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<ri:Resource created="2016-10-18T11:38:53Z" 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>BVRI LCs of type Ib supernova iPTF13bvn</title><shortName>J/ApJ/825/L22</shortName><identifier>ivo://CDS.VizieR/J/ApJ/825/L22</identifier><altIdentifier>doi:10.26093/cds/vizier.18259022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Folatelli G.</name></creator><creator><name>Van Dyk S.D.</name></creator><creator><name>Kuncarayakti H.</name></creator><creator><name>Maeda K.</name></creator><creator><name>Bersten M.C.,Nomoto K.</name></creator><creator><name>Pignata G.</name></creator><creator><name>Hamuy M.</name></creator><creator><name>Quimby R.M.</name></creator><creator><name>Zheng W.</name></creator><creator><name>Filippenko A.V.,Clubb K.I.</name></creator><creator><name>Smith N.</name></creator><creator><name>Elias-Rosa N.</name></creator><creator><name>Foley R.J.</name></creator><creator><name>Miller A.A.</name></creator><date role="Updated">2017-07-06T06:25:53Z</date><date role="Created">2016-10-18T11:38:53Z</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>supernovae</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>Supernova (SN) iPTF13bvn in NGC 5806 was the first Type Ib SN to have been tentatively associated with a progenitor in pre-explosion images. We performed deep ultraviolet (UV) and optical Hubble Space Telescope observations of the SN site ~740 days after explosion. We detect an object in the optical bands that is fainter than the pre-explosion object. This dimming is likely not produced by dust absorption in the ejecta; thus, our finding confirms the connection of the progenitor candidate with the SN. The object in our data is likely dominated by the fading SN, implying that the pre-SN flux is mostly due to the progenitor. We compare our revised pre-SN photometry with previously proposed models. Although binary progenitors are favored, models need to be refined. In particular, to comply with our deep UV detection limit, any companion star must be less luminous than a late-O star or substantially obscured by newly formed dust. A definitive progenitor characterization will require further observations to disentangle the contribution of a much fainter SN and its environment.</description><source format="bibcode">2016ApJ...825L..22F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/825/L22</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/A+A/580/A142">J/A+A/580/A142 : SN 2011dh. The first two years (Ergon+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/574/A60">J/A+A/574/A60 : Light curve templates of SNe Ib/c from SDSS (Taddia+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A12">J/A+A/573/A12 : SN1993J spectra 100-500d post-explosion (Jerkstrand+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A17">J/A+A/562/A17 : SN 2011dh - The first 100 days (Ergon+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/774">J/MNRAS/436/774 : Core collapse supernovae (type Ibc) (Eldridge+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A131">J/A+A/558/A131 : Model spectra of hot stars at the pre-SN stage (Groh+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/97">J/ApJ/741/97 : Light curves of Ibc supernovae (Drout+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/418">J/ApJS/190/418 : Light curves for 165 SNe (Ganeshalingam+, 2010)</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/825/L22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/825/L22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/825/L22</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/825/L22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/825/L22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/825/L22</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>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/825/L22/table3</name><description>KAIT and Nickel Photometry of iPTF13bvn</description><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>MJD</name><description>Modified Julian date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>Rest-frame phase (1)</description><unit>d</unit><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Bmag</name><description>Limit flag on Bmag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Bmag</name><description>[15.8/21.7] Apparent B band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Bmag</name><description>[0.05/0.5]? 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