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<ri:Resource created="2016-02-03T12:59:42Z" 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>R-band PTF observations of SNe IIb</title><shortName>J/ApJ/811/117</shortName><identifier>ivo://CDS.VizieR/J/ApJ/811/117</identifier><altIdentifier>doi:10.26093/cds/vizier.18110117</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Strotjohann N.L.</name></creator><creator><name>Ofek E.O.</name></creator><creator><name>Gal-Yam A.</name></creator><creator><name>Sullivan M.</name></creator><creator><name>Kulkarni S.R.,Shaviv N.J.</name></creator><creator><name>Fremling C.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Nugent P.E.</name></creator><creator><name>Cao Y.</name></creator><creator><name>Arcavi I.,Sollerman J.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Yaron O.</name></creator><creator><name>Laher R.</name></creator><creator><name>Surace J.</name></creator><date role="Updated">2017-10-18T08:24:16Z</date><date role="Created">2016-02-03T12:59:42Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>redshifted</subject><description>The progenitor stars of several Type IIb supernovae (SNe) show indications of extended hydrogen envelopes. These envelopes might be the outcome of luminous energetic pre-explosion events, so-called precursor eruptions. We use the Palomar Transient Factory (PTF) pre-explosion observations of a sample of 27 nearby SNe IIb to look for such precursors during the final years prior to the SN explosion. No precursors are found when combining the observations in 15-day bins, and we calculate the absolute-magnitude-dependent upper limit on the precursor rate. At the 90% confidence level, SNe IIb have on average &lt;0.86 precursors as bright as an absolute R-band magnitude of -14 in the final 3.5 years before the explosion and &lt;0.56 events over the final year. In contrast, precursors among SNe IIn have a &gt;~5 times higher rate. The kinetic energy required to unbind a low-mass stellar envelope is comparable to the radiated energy of a few-weeks-long precursor that would be detectable for the closest SNe in our sample. Therefore, mass ejections, if they are common in such SNe, are radiatively inefficient or have durations longer than months. Indeed, when using 60-day bins, a faint precursor candidate is detected prior to SN 2012cs (~2% false-alarm probability). We also report the detection of the progenitor of SN 2011dh that does not show detectable variability over the final two years before the explosion. The suggested progenitor of SN 2012P is still present, and hence is likely a compact star cluster or an unrelated object.</description><source format="bibcode">2015ApJ...811..117S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/811/117</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/II/313">II/313 : Palomar Transient Factory (PTF) photometric catalog 1.0 (Ofek+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A142">J/A+A/580/A142 : SN 2011dh. The first two years (Ergon+, 2015)</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/other/Nat/494.65">J/other/Nat/494.65 : SN 2010mc outburst before explosion (Ofek+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/L19">J/ApJ/778/L19 : SN 2011dh (type IIb) 3.6 &amp; 4.5um light curves (Helou+, 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/ApJ/742/L18">J/ApJ/742/L18 : Follow-up photometry of the SN IIb PTF 11eon (Arcavi+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PZ/29.2">J/other/PZ/29.2 : SN 2008ax UBVRI light curves (Tsvetkov+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/696/870">J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)</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/811/117</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/811/117</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/811/117</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/811/117</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/811/117</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/811/117</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/811/117/table1 (Supernova sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/811/117/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/811/117/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/811/117/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>347.144705</ra><dec>18.93713111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/539 543 2261 7234 7766 8195 8754 9620 10189 10544 10574 11027 11693 13570 17525 19201 19526 19979 19991 20009 20116 26806 27803 27913 28529 28538 36729</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/811/117?format=ascii</footprint><waveband>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/811/117/table1</name><description>Supernova sample</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>l_Name</name><description>[l] l: SN added to our sample from the literature</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>SN identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>primary</flag></column><column><name>PTF</name><description>Other PTF name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>[0.0016/0.05] SN redshift obtained from spectroscopy</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DM</name><description>[29.4/36.8] Distance modulus (1)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>[0.01/0.2] Galactic extinction taken from Schlegel et al. 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