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<ri:Resource created="2016-01-26T07:19:24Z" 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>JK photometry of NGC 2808</title><shortName>J/A+A/586/A51</shortName><identifier>ivo://CDS.VizieR/J/A+A/586/A51</identifier><altIdentifier>doi:10.26093/cds/vizier.35860051</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Massari D.</name></creator><creator><name>Fiorentino G.</name></creator><creator><name>McConnachie A.</name></creator><creator><name>Bono G.</name></creator><creator><name>Dall'Ora M.,Ferraro I.</name></creator><creator><name>Iannicola G.</name></creator><creator><name>Stetson P.B.</name></creator><creator><name>Turri P.</name></creator><creator><name>Tolstoy E.</name></creator><date role="Updated">2016-01-26T06:19:48Z</date><date role="Created">2016-01-26T07:19:24Z</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>globular-star-clusters</subject><subject>infrared-photometry</subject><description>Globular clusters are the oldest stellar systems in the Milky Way, and they probe the early epoch of the Galaxy formation. However, the uncertainties on their absolute age are still too large to soundly constrain how the Galactic structures have assembled. The aim of this work is to obtain an accurate estimate of the absolute age of the globular cluster NGC 2808 using deep IR data obtained with the multi-conjugate adaptive optics system operating at the Gemini South telescope (GeMS). This exquisite photometry, combined with that obtained in V and I-bands with HST, allowed us to detect the faint Main Sequence Knee feature in NGC 2808 colour magnitude diagram. 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