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<ri:Resource created="2017-01-04T09:04:53Z" 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>Spectroscopy of SNe Ib, IIb and Ic</title><shortName>J/ApJ/827/90</shortName><identifier>ivo://CDS.VizieR/J/ApJ/827/90</identifier><altIdentifier>doi:10.26093/cds/vizier.18270090</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu Y.-Q.</name></creator><creator><name>Modjaz M.</name></creator><creator><name>Bianco F.B.</name></creator><creator><name>Graur O.</name></creator><date role="Updated">2017-06-27T06:38:17Z</date><date role="Created">2017-01-04T09:04:53Z</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>Using the largest spectroscopic data set of stripped-envelope core-collapse supernovae (stripped SNe), we present a systematic investigation of spectral properties of Type IIb SNe (SNe IIb), Type Ib SNe (SNe Ib), and Type Ic SNe (SNe Ic). Prior studies have been based on individual objects or small samples. Here, we analyze 242 spectra of 14 SNe IIb, 262 spectra of 21 SNe Ib, and 207 spectra of 17 SNe Ic based on the stripped SN data set of Modjaz et al. (2016ApJ...832..108M) and other published spectra of individual SNe. Each SN in our sample has a secure spectroscopic ID, a date of V-band maximum light, and most have multiple spectra at different phases. We analyze these spectra as a function of subtype and phase in order to improve the SN identification scheme and constrain the progenitors of different kinds of stripped SNe. By comparing spectra of SNe IIb with those of SNe Ib, we find that the strength of H{alpha} can be used to quantitatively differentiate between these two subtypes at all epochs. Moreover, we find a continuum in observational properties between SNe IIb and Ib. We address the question of hidden He in SNe Ic by comparing our observations with predictions from various models that either include hidden He or in which He has been burnt. Our results favor the He-free progenitor models for SNe Ic. Finally, we construct continuum-divided average spectra as a function of subtype and phase to quantify the spectral diversity of the different types of stripped SNe.</description><source format="bibcode">2016ApJ...827...90L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/827/90</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/ApJ/825/L22">J/ApJ/825/L22 : BVRI LCs of type Ib supernova iPTF13bvn (Folatelli+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/593/A68">J/A+A/593/A68 : PTF12os &amp; iPTF13bvn spectra &amp; light curves (Fremling+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/574/A60">J/A+A/574/A60 : Light curve templates of SNe Ib/c from SDSS (Taddia+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A12">J/A+A/573/A12 : SN1993J spectra 100-500d post-explosion (Jerkstrand+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/19">J/ApJS/213/19 : Optical and near-IR light curves of 64 SNe (Bianco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/99">J/AJ/147/99 : Spectrosc. of 73 stripped core-collapse SNe (Modjaz+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A17">J/A+A/562/A17 : SN 2011dh - The first 100 days (Ergon+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/774">J/MNRAS/436/774 : Core collapse supernovae (type Ibc) (Eldridge+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/308">J/MNRAS/431/308 : SN 2011fu BVRI light curves (Kumar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/1746">J/MNRAS/430/1746 : 90 new SNIa from SDSS DR7 (Graur+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PZ/32.6">J/other/PZ/32.6 : UBVRI light curves of SN 2011dh (Tsvetkov+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1819">J/MNRAS/425/1819 : Berkeley supernova Ia program. 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Uncertainty in VFeII</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VOI</name><description>[-11000/-4440]? O I 7774A velocity (2)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_VOI</name><description>? Uncertainty in VOI</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/827/90/sne</name><description>Spectral sample of SNe IIb, SNe Ib and SNe Ic</description><column><name>ID</name><description>SN Name (SN YYYYaa, iPTF13bvn or PTF12gzk)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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He I 6678A equivalent width (2)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EWHeI6</name><description>? Uncertainty in EWHeI6 (2)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EWHeI7</name><description>[16/148]? He I 7065A equivalent width (2)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EWHeI7</name><description>? Uncertainty in EWHeI7 (2)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EWHa</name><description>[8/216]? 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