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<ri:Resource created="2021-09-08T08:17:08Z" 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>Properties of 185 SNe Ia and their 180 hosts</title><shortName>J/MNRAS/505/L52</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/505/L52</identifier><altIdentifier>doi:10.26093/cds/vizier.75059052</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hakobyan A.A.</name></creator><creator><name>Karapetyan A.G.</name></creator><creator><name>Barkhudaryan L.V.</name></creator><creator><name>Gevorgyan M.H.,Adibekyan V.</name></creator><date role="Updated">2024-08-21T20:18:07Z</date><date role="Created">2021-09-08T08:17:08Z</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>galaxies</subject><subject>catalogs</subject><subject>surveys</subject><description>Using a sample of nearby spiral galaxies hosting 185 supernovae (SNe) Ia, we perform a comparative analysis of the locations and light-curve decline rates ({Delta}m_15_) of normal and peculiar SNe Ia in the star formation deserts (SFDs) and beyond. To accomplish this, we present a simple visual classification approach based on the UV/H {alpha} images of the discs of host galaxies. We demonstrate that, from the perspective of the dynamical time-scale of the SFD, where the star formation is suppressed by the bar evolution, the {Delta}m_15_ of SN Ia and progenitor age can be related. The SFD phenomenon gives an excellent possibility to separate a subpopulation of SN Ia progenitors with ages older than a few Gyr. We show, for the first time, that the SFDs contain mostly faster declining SNe Ia ({Delta}m_15_&gt;1.25). For the galaxies without SFDs, the region within the bar radius, and outer disc contain mostly slower declining SNe Ia. 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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>SN</name><description>Supernova (SN) name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Gal</name><description>SN host galaxy name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>MType</name><description>Galaxy morphological type</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>u_MType</name><description>[:?] Uncertainty flag on morphology (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Bar</name><description>[B] Presence of bar in the host galaxy</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>u_Bar</name><description>[:?] Uncertainty flag on bar (2)</description><ucd>meta.code.error;src.morph.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>clDisc</name><description>Star formation (SF) class of galaxy disc (3)</description><ucd>meta.code.class;phys.SFR</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>u_clDisc</name><description>[:?] Uncertainty flag on SF class (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>u_SNloc</name><description>[:] Uncertainty flag on SN location (5)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Rsn</name><description>Deprojected and normalized galactocentric distance of SN</description><ucd>pos.distance;arith.ratio;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rdem</name><description>? Host galaxy demarcation radius</description><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column></table></schema></tableset></ri:Resource>