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<ri:Resource created="2026-09-23T08:47:34Z" status="active" updated="2026-09-23T07:47:58Z" 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>eRASS1-2MRS group catalog</title><shortName>J/A+A/713/A299</shortName><identifier>ivo://CDS.VizieR/J/A+A/713/A299</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Finoguenov A.</name></creator><creator><name>Seppi R.</name></creator><creator><name>Eckert D.</name></creator><creator><name>Khalil H.</name></creator><creator><name>Kosowski J.</name></creator><creator><name>Tempel E.,Gastaldello F.</name></creator><creator><name>Lovisari L.</name></creator><date role="Updated">2026-09-23T07:47:58Z</date><date role="Created">2026-09-23T08:47:34Z</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>Understanding baryonic physics at the scale of galaxy groups is essential for high-precision cosmological studies of the large-scale structure. Most models predict that the intergalactic medium in groups is hot and extends well beyond the virial radius, emitting X-rays on scales of up to several degrees in nearby systems. Early X-ray searches using ROSAT showed significant promise in recovering and identifying this emission. We aim to exploit the large area coverage, good sensitivity, and low instrumental background of eROSITA to detect the faint surface brightness emission of galaxy groups from the Two Micron All Sky Survey Redshift Survey (2MRS). Using the data from eROSITA-DE Data Release 1, including images, exposure maps, and local background maps, we performed a wavelet decomposition of image mosaics in the 0.6-2.3keV band at angular scales of 1/8'-16'. We adopted 8-16' scales for source detection and 2'-4' scales to improve catalog purity. A novel identification method based on the ranked partial Hausdorff distance fully exploits the X-ray image and group membership information. Random catalogs were used to control match purity, and the identification threshold was chosen to maximize the catalog size at a fixed purity. We present a catalog of 619 X-ray galaxy groups with 80% purity, and define subsamples with 90% and 97% purity. Bright sources closely match the AXES-2MRS catalog (which is based on ROSAT All Sky Survey data analysis on spatial scales of 12'-24'). The X-ray luminosity function of our groups agrees with previous studies down to 5x10^41^erg/s. Using dynamical mass estimates, we find that the X-ray counterpart completeness for groups with &gt;=4 members exceeds 60% for masses &gt;2e13 Msun. We modeled the 2MRS group catalog and justify the inclusion of two-member groups in the identification. This study demonstrates that large X-ray sources on spatial scales relevant for cosmological studies of baryonic distributions can be reliably detected and identified using nearby galaxy group catalogs.</description><source format="bibcode">2026A&amp;A...713A.299F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/713/A299</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/682/A34">J/A+A/682/A34 : SRG/eROSITA all-sky survey catalogs (eRASS1) (Merloni+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/688/A210">J/A+A/688/A210 : 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