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<ri:Resource created="1997-12-09T20:36:59Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>UBV Photometry of globular cluster NGC1841</title><shortName>J/AJ/112/2020</shortName><identifier>ivo://CDS.VizieR/J/AJ/112/2020</identifier><altIdentifier>doi:10.26093/cds/vizier.51122020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Alcaino G.</name></creator><creator><name>Liller W.</name></creator><creator><name>Alvarado F.</name></creator><creator><name>Kravtsov V.</name></creator><creator><name>Ipatov A.,Samus N.</name></creator><creator><name>Smirnov O.</name></creator><date role="Updated">2023-04-06T16:50:22Z</date><date role="Created">1997-12-09T20:36:59Z</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>ccd-photometry</subject><description>The observations were acquired in two nights, 1993 December 20-22, with the EMMI camera on the NTT telescope at ESO. The photometric limit is close to the cluster main-sequence turnoff; a comparison of the photometry with Walker (1990AJ....100.1532W) shows slight systematic differences . the present magnitudes being fainter by 0.03-0.05mag, and colors being bluer by 0.05mag. The estimated parameters of the populous globular cluster NGC 1841, located approximately 15deg from each of the Magellanic Clouds and probably dynamically associated with the LMC, are: [Fe/H] = -2.0 +/- 0.15 E(B-V) = 0.17 +/- 0.03 mag (m-M)_0_ = 18.26 +/- 0.11 mag (true distance modulus)</description><source format="bibcode">1996AJ....112.2020A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/112/2020</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/104/1063">J/PASP/104/1063 : BV Color-Magnitude Diagram for NGC 1851 (Walker 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/105/527">J/AJ/105/527 : RR Lyr stars in NGC 1835 (Walker 1993)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/112/2020</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/112/2020</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/112/2020</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/112/2020</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/112/2020</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/112/2020</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/112/2020/table3</name><description>The stars with photometry</description><column><name>B-V</name><description>B-V color</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U-B</name><description>? U-B color</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>[1/1347]+ Running number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag><flag>indexed</flag></column><column><name>x</name><description>*coordinate</description><unit>pix</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>y</name><description>*coordinate</description><unit>pix</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>