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<ri:Resource created="2023-04-27T15:28:40Z" 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>Sub-Chandrasekhar progenitors for Type Ia SNe</title><shortName>J/MNRAS/491/2902</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/491/2902</identifier><altIdentifier>doi:10.26093/cds/vizier.74912902</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Flors A.</name></creator><creator><name>Spyromilio J.</name></creator><creator><name>Taubenberger S.</name></creator><creator><name>Blondin S.</name></creator><creator><name>Cartier R.,Leibundgut B.</name></creator><creator><name>Dessart L.</name></creator><creator><name>Dhawan S.</name></creator><creator><name>Hillebrandt W.</name></creator><date role="Updated">2024-08-20T20:14:37Z</date><date role="Created">2023-04-27T15:28:40Z</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>spectroscopy</subject><subject>infrared-astronomy</subject><subject>chemically-peculiar-stars</subject><description>A non-local-thermodynamic-equilibrium level population model of the first and second ionization stages of iron, nickel, and cobalt is used to fit a sample of XShooter optical + near-infrared (NIR) spectra of Type Ia supernovae (SNe Ia). From the ratio of the NIR lines to the optical lines limits can be placed on the temperature and density of the emission region. We find a similar evolution of these parameters across our sample. Using the evolution of the FeII 12570-7155{AA} line as a prior in fits of spectra covering only the optical wavelengths we show that the 7200{AA} feature is fully explained by [FeII] and [NiII] alone. This approach allows us to determine the abundance of NiII/FeII for a large sample of 130 optical spectra of 58 SNe Ia with uncertainties small enough to distinguish between Chandrasekhar mass (M_Ch_) and sub-Chandrasekhar mass (sub-M_Ch_) explosion models. We conclude that the majority (85 per cent) of normal SNe Ia have a Ni/Fe abundance that is in agreement with predictions of sub-M_Ch_ explosion simulations of ~Z_{sun}_ progenitors. Only a small fraction (11 per cent) of objects in the sample have a Ni/Fe abundance in agreement with M_Ch_ explosion models.</description><source format="bibcode">2020MNRAS.491.2902F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/491/2902</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>IsServedBy</relationshipType><relatedResource>Conesearch 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/MNRAS/491/2902</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/491/2902</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/491/2902</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/491/2902</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/491/2902</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/491/2902</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 xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/491/2902/tableb1 (Overview of spectra observations)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/491/2902/tableb1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/491/2902/tableb1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/491/2902/tableb1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>190.7361667</ra><dec>13.2565</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/611 4149 4447 4719 5975 7606 11434 11496 12455 13907 15056 17340 17741 17761 18011 18325 18854 21300 22650 23077 23349 24920 24926 25344 25353 25571 25770 25960 26309 26336 27367 27426 27512 27738 27918 28035 28294 28299 31158 31230 34493 34531 34534 35885 36045 36391 37429 38655 38664 38956 40424 43339 44000 44915 46104 46399 48665</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/491/2902?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/491/2902/tableb1</name><description>Overview of spectra observations</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType><flag>nullable</flag></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</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>Name</name><description>Supernova name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Subtype</name><description>Supernova subtype (Ia-norm or 91T-like)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>E(B-V)</name><description>B-V colour excess</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Datemax</name><description>Date of B-band maximum</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Epoch</name><description>Epoch of the observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>Telescope used for the observation</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Inst</name><description>Instrument used for the observation</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Refsp</name><description>Reference for the spectra</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Refext</name><description>? Other reference</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Ni/Feinf</name><description>Ni/Fe mass ratio in the limit t-&gt;{infty}</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Ni/Feinf</name><description>Upper error on Ni/Feinf</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ni/Feinf</name><description>Lower error on Ni/Feinf</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/491/2902/refs</name><description>References for Table B1</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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