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<ri:Resource created="2016-04-01T07:56:57Z" status="active" updated="2025-06-13T15:25:00Z" 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>Spectrophotometric time series obs. of twin SNIa</title><shortName>J/ApJ/815/58</shortName><identifier>ivo://CDS.VizieR/J/ApJ/815/58</identifier><altIdentifier>doi:10.26093/cds/vizier.18150058</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fakhouri H.K.</name></creator><creator><name>Boone K.</name></creator><creator><name>Aldering G.</name></creator><creator><name>Antilogus P.</name></creator><creator><name>Aragon C.</name></creator><creator><name>Bailey S.,Baltay C.</name></creator><creator><name>Barbary K.</name></creator><creator><name>Baugh D.</name></creator><creator><name>Bongard S.</name></creator><creator><name>Buton C.</name></creator><creator><name>Chen J.,Childress M.</name></creator><creator><name>Chotard N.</name></creator><creator><name>Copin Y.</name></creator><creator><name>Fagrelius P.</name></creator><creator><name>Feindt U.</name></creator><creator><name>Fleury M.,Fouchez D.</name></creator><creator><name>Gangler E.</name></creator><creator><name>Hayden B.</name></creator><creator><name>Kim A.G.</name></creator><creator><name>Kowalski M.</name></creator><creator><name>Leget P.-F.,Lombardo S.</name></creator><creator><name>Nordin J.</name></creator><creator><name>Pain R.</name></creator><creator><name>Pecontal E.</name></creator><creator><name>Pereira R.</name></creator><creator><name>Perlmutter S.,Rabinowitz D.</name></creator><creator><name>Ren J.</name></creator><creator><name>Rigault M.</name></creator><creator><name>Rubin D.</name></creator><creator><name>Runge K.</name></creator><creator><name>Saunders C.,Scalzo R.</name></creator><creator><name>Smadja G.</name></creator><creator><name>Sofiatti C.</name></creator><creator><name>Strovink M.</name></creator><creator><name>Suzuki N.</name></creator><creator><name>Tao C.,Thomas R.C.</name></creator><creator><name>Weaver B.A.</name></creator><creator><name>(the Nearby Supernova Factory)</name></creator><date role="Updated">2018-01-05T08:56:32Z</date><date role="Created">2016-04-01T07:56:57Z</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><description>We introduce a method for identifying "twin" Type Ia supernovae (SNeIa) and using them to improve distance measurements. This novel approach to SN Ia standardization is made possible by spectrophotometric time series observations from the Nearby Supernova Factory (SNfactory). We begin with a well-measured set of SNe, find pairs whose spectra match well across the entire optical window, and then test whether this leads to a smaller dispersion in their absolute brightnesses. This analysis is completed in a blinded fashion, ensuring that decisions made in implementing the method do not inadvertently bias the result. We find that pairs of SNe with more closely matched spectra indeed have reduced brightness dispersion. We are able to standardize this initial set of SNfactory SNe to 0.083+/-0.012mag, implying a dispersion of 0.072+/-0.010mag in the absence of peculiar velocities. We estimate that with larger numbers of comparison SNe, e.g., using the final SNfactory spectrophotometric data set as a reference, this method will be capable of standardizing high-redshift SNe to within 0.06-0.07mag. These results imply that at least 3/4 of the variance in Hubble residuals in current SN cosmology analyses is due to previously unaccounted-for astrophysical differences among the SNe.</description><source format="bibcode">2015ApJ...815...58F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/815/58</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/J/A+A/568/A22">J/A+A/568/A22 : Joint analysis of the SDSS-II &amp; SNLS SNe Ia (Betoule+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/3258">J/MNRAS/444/3258 : Velocities and EW of PTF SNe Ia (Maguire+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/438/1391">J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/107">J/ApJ/770/107 : Host galaxies of SNIa from SNfactory (Childress+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A8">J/A+A/549/A8 : Atmospheric extinction data above Mauna Kea (Buton+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. I. (Silverman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/99">J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/85">J/ApJ/746/85 : THe HST Cluster Supernova Survey. V. (Suzuki+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/L4">J/A+A/529/L4 : Reddening law of type Ia supernovae (Chotard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/120">J/ApJ/731/120 : Intrinsic SN Ia light curves (Mandel+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/1">J/ApJS/192/1 : Light-curve parameters from the SNLS (Conley+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/566">J/ApJ/722/566 : SNe Ia host galaxies in SDSS-II SN survey (Lampeitl+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/406/782">J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/L139">J/ApJ/699/L139 : Spectral parameters of SNe Ia (Wang+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/500/L17">J/A+A/500/L17 : Spectral flux ratio of SN Ia (Bailey+, 2009)</relatedResource><relatedResource>http://snfactory.lbl.gov/ : The Nearby Supernova Factory home page</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/815/58</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/815/58</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/815/58</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/815/58</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/815/58</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/815/58</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/ApJ/815/58/sne (List of the 49 supernovae in the final sample; table added by CDS)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/815/58/sne?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/815/58/sne?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/815/58/sne?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>326.625</ra><dec>6.4185833</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/166 4430 5999 8217 8344 8537 8573 8764 8788 9539 10040 10120 10144 10158 10401 11287 12349 13059 13334 13572 15096 17237 17315 17438 17513 17591 17644 17818 18017 19161 19187 19283 19387 19393 20051 20061 20080 21857 30174 31049 31418 32482 44635 44706 48346 48604 48925</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/815/58?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/815/58/table5</name><description>Full data for the best supernovae pairs from the near-maximum R_V_=3.1 analysis</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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