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<ri:Resource created="2025-02-18T15:59:40Z" status="active" updated="2025-07-18T20:17:18Z" 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>Membership probabilities of M 37 stars</title><shortName>J/MNRAS/511/4702</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/4702</identifier><altIdentifier>doi:10.26093/cds/vizier.75114702</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Griggio M.</name></creator><creator><name>Bedin L.R.</name></creator><date role="Updated">2025-07-18T20:17:18Z</date><date role="Created">2025-02-18T15:59:40Z</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>open-star-clusters</subject><subject>astronomical-models</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>astrometry</subject><description>In this work, starting from the well-accepted relations in literature, we introduce a new formalism to compute the astrometric membership probabilities for sources in star clusters, and we provide an application to the case of the open cluster M 37. The novelty of our approach is a refined - and magnitude- dependent - modelling of the parallax distribution of the field stars. We employ the here-derived list of members to estimate the cluster's mean systemic astrometric parameters, which are based on the most recent Gaia's catalogue (EDR3).</description><source format="bibcode">2022MNRAS.511.4702G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/4702</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/ApJ/908/L5">J/ApJ/908/L5 : Color-magnitude diagram for {omega} Centauri (Soltis+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/959">J/A+A/493/959 : UBV(RI)cHalpha photometry in omega Cen (Bellini+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/609">J/A+A/484/609 : BVI photometry and proper motions in M67 (Yadav+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/23">J/ApJ/856/23 : BANYAN. 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