survey. We applied the hierarchical density-based clustering algorithm HDBSCAN to the redMaPPer galaxy cluster catalog to identify and characterize substructure from the probabilistic membership assignments. This provides a refined membership catalog and a classification of each cluster as containing substructure or not. We then cross-matched this sample with the eROSITA X-ray morphology catalog to correlate optical substructure with a comprehensive set of X-ray morphological parameters. Finally, we analyzed the scaling relation between X-ray luminosity and optical richness for clusters with and without substructure. Substructure is a common feature, present in approximately 40% of clusters; a quarter of the full sample exhibits a fractional contribution to richness in excess of 35%. We find a highly significant correlation between optical substructure and disturbed X-ray morphologies, a trend that is strongest for high-mass clusters. The clusters with substructure also drive a stronger redshift evolution in the scatter of the Lx-{lambda} relation. At low redshifts (z&lt;0.2), they display a systematically higher X-ray luminosity at fixed richness compared to relaxed systems. We demonstrate that substructure identification with redMaPPer is viable and essential for enhancing the precision of cluster cosmology. We attribute the enhanced effect of mergers on X-ray properties at low redshifts to the increased density contrast of low-redshift cool cores and longer substructure survival times, which are possibly due to the suppression of disruptive mixing by effects such as magnetic draping. At lower cluster richness, a discordance between X-ray morphology and the merging state indicates a growing relative importance of active galactic nucleus feedback in governing X-ray morphology.</description><source format="bibcode">2026A&amp;A...710A..57T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/710/A57</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/685/A106">J/A+A/685/A106 : eRASS. 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46071 46080 46087 46092 46100-46101 46108 46115 46127 46160 46166 46179 46196 46224 46235 46242 46252 46254 46258 46264 46272-46273 46277 46312 46314 46316 46326 46328 46332 46342 46364 46368-46369 46376 46378 46380-46382 46385 46387-46389 46396 46434-46435 46444 46459 46471 46492 46499 46516 46535 46540 46595 46609 46611-46612 46632 46637 46660 46673 46677 46694 46739 46752 46754 47153 47165 47168 47177 47188 47204 47217 47221 47225 47314 47317 47319-47320 47327 47358-47360 47390 47404-47405 47409 47418 47420 47489 47491 47511 47533 47708</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/710/A57?format=ascii</footprint><waveband>X-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/710/A57/main</name><description>redMaPPer clusters with identified substructure</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>Name</name><description>1eRASS Name (IAUNAME)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>DetUID</name><description>eROSITA detection id</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="32*">char</dataType></column><column><name>RAJ2000</name><description>X-ray cluster center right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>X-ray cluster center declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z1</name><description>Redshift of X-ray source</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Cluster</name><description>Cluster id</description><ucd>meta.id</ucd></column><column><name>RA2deg</name><description>Optical center right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DE2deg</name><description>Optical center declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>z2</name><description>Redshift of optical cluster</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Nsubcl</name><description>Number of subclusters (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>L500</name><description>0.2-2.3keV luminosity within R500 (in 10^42^erg/s)</description><unit>1e+35W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_L500</name><description>1sigma lower limit of L500 (in 10^42^erg/s)</description><unit>1e+35W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_L500</name><description>1sigma upper limit of L500 (in 10^42^erg/s)</description><unit>1e+35W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ScaleVal</name><description>Scaling value</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MaskFrac</name><description>Masking fraction</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>lambda</name><description>Optical richness</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_lambda</name><description>Richness error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mu</name><description>Mass ratio (2)</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/710/A57/members</name><description>Cluster member galaxy catalogue</description><column><name>Galaxy</name><description>Galaxy id</description><ucd>meta.id;meta.main</ucd></column><column><name>z</name><description>Cluster redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RAJ2000</name><description>Galaxy right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Galaxy declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>pvalue</name><description>redMaPPer p-value</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CG</name><description>[0/1] True (1) if a central galaxy</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>label</name><description>[0/8] Subcluster label</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Prob</name><description>HDBSCAN p-value</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">double</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>Cluster</name><description>Cluster id</description><ucd>meta.id.parent</ucd></column></table></schema></tableset></ri:Resource>