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<ri:Resource created="2019-09-23T09:37:25Z" 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>SN2016hnk photometry and spectroscopy</title><shortName>J/A+A/630/A76</shortName><identifier>ivo://CDS.VizieR/J/A+A/630/A76</identifier><altIdentifier>doi:10.26093/cds/vizier.36300076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Galbany L.</name></creator><creator><name>Ashall C.</name></creator><creator><name>Hoeflich P.</name></creator><creator><name>Gonzalez-Gaitan S.</name></creator><creator><name>Taubenberger S.,Stritzinger M.</name></creator><creator><name>Hsiao E.Y.</name></creator><creator><name>Mazzali P.</name></creator><creator><name>Baron E.</name></creator><creator><name>Blondin S.</name></creator><creator><name>Bose S.,Bulla M.</name></creator><creator><name>Burke J.F.</name></creator><creator><name>Burns C.R.</name></creator><creator><name>Cartier R.</name></creator><creator><name>Chen P.</name></creator><creator><name>Della Valle M.,Diamond T.R.</name></creator><creator><name>Gutierrez C.P.</name></creator><creator><name>Harmanen J.</name></creator><creator><name>Hiramatsu D.</name></creator><creator><name>Holoien T.W.-S,Hosseinzadeh G.</name></creator><creator><name>Howell D.A.</name></creator><creator><name>Huang Y.</name></creator><creator><name>Inserra C.</name></creator><creator><name>de Jaeger T.</name></creator><creator><name>Jha S.W.,Kangas T.</name></creator><creator><name>Kromer M.</name></creator><creator><name>Lyman J.D.</name></creator><creator><name>Maguire K.</name></creator><creator><name>Howie Marion G.,Milisavljevic D.</name></creator><creator><name>Prentice S.J.</name></creator><creator><name>Razza A.</name></creator><creator><name>Reynolds T.M.</name></creator><creator><name>Sand D.J.,Shappee B.J.</name></creator><creator><name>Shekhar R.</name></creator><creator><name>Smartt S.J.</name></creator><creator><name>Stassun K.G.</name></creator><creator><name>Sullivan M.,Valenti S.</name></creator><creator><name>Villanueva S.</name></creator><creator><name>Wang X.</name></creator><creator><name>Craig Wheeler J.</name></creator><creator><name>Zhai Q.</name></creator><creator><name>Zhang J.</name></creator><date role="Updated">2022-05-11T09:16:00Z</date><date role="Created">2019-09-23T09:37:25Z</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>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>infrared-photometry</subject><subject>spectroscopy</subject><subject>line-intensities</subject><description>We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of its host galaxy, MCG -01-06-070, and nearby environment. Our goal with this complete dataset is to understand the nature of this peculiar object. Methods: Properties of the SN local environment are characterized by means of single stellar population synthesis applied to IFS observations taken two years after the SN exploded. We performed detailed analyses of SN photometric data by studying its peculiar light and color curves. SN 2016hnk spectra were compared to other 1991bg-like SNe Ia, 2002es-like SNe Ia, and Ca-rich transients. In addition, we used abundance stratification modeling to identify the various spectral features in the early phase spectral sequence and also compared the dataset to a modified non-LTE model previously produced for the subluminous SN1999by. Results: SN 2016hnk is consistent with being a subluminous (MB=-16.7mag, sBV=0.43+/-0.03), highly reddened object. The IFS of its host galaxy reveals both a significant amount of dust at the SN location, residual star formation, and a high proportion of old stellar populations in the local environment compared to other locations in the galaxy, which favors an old progenitor for SN 2016hnk. Inspection of a nebular spectrum obtained one year after maximum contains two narrow emission lines attributed to the forbidden [CaII] {lambda}{lambda}7291,7324 doublet with a Doppler shift of 700km/s. Based on various observational diagnostics, we argue that the progenitor of SN 2016hnk was likely a near Chandrasekhar-mass (MCh) carbon-oxygen white dwarf that produced 0.108M_{sun}_ of 56 Ni. Our modeling suggests that the narrow [CaII] features observed in the nebular spectrum are associated with 48 Ca from electron capture during the explosion, which is expected to occur only in white dwarfs that explode near or at the MCh limit.</description><source format="bibcode">2019A&amp;A...630A..76G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/630/A76</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/630/A76</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/630/A76</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/630/A76</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/630/A76</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/630/A76</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/630/A76</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><spectral>7.952274030004205e-20 4.920466254354166e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/630/A76/tablec1</name><description>ASASSN V-band photometry and upper limits</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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SiII6355 pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WOI</name><description>? OI pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WOI</name><description>? OI pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WCaIINIR</name><description>? CaIINIR pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WCaIINIR</name><description>? CaIINIR pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>Epoch</name><description>B-band rest-frame epoch</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WCaIIHK</name><description>? CaIIHK pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WCaIIHK</name><description>? CaIIHK pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WFeII</name><description>? FeII pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WFeII</name><description>? FeII pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WSIIW1</name><description>? SIIW1 pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WSIIW1</name><description>? SIIW1 pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WSIIW2</name><description>? SIIW2 pseudo equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_WSIIW2</name><description>? SIIW2 pseudo equivalent width error</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>