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<ri:Resource created="2024-04-05T09:21:17Z" 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>Subaru/HDS spectra of V5669 Sgr</title><shortName>J/ApJ/916/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/916/44</identifier><altIdentifier>doi:10.26093/cds/vizier.19160044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Arai A.</name></creator><creator><name>Tajitsu A.</name></creator><creator><name>Kawakita H.</name></creator><creator><name>Shinnaka Y.</name></creator><date role="Updated">2024-11-06T20:23:17Z</date><date role="Created">2024-04-05T09:21:17Z</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>novae</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><description>We report the new detection of ^7^BeII in the ultraviolet spectra of V5669 Sgr during its early decline phase (+24 and +28d). We identified three blueshifted absorption systems in our spectra. The first two, referred to as low- and high-velocity components, were noticeably identified among HI Balmer, NaI D, and FeII whose lower energies of transients are low (&lt;4eV). The third absorption component was identified among NII, HeI, and CII lines whose lower energy levels are relatively high (9-21eV). The absorption lines of ^7^BeII at 3130.583{AA} and 3132.228{AA} were identified as the first and second components in our observations. No evidence suggested the existence of LiI at 6708{AA} in any velocity components. The estimated number density ratio of lithium relative to hydrogen, which was finally produced by this object using the equivalent widths of ^7^Be and CaII K, N(^7^Li)/N(H)_final_, is 4.0+/-0.7x10^-6^. This value is an order of magnitude lower than the average observed values for classical novae wherein 7Be has been detected, and is comparable to the most optimistic value of theoretical predictions.</description><source format="bibcode">2021ApJ...916...44A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/916/44</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/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/6155">J/other/IBVS/6155 : 81th name-list of variable stars. II. (Kazarovets+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/830/30">J/ApJ/830/30 : HDS spectrum of nova V2659 Cyg (Nova Cyg 2014) (Arai+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/910/120">J/ApJ/910/120 : Dwarf nova outbursts detected by ASAS-SN (Kawash+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/647/A169">J/A+A/647/A169 : VVV survey near-infrared colour catalogue (Herpich+, 2021)</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/ApJ/916/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/916/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/916/44</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/916/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/916/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/916/44</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><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/ApJ/916/44</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/916/44/table2</name><description>Journal of observations of V5669 Sgr by Subaru/HDS</description><column><name>MJD</name><description>[57318.19/57322.22] Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>t</name><description>[24.09/28.12] Days after t_max_ (2015 Sep 29.1; MJD57294.1)</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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