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<ri:Resource created="2022-10-25T12:25:05Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>KMTNet BVi photometry of SNIa KSP-OT-201509b</title><shortName>J/ApJ/910/151</shortName><identifier>ivo://CDS.VizieR/J/ApJ/910/151</identifier><altIdentifier>doi:10.26093/cds/vizier.19100151</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moon D.-S.</name></creator><creator><name>Ni Y.Qi</name></creator><creator><name>Drout M.R.</name></creator><creator><name>Gonzalez-Gaitan S.</name></creator><creator><name>Afsariardchi N.,Park H.S.</name></creator><creator><name>Lee Y.</name></creator><creator><name>Kim S.C.</name></creator><creator><name>Antoniadis J.</name></creator><creator><name>Kim D.-J.</name></creator><creator><name>Lee Y.</name></creator><date role="Updated">2022-11-25T13:34:09Z</date><date role="Created">2022-10-25T12:25:05Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We report the early discovery and multicolor (BVI) high-cadence light-curve analyses of the rapidly declining sub-Chandrasekhar Type Ia supernova KSP-OT-201509b (= AT 2015cx) from the KMTNet Supernova Program. The Phillips and color stretch parameters of KSP-OT-201509b are {Delta}M_B,15_~1.62mag and s_BV_~0.54, respectively, at an inferred redshift of 0.072. These, together with other measured parameters (such as the strength of the secondary I-band peak, colors, and luminosity), identify the source to be a rapidly declining Type Ia of a transitional nature that is closer to Branch-normal than 91bg-like. Its early light-curve evolution and bolometric luminosity are consistent with those of homologously expanding ejecta powered by radioactive decay and a Type Ia SN explosion with 0.32+/-0.01M_{sun}_ of synthesized ^56^Ni mass, 0.84+/-0.12M_{sun}_ of ejecta mass, and (0.61+/-0.14)x10^51^erg of ejecta kinetic energy. While its B-V and V-I colors evolve largely synchronously with the changes in the I-band light curve, as found in other supernovae, we also find the presence of an early redward evolution in V-I prior to -10 days since peak. The bolometric light curve of the source is compatible with a stratified ^56^Ni distribution extended to shallow layers of the exploding progenitor. Comparisons between the observed light curves and those predicted from ejecta-companion interactions clearly disfavor Roche lobe-filling companion stars at large separation distances, thus supporting a double-degenerate scenario for its origin. The lack of any apparent host galaxy in our deep stack images reaching a sensitivity limit of ~28mag/arcsec^2^ makes KSP-OT-201509b a hostless Type Ia supernova and offers new insights into supernova host galaxy environments.</description><source format="bibcode">2021ApJ...910..151M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/151</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/1485">J/MNRAS/383/1485 : BVRI light curves of SN 2003jd (Valenti+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/519">J/AJ/139/519 : Carnegie supernova project. 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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>MJD</name><description>[57289.89/57359.48] Time, Modified Julian Date (JD-2400000.5)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>omag</name><description>[18.37/22.18] Observed magnitude in Filt (1)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_omag</name><description>[0.016/0.5] Uncertainty in omag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Filt</name><description>[BVi] Band</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>