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<ri:Resource created="2022-05-18T13:37:43Z" 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>X-ray properties of eFEDS clusters and groups</title><shortName>J/A+A/661/A7</shortName><identifier>ivo://CDS.VizieR/J/A+A/661/A7</identifier><altIdentifier>doi:10.26093/cds/vizier.36610007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bahar Y.E.</name></creator><creator><name>Bulbul E.</name></creator><creator><name>Clerc N.</name></creator><creator><name>Ghirardini V.</name></creator><creator><name>Liu A.</name></creator><creator><name>Nandra K.,Pacaud F.</name></creator><creator><name>Chiu I-N.</name></creator><creator><name>Comparat J.</name></creator><creator><name>Ider-Chitham J.</name></creator><creator><name>Klein M.</name></creator><creator><name>Liu T.,Merloni A.</name></creator><creator><name>Migkas K.</name></creator><creator><name>Okabe N.</name></creator><creator><name>Ramos-Ceja M.E.</name></creator><creator><name>Reiprich T.H.,Sanders J.S.</name></creator><creator><name>Schrabback T.</name></creator><date role="Updated">2024-10-21T20:01:35Z</date><date role="Created">2022-05-18T13:37:43Z</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>surveys</subject><subject>x-ray-sources</subject><description>Scaling relations link the physical properties of clusters at cosmic scales. They are used to probe the evolution of large-scale structure, estimate observables of clusters, and constrain cosmological parameters through cluster counts. We investigate the scaling relations between X-ray observables of the clusters detected in the eFEDS field using Spectrum-Roentgen-Gamma/eROSITA observations taking into account the selection effects and the distributions of observables with cosmic time. We extract X-ray observables (Lx, Lbol, T, Mgas, Yx) within R500 for the sample of 542 clusters in the eFEDS field. By applying detection and extent likelihood cuts, we construct a subsample of 265 clusters with a contamination level of &lt;10% (including AGNs and spurious fluctuations) to be used in our scaling relations analysis. The selection function based on the state-of-the-art simulations of the eROSITA sky is fully accounted for in our work. We provide the X-ray observables in the core- included &lt;R500 and core-excised 0.15*R500-R500 apertures for 542 galaxy clusters and groups detected in the eFEDS field. Additionally, we present our best-fit results for the normalization, slope, redshift evolution, and intrinsic scatter parameters of the X-ray scaling relations between Lx-T, Lx- Mgas, Lx-Yx, Lbol-T, Lbol-Mgas, Lbol-Yx, and Mgas-T. We find that the best-fit slopes significantly deviate from the self-similar model at a &gt;4sigma confidence level, but our results are nevertheless in good agreement with the simulations including non-gravitational physics, and the recent results that take into account selection effects. The strong deviations we find from the self-similar scenario indicate that the non-gravitational effects play an important role in shaping the observed physical state of clusters. This work extends the scaling relations to the low-mass, low-luminosity galaxy cluster and group regime using eFEDS observations, demonstrating the ability of eROSITA to measure emission from the intracluster medium out to R500 with survey-depth exposures and constrain the scaling relations in a wide mass-luminosity-redshift range.</description><source format="bibcode">2022A&amp;A...661A...7B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/661/A7</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/661/A1">J/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A2">J/A+A/661/A2 : Galaxy clusters and groups in eFEDS (Liu+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A3">J/A+A/661/A3 : eFEDS counterparts to point-like sources (Salvato+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A4">J/A+A/661/A4 : eFEDS optical cluster and group catalog (Klein+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A5">J/A+A/661/A5 : The eFEDS AGN catalog (Liu+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A8">J/A+A/661/A8 : eFEDS catalogue of variable X-ray sources (Boller+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A10">J/A+A/661/A10 : eFEDS galaxy clusters and groups in disguise (Bulbul+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A23">J/A+A/661/A23 : Exoplanet X-ray irradiation &amp; 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