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<ri:Resource created="2021-07-22T08:56:19Z" 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>SNe Ic from (i)PTF light curves</title><shortName>J/A+A/651/A81</shortName><identifier>ivo://CDS.VizieR/J/A+A/651/A81</identifier><altIdentifier>doi:10.26093/cds/vizier.36510081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barbarino C.</name></creator><creator><name>Sollerman J.</name></creator><creator><name>Taddia F.</name></creator><creator><name>Fremling C.</name></creator><creator><name>Karamehmetoglu E.,Arcavi I.</name></creator><creator><name>Gal-Yam A.</name></creator><creator><name>Laher R.</name></creator><creator><name>Schulze S.</name></creator><creator><name>Wozniak P.</name></creator><creator><name>Yan L.</name></creator><date role="Updated">2023-01-11T14:18:17Z</date><date role="Created">2021-07-22T08:56:19Z</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>photometry</subject><description>Type Ic supernovae represent the explosions of the most stripped massive stars, but their progenitors and explosion mechanisms remain unclear. Larger samples of observed supernovae can help characterize the population of these transients. We present an analysis of 44 spectroscopically normal Type Ic supernovae, with focus on the light curves. The photometric data were obtained over 7 years with the Palomar Transient Factory (PTF) and its continuation, the intermediate Palomar TransientFactory (iPTF). 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