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<ri:Resource created="2013-09-06T14:53:06Z" 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>Soft X-ray emission of Type Ia SN progenitors</title><shortName>J/MNRAS/426/2668</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/426/2668</identifier><altIdentifier>doi:10.26093/cds/vizier.74262668</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nielsen M.T.B.</name></creator><creator><name>Voss R.</name></creator><creator><name>Nelemans G.</name></creator><date role="Updated">2024-07-19T20:16:39Z</date><date role="Created">2013-09-06T14:53:06Z</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>x-ray-sources</subject><description>We present an analysis of Chandra observations of the position of 10 nearby (&lt;25Mpc) Type Ia supernovae, taken before the explosions. No sources corresponding to progenitors were found in any of the observations. We calculated upper limits on the bolometric luminosities of the progenitors assuming blackbody X-ray spectra with temperatures of 30-150eV. This is inspired by the fact that luminous super-soft X-ray sources have been suggested as the direct progenitors of Type Ia supernovae. The upper limits of two supernovae in our sample are comparable to the luminosities of the brightest observed super-soft sources, ruling out such sources as the progenitors of these supernovae. In contrast to Liu et al. (2012ApJ...749..141L), we find that for SN2011fe we can rule out Eddington luminosity systems for blackbody temperatures as low as 40eV. Our findings are consistent with statistical studies comparing the observed Type Ia supernova rate to the number of super-soft sources or the integrated X-ray luminosity in external galaxies. This suggests that either the progenitors of Type Ia supernovae are not accreting, nuclear burning white dwarfs or that they do not look like the classical super-soft sources, e.g. because they are obscured.</description><source format="bibcode">2012MNRAS.426.2668N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/426/2668</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><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2013)</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/426/2668</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/426/2668</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/426/2668</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/426/2668</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/426/2668</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/426/2668</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/426/2668/SNe (List of studied SNe with upper limit bolometric luminosities (tables 1 and 3 of the paper))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/426/2668/SNe?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/426/2668/SNe?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/426/2668/SNe?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>154.5153333</ra><dec>21.835</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/426/2668/table2 (Chandra observations used in this study. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SN</name><description>Supernova name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</flag></column><column><name>n_SN</name><description>[*] SN 2011fe has 2 entries with 2 NH values</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Gal</name><description>Host galaxy name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Dist</name><description>Distance</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_NH</name><description>Reference for NH</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="39*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>t.exp</name><description>Chandra exposure time</description><unit>ks</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_t.exp</name><description>[b] Total exposure time is given for the combined image (several observations)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ct</name><description>[0/44] Chandra counts (0.3-1keV) in source region</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Emap30</name><description>Value of exposure map at position at 30eV</description><unit>s.cm**2</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lbol30</name><description>Unabsorbed 3{sigma} upper limit bolometric luminosity at 30eV (erg/s)</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Emap50</name><description>Value of exposure map at position at 50eV</description><unit>s.cm**2</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lbol50</name><description>Unabsorbed 3{sigma} upper limit bolometric luminosity at 50eV (erg/s)</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Emap100</name><description>Value of exposure map at position at 100eV</description><unit>s.cm**2</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lbol100</name><description>Unabsorbed 3{sigma} upper limit bolometric luminosity at 100eV (erg/s)</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Emap150</name><description>Value of exposure map at position at 150eV</description><unit>s.cm**2</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lbol150</name><description>Unabsorbed 3{sigma} upper limit bolometric luminosity at 150eV (erg/s)</description><unit>1e-07W</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/426/2668/table2</name><description>Chandra observations used in this study. 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