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<ri:Resource created="2024-10-24T08:26:42Z" status="active" updated="2025-06-13T15:25:00Z" 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>UV &amp; opt. phot. &amp; spectra of Type Ia SN2011aa</title><shortName>J/ApJ/938/L22</shortName><identifier>ivo://CDS.VizieR/J/ApJ/938/L22</identifier><altIdentifier>doi:10.26093/cds/vizier.19389022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dutta A.</name></creator><creator><name>Anupama G.C.</name></creator><creator><name>Chakradhari N.K.</name></creator><creator><name>Sahu D.K.</name></creator><date role="Updated">2025-03-18T20:07:37Z</date><date role="Created">2024-10-24T08:26:42Z</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>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present optical observations and Monte Carlo radiative transfer modeling of the Type Ia supernova (SN Ia) SN 2011aa. With a {Delta}m_15_(B) of 0.59+/-0.07mag and a peak magnitude M_B_ of -19.30+/-0.27mag, SN 2011aa has the slowest decline rate among SNe Ia. The secondary maximum in the I band is absent or as equally bright as the primary maximum. The velocity of CII is lower than the velocity of SiII. This indicates either the presence of C at lower velocities than Si or a line-of-sight effect. Application of Arnett's radiation diffusion model to the bolometric light curve indicates a massive ejecta M_ej_ 1.8-2.6M_{sun}_. The slow decline rate and large ejecta mass, with a normal peak magnitude, are well explained by a double degenerate, violent merger explosion model. The synthetic spectra and light curves generated with SEDONA considering a violent merger density profile match the observations.</description><source format="bibcode">2022ApJ...938L..22D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/938/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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4517">J/AJ/137/4517 : UVOT light curves of supernovae (Brown+, 2009)</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/ApJ/748/L29">J/ApJ/748/L29 : SN Ia supernovae observed by Swift/XRT (Russell+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/2440">J/MNRAS/445/2440 : SN with associated Planck CMB temperatures (Yershov+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/29">J/ApJ/787/29 : UVOT phot. of Super-Chandrasekhar mass SNe Ia (Brown+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/795/142">J/ApJ/795/142 : Defining photometric peculiar SNe Ia (Gonzalez-Gaitan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/220/9">J/ApJS/220/9 : CfAIR2: NIR light curves of Type Ia SNe (Friedman+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/923/197">J/ApJ/923/197 : SNIa observed in H-band with UV-opt. LCs (Ponder+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/925/217">J/ApJ/925/217 : Optical phot. and sp. monitoring of SN 2020sck (Dutta+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/39.46">J/other/PASA/39.46 : Pantheon+ SN Ia redshift and PV Data (Carr+, 2022)</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/938/L22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/938/L22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/938/L22</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/938/L22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/938/L22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/938/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><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/ApJ/938/L22</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/938/L22/fig1</name><description>Swift-UVOT and HCT-UBVRI magnitudes of SN 2011aa</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>JD</name><description>Julian date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>[-10.2/127] Phase (1)</description><unit>d</unit><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Filt</name><description>Filter</description><ucd>meta.id;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>omag</name><description>[14.1/19.4] Observed magnitude in Filt</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_omag</name><description>[0.004/0.3] Uncertainty in omag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/938/L22/list</name><description>List of the spectra (Data behind Figure 2)</description><column><name>sp</name><description>Interactive spectrum plot</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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