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<ri:Resource created="2015-12-08T11:47:20Z" 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>Si and Ca high-velocity features in SNe Ia</title><shortName>J/ApJS/220/20</shortName><identifier>ivo://CDS.VizieR/J/ApJS/220/20</identifier><altIdentifier>doi:10.26093/cds/vizier.22200020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhao X.</name></creator><creator><name>Wang X.</name></creator><creator><name>Maeda K.</name></creator><creator><name>Sai H.</name></creator><creator><name>Zhang T.</name></creator><creator><name>Zhang J.</name></creator><creator><name>Huang F.</name></creator><creator><name>Rui L.,Zhou Q.</name></creator><creator><name>Mo J.</name></creator><date role="Updated">2017-12-18T07:57:39Z</date><date role="Created">2015-12-08T11:47:20Z</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>spectroscopy</subject><subject>line-intensities</subject><description>The high-velocity features (HVFs) in optical spectra of type Ia supernovae (SNe Ia) are examined with a large sample including very early-time spectra (e.g., t&lt;-7days). Multiple Gaussian fits are applied to examine the HVFs and their evolutions, using constraints on expansion velocities for the same species (i.e., SiII5972 and SiII6355). We find that strong HVFs tend to appear in SNe Ia with smaller decline rates (e.g., {Delta}m_15_(B)&lt;~1.4mag), clarifying that the finding by Childress et al. (2014MNRAS.437..338C) for the Ca-HVFs in near-maximum-light spectra applies both to the Si-HVFs and Ca-HVFs in the earlier phase. The Si-HVFs seem to be more common in rapidly expanding SNe Ia, which is different from the earlier result that Ca-HVFs are associated with SNe Ia that have slower SiII6355 velocities at maximum light (i.e., V^Si^_max_). Moreover, SNe Ia with both stronger HVFs at early phases and larger V^Si^_max_ are found to have noticeably redder B-V colors and to occur preferentially in the inner regions of their host galaxies, while those with stronger HVFs but smaller V^Si^_max_ show opposite tendencies, suggesting that these two subclasses have different explosion environments and their HVFs may have different origins. We further examine the relationships between the absorption features of SiII6355 and CaII IR lines, and find that their photospheric components are well correlated in velocity and strength but that the corresponding HVFs show larger scatter. These results cannot be explained with ionization and/or thermal processes alone, and different mechanisms are required for the creation of HVF-forming regions in SNe Ia.</description><source format="bibcode">2015ApJS..220...20Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/220/20</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/578/A9">J/A+A/578/A9 : Optical and NIR spectra of SN iPTF13ebh (Hsiao+, 2015)</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/AJ/148/1">J/AJ/148/1 : Optical and ultraviolet photometry of SN 2012fr (Zhang+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/773/53">J/ApJ/773/53 : Type Ia SNe spectroscopy by the CSP (Folatelli+, 2013)</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/other/Sci/340.170">J/other/Sci/340.170 : Classifications of 188 SNe Ia (Wang+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1819">J/MNRAS/425/1819 : Berkeley supernova Ia program. 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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>IAU SN Ia designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</flag></column><column><name>Nf</name><description>Number of SiII/CaII fit for this SN (tables 3,4,5)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SubCl</name><description>Wang et al. subclassification (2009ApJ...699L.139W) (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>m15B</name><description>[0.6/2]? 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Recession velocity in 3K CMB ref frame</description><unit>km/s</unit><ucd>phys.veloc;pos.frame;pos.cmb</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MType</name><description>Morphological Hubble type of host galaxy</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>DType</name><description>[-5/10]? Digital Hubble type of host galaxy</description><ucd>meta.note;src.morph.type</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rsn</name><description>[0.02/2.5]? Projected galactocentric distance of the SN in its host galaxy, in units of the galaxy radius (Rsn/Rgal)</description><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KMAG</name><description>[-26.3/-20.4]? Galaxy absolute K magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_KMAG</name><description>[0.07/1]? uncertainty on KMAG</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HVF</name><description>Subclassifications of high velocity features, based on Rhvf from SiII 6355 absorption ("IB", "strong" or "weak")</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Rf(Si6355)e</name><description>[0/1]? Rhvf from SiII 6355 absorption; at early phases -- t~-8d (2)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rf(CaIR)e</name><description>[0.1/12.5]? Rhvf from CaII IR triplet; at early phases, t~-8d (2)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rf(CaIR)m</name><description>[0/2.1]? 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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>IAU SN Ia designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Phase</name><description>Days since the B-band maximum light</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VSi6355</name><description>[9153/17110] Photospheric velocity of SiII6355 absorption</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWSi6355</name><description>[15/210] Pseudo-Equivalent width of the photospheric component of SiII6355 absorption</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VfSi6355</name><description>[16000/24000] Velocity of the high-velocity feature of SiII 6355 absorption</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWfSi6355</name><description>[0/125] Pseudo-Equivalent width of the high-velocity feature of SiII 6355</description><unit>0.1nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rf(Si6355)</name><description>[0/5.3] Ratio of pEWf to pEW</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VSi5972</name><description>[9500/16915] Photospheric velocity of SiII5972</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWSi5972</name><description>[0/66] Pseudo-Equivalent width of photospheric component of SiII 5972</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJS/220/20/table4</name><description>Fit results of the CaII IR triplet of Sample B (47 SNe)</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>SN</name><description>IAU SN Ia designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Phase</name><description>Days since the B-band maximum light</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VCaIR</name><description>[9756/16010] Velocity of the photospheric components of CaII IR triplet</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWCaIR</name><description>[5/186] Pseudo-Equivalent width of the photospheric components of CaII IR triplet</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VfCaIR</name><description>[19503/27299] Velocity of the high-velocity feature components of CaII IR triplet</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWfCaIR</name><description>[8/331] Pseudo-Equivalent width of the high-velocity feature components of CaII IR triplet</description><unit>0.1nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rf(CaIR)</name><description>[0.2/17] Ratio of pEWf to pEW</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJS/220/20/table5</name><description>Fit results of the SiII 6355 and CaII IR absorptions from Sample C (126 SNe)</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>SN</name><description>IAU SN Ia designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Phase</name><description>Days since the B-band maximum light</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VSi6355</name><description>[8500/15059] Velocity of the photospheric components of SiII 6355 absorption</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWSi6355</name><description>[50/190] Pseudo-Equivalent width of the photospheric component of SiII 6355 absorption</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VCaIR</name><description>[7799/15418] Velocity of the photospheric components of CaII IR triplet</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWCaIR</name><description>[33/230] Pseudo-Equivalent width of the photospheric components of CaII IR triplet</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VfCaIR</name><description>[15806/34116] Velocity of the high-velocity feature components of CaII IR triplet</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pEWfCaIR</name><description>[0/196] Pseudo-Equivalent width of the high-velocity feature components of CaII IR triplet</description><unit>0.1nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rf(CaIR)</name><description>[0/2.1] Ratio of pEWhvf to pEWpho</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>