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<ri:Resource created="2020-11-24T12:23:08Z" 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 407 SNe and their 394 hosts</title><shortName>J/MNRAS/499/1424</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/499/1424</identifier><altIdentifier>doi:10.26093/cds/vizier.74991424</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hakobyan A.A.</name></creator><creator><name>Barkhudaryan L.V.</name></creator><creator><name>Karapetyan A.G.</name></creator><creator><name>Gevorgyan M.H.,Mamon G.A.</name></creator><creator><name>Kunth D.</name></creator><creator><name>Adibekyan V.</name></creator><creator><name>Turatto M.</name></creator><date role="Updated">2024-08-21T20:16:19Z</date><date role="Created">2020-11-24T12:23:08Z</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>visible-astronomy</subject><subject>catalogs</subject><subject>surveys</subject><description>We present an analysis of the light curve (LC) decline rates ({DELTA}m_15_) of 407 normal and peculiar supernovae (SNe) Ia and global parameters of their host galaxies. As previously known, there is a significant correlation between the {DELTA}m_15_ of normal SNe Ia and global ages (morphologies, colours, and masses) of their hosts. On average, those normal SNe Ia that are in galaxies from the Red Sequence (early-type, massive, old hosts) have faster declining LCs in comparison with those from the Blue Cloud (late-type, less massive, younger hosts) of the colour-mass diagram. The observed correlations between the {DELTA}m_15_ of normal SNe Ia and hosts' parameters appear to be due to the superposition of at least two distinct populations of faster and slower declining normal SNe Ia from older and younger stellar components. We show, for the first time, that the {DELTA}m_15_ of 91bg- and 91T-like SNe is independent of host morphology and colour. The distribution of hosts on the colour-mass diagram confirms the known tendency for 91bg-like SNe to occur in globally red/old galaxies, while 91T-like events prefer blue/younger hosts. On average, the youngest global ages of 02cx-like SNe hosts and their positions in the colour-mass diagram hint that these events likely originate from young population, but they differ from 91T-like events in the LC decline rate. Finally, we discuss the possible explosion channels and present our favoured SN Ia models that have the potential to explain the observed SN-host relations.</description><source format="bibcode">2020MNRAS.499.1424H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/499/1424</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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A81">J/A+A/544/A81 : Supernovae and their hosts in SDSS DR8 (Hakobyan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/2428">J/MNRAS/444/2428 : Disturbance levels of SNe host galaxies (Hakobyan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/2848">J/MNRAS/456/2848 : Properties of 500 SNe &amp; their 419 hosts (Hakobyan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/471/1390">J/MNRAS/471/1390 : Properties of 102 SNe &amp; their 100 hosts (Hakobyan+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/481/566">J/MNRAS/481/566 : Properties of 333 SNe &amp; their 269 hosts (Karapetyan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/490/718">J/MNRAS/490/718 : Properties of 109 SNe &amp; their 104 hosts(Barkhudaryan+, 2019)</relatedResource><relatedResource>http://www.sdss.org : SDSS Home Page</relatedResource><relatedResource>https://sne.space : The Open Supernova 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(1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><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>SN</name><description>Supernova (SN) designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>r_Type</name><description>Source of SN subclass</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="43*">char</dataType></column><column><name>dm15</name><description>SN light curve (LC) decline rate</description><unit>mag</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dm15</name><description>Error of SN LC decline rate</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_dm15</name><description>Source of SN LC decline rate</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>Gal</name><description>SN host galaxy name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>Dist</name><description>Host galaxy distance</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>umag</name><description>? 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