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<ri:Resource created="2024-02-29T08:22:05Z" 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>Radio flux measurements of type Ib/c &amp; II SNe</title><shortName>J/ApJ/908/75</shortName><identifier>ivo://CDS.VizieR/J/ApJ/908/75</identifier><altIdentifier>doi:10.26093/cds/vizier.19080075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bietenholz M.F.</name></creator><creator><name>Bartel N.</name></creator><creator><name>Argo M.</name></creator><creator><name>Dua R.</name></creator><creator><name>Ryder S.</name></creator><creator><name>Soderberg A.</name></creator><date role="Updated">2025-02-13T20:11:19Z</date><date role="Created">2024-02-29T08:22:05Z</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>radio-spectroscopy</subject><description>We assemble a large set of 2-10GHz radio flux density measurements and upper limits of 294 different supernovae (SNe), from the literature and our own and archival data. Only 31% of SNe were detected. We characterize the SN radio lightcurves near the peak using a two-parameter model, with tpk being the time to rise to a peak and Lpk the spectral luminosity at that peak. Over all SNe in our sample at D&lt;100Mpc, we find that tpk=10^1.7+/-0.9^days and that Lpk=10^25.5+/-1.6^erg/s/Hz, and therefore that generally 50% of SNe will have Lpk&lt;10^25.5^erg/s/Hz. These Lpk values are ~30 times lower than those for only detected SNe. Types Ib/c and II (excluding IIn's) have similar mean values of Lpk but the former have a wider range, whereas Type IIn SNe have ~10 times higher values with Lpk=10^26.5+/-1.1^erg/s/Hz. As for tpk, Type Ib/c have tpk of only 10^1.1+/-0.5^days while Type II have tpk=10^1.6+/-1.0^ and Type IIn the longest timescales with tpk=10^3.1+/-0.7^days. We also estimate the distribution of progenitor mass-loss rates, M, and find that the mean and standard deviation of log(dM/dt/M_{sun}_yr^-1^) are -5.4+/-1.2 (assuming v_wind_=1000km/s) for Type Ib/c SNe, and -6.9+/-1.4 (assuming v_wind_=10km/s) for Type II SNe excluding Type IIn.</description><source format="bibcode">2021ApJ...908...75B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/908/75</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/J/MNRAS/412/1441">J/MNRAS/412/1441 : SNe luminosity functions (Li+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/747/L5">J/ApJ/747/L5 : R-band observations of PTF 10vgv (Corsi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/57">J/ApJ/821/57 : Photometry of the Type Ib/c SN2013ge (Drout+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/593/A18">J/A+A/593/A18 : SN 2008iz 4.8 and 8.4GHz images (Kimani+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/863/163">J/ApJ/863/163 : Type IIP supernova SN 2004dj radio obs (Nayana+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/887/169">J/ApJ/887/169 : UV-Opt light curves of the type Ic SN 2018gep (Ho+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/147">J/ApJ/883/147 : UV-NIR LC of energetic Hstripped SN2016coi (Terreran+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/893/132">J/ApJ/893/132 : Optical follow-up of SNIc ZTF18aaqjovh (Ho+, 2020)</relatedResource><relatedResource 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