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<ri:Resource created="2017-03-13T12:46:09Z" status="active" updated="2025-06-13T15:25:00Z" 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 SN host galaxies</title><shortName>J/ApJ/789/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/789/23</identifier><altIdentifier>doi:10.26093/cds/vizier.17890023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kelly P.L.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Modjaz M.</name></creator><creator><name>Kocevski D.</name></creator><date role="Updated">2017-12-15T10:54:44Z</date><date role="Created">2017-03-13T12:46:09Z</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>galaxies</subject><subject>catalogs</subject><subject>supernovae</subject><subject>gamma-ray-astronomy</subject><subject>redshifted</subject><description>Spectra of broad-lined Type Ic supernovae (SNe Ic-BL), the only kind of SN observed at the locations of long-duration gamma-ray bursts (LGRBs), exhibit wide features indicative of high ejecta velocities (~0.1c). We study the host galaxies of a sample of 245 low-redshift (z &lt; 0.2) core-collapse SNe, including 17 SNe Ic-BL, discovered by galaxy-untargeted searches, and 15 optically luminous and dust-obscured z &lt; 1.2 LGRBs. We show that, in comparison with Sloan Digital Sky Survey galaxies having similar stellar masses, the hosts of low-redshift SNe Ic-BL and z &lt; 1.2 LGRBs have high stellar mass and star formation rate densities. Core-collapse SNe having typical ejecta velocities, in contrast, show no preference for such galaxies. Moreover, we find that the hosts of SNe Ic-BL, unlike those of SNe Ib/Ic and SNe II, exhibit high gas velocity dispersions for their stellar masses. The patterns likely reflect variations among star-forming environments and suggest that LGRBs can be used as probes of conditions in high-redshift galaxies. They may be caused by efficient formation of massive binary progenitor systems in densely star-forming regions, or, less probably, a higher fraction of stars created with the initial masses required for an SN Ic-BL or LGRB. Finally, we show that the preference of SNe Ic-BL and LGRBs for galaxies with high stellar mass and star formation rate densities cannot be attributed to a preference for low metal abundances but must reflect the influence of a separate environmental factor.</description><source format="bibcode">2014ApJ...789...23K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/789/23</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/ApJ/673/999">J/ApJ/673/999 : Supernova and host galaxies metallicities (Prieto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/566">J/ApJ/722/566 : Host galaxies of SNe Ia in SDSS-II SN survey</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/92">J/ApJ/740/92 : SN.Ia host galaxies properties (Gupta+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A81">J/A+A/544/A81 : Supernovae and their hosts in the SDSS DR8 (Hakobyan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/61">J/ApJ/755/61 : SN Ia host galaxies SFR from SDSS-II (Smith+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/107">J/ApJ/759/107 : Core-collapse SNe and host galaxies (Kelly+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2841">J/MNRAS/424/2841 : Morphology of supernova host galaxies (Habergham+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/107">J/ApJ/770/107 : Host galaxies of SNIa from SNfactory (Childress+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/1680">J/MNRAS/435/1680 : SN Ia host galaxy properties (Johansson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/438/1391">J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)</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/448/732">J/MNRAS/448/732 : Type Ia SN environment within host galaxies (Anderson+ 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/115">J/ApJ/821/115 : SDSS-II SN Survey: host-galaxy spectral data (Wolf+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/830/13">J/ApJ/830/13 : Host-galaxy 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