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<ri:Resource created="2025-07-17T09:14:52Z" status="active" updated="2025-08-01T20:03:15Z" 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>Metallicities of old open clusters</title><shortName>J/A+A/699/A246</shortName><identifier>ivo://CDS.VizieR/J/A+A/699/A246</identifier><altIdentifier>doi:10.26093/cds/vizier.36990246</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hu Q</name></creator><creator><name>Soubiran C.</name></creator><date role="Updated">2025-08-01T20:03:15Z</date><date role="Created">2025-07-17T09:14:52Z</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>milky-way-galaxy</subject><subject>open-star-clusters</subject><subject>metallicity</subject><description>We determined precise and homogeneous metallicities for old open clusters (&gt;=500Myr) from all-sky catalogues of stellar parameters leveraging Gaia spectrophotometry. Our purpose was to revisit the metallicity distribution of the oldest open clusters as a function of their Galactic position and age with improved statistics. Several catalogues of stellar parameters have been cross-matched to the most recent census of open clusters and their members. Median metallicities per cluster and per catalogue were evaluated by comparison to high-resolution spectroscopy. Our sample includes 1113 open clusters. A typical precision of 0.05dex is achieved for a subsample of nearly 600 clusters when only their bright red giants are considered. Metal-rich and metal-poor clusters never studied before are presented, as well as remnants of dissolving clusters. Galactic maps show a smooth decrease of metallicity from inside to outside the disc. We measured the radial and vertical gradients, their evolution with time and the age-metallicity relation in bins of Galactocentric distance.</description><source format="bibcode">2025A&amp;A...699A.246H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/A246</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/I/354">I/354 : StarHorse2, Gaia EDR3 photo-astrometric dist. (Anders+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/160">V/160 : SHBoost 2024 (Khalatyan+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/618/A93">J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/167/12">J/AJ/167/12 : Open cluster parameters with ANN (Cavallo+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/686/A42">J/A+A/686/A42 : Improving the open cluster census. III. 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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 name adopted from Cavallo et al., (2024, Cat. J/AJ/167/12)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>RA_ICRS</name><description>Right Ascension (ICRS) at Ep=J2000</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=J2000</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>MA22</name><description>? Median metallicity from Anders et al., (2022, Cat. Cat. I/354)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MA22</name><description>? Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NA22</name><description>? Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MA23f</name><description>Median metallicity from Andrae et al., (2023ApJS..267....8A) (1)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_MA23f</name><description>Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NA23f</name><description>Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MA23g</name><description>? Median metallicity from Andrae et al., (2023ApJS..267....8A) (2)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MA23g</name><description>? Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NA23g</name><description>? Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MZ23</name><description>? Median metallicity from Zhang et al. (2023MNRAS.524.1855)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MZ23</name><description>? Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NZ23</name><description>? Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MK24</name><description>? Median metallicity from Khalatyan et al., (2024, Cat. V/160)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MK24</name><description>? Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NK24</name><description>? Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MF24</name><description>? Median metallicity from Fallows et al., (2024MNRAS.531.2126F)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_MF24</name><description>? Metallicity uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NF24</name><description>? Number of considered members</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>