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<ri:Resource created="2026-06-03T08:01:11Z" status="active" updated="2026-07-08T07:16:58Z" 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>X-CLASS low z groups and galaxy clusters</title><shortName>J/A+A/710/A77</shortName><identifier>ivo://CDS.VizieR/J/A+A/710/A77</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moysan Q.</name></creator><creator><name>Sarron F.</name></creator><creator><name>Clerc N.</name></creator><creator><name>Soucail G.</name></creator><creator><name>Adami C.</name></creator><creator><name>Altieri B.,Cabanac R.</name></creator><creator><name>Chira M.</name></creator><creator><name>Comparat J.</name></creator><creator><name>Coia D.</name></creator><creator><name>Drigga E.</name></creator><creator><name>Gaynullina E.,Khalikova A.</name></creator><creator><name>Koulouridis E.</name></creator><creator><name>Migkas K.</name></creator><creator><name>Molham M.</name></creator><creator><name>Paquereau L.,Sadibekova T.</name></creator><creator><name>Valtchanov I.</name></creator><date role="Updated">2026-07-08T07:16:58Z</date><date role="Created">2026-06-03T08:01:11Z</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>x-ray-sources</subject><subject>galaxy-clusters</subject><subject>redshifted</subject><description>Properties of the hot intracluster and intragroup medium are mostly set by the underlying gravitational potential well, although complex astrophysical processes at play during their buildup may leave a significant imprint. Observational constraints on the degree and scales of such nongravitational processes require well-selected samples of objects and deep observations of their gas content. We aim to study the scaling relation between two global properties of the hot gas, namely its soft-band X-ray luminosity (L_X_) and its temperature (T), by studying a sample of low-mass systems associated with precise redshifts, simultaneously accounting for sample selection biases and associated measurement uncertainties. This work takes as input a large catalog of X-ray-selected galaxy clusters (X-CLASS). We performed a thorough revision of the redshifts of sources using deep photometric data from the Legacy Surveys and our own tailored spectroscopic follow-up of 52 low-redshift systems. We devised a spectroscopically complete sample of 155 low-redshift (0.07&lt;z&lt;0.2) systems, and we measured properties of their X-ray emitting gas, with median ^-^T=1.7keV and median ^-^L_X_=10^43^erg/s. We inferred the relation between L_X_ and T in a Bayesian framework. Our sample of groups and clusters with a median total mass of ~6x10^13^M_{sun}_ reveals a relation L_X_-T steeper than that predicted by the self-similar model, with a slope of B=3.2+/-0.1. This result fits well within recent studies that together indicate a trend of an increasing slope with decreasing median halo mass. This work supports a scenario of a stronger decrease in luminosity with decreasing mass in the group regime than for massive galaxy clusters. This effect is possibly due to strong and sustained feedback expelling gas efficiently from their shallower potential wells. We release the list of updated redshifts (photometric and spectroscopic) for the full X-CLASS sample and the gas properties of the low-redshift sample. The cluster photometric redshift code presented in the paper photXclus is made publicly available (https://codeberg.org/fsarron/photXclus).</description><source format="bibcode">2026A&amp;A...710A..77M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/710/A77</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/MNRAS/494/161">J/MNRAS/494/161 : The X-CLASS-redMaPPer galaxy cluster sample (Molham+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/652/A12">J/A+A/652/A12 : The new X-Class catalogue (Koulouridis+, 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Spectroscopic temperature measurement</description><unit>keV</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_T</name><description>? Spectroscopic temperature positive uncertainty</description><unit>keV</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_T</name><description>? Spectroscopic temperature negative uncertainty</description><unit>keV</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Z</name><description>? Metallicity measurement</description><unit>Sun</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>n_Z</name><description>[*] * indicates fixed metallicity</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>E_Z</name><description>? Metallicity positive uncertainty</description><unit>Sun</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Z</name><description>? Metallicity negative uncertainty</description><unit>Sun</unit><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>L500</name><description>? Luminosity L500 measurements in 10^42^erg/s</description><unit>1e+35W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_L500</name><description>? Luminosity L500 positive uncertainty in 10^42^erg/s</description><unit>1e+35W</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_L500</name><description>? Luminosity L500 negative uncertainty in 10^42^erg/s</description><unit>1e+35W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R500</name><description>? Radius R500 of the cluster derived from scaling relation</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>chi2/nu</name><description>Goodness of the backgroung estimation of the pointing</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>