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<ri:Resource created="2015-02-10T13:36:40Z" 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>Redshifts of 65 CANDELS supernovae</title><shortName>J/AJ/148/13</shortName><identifier>ivo://CDS.VizieR/J/AJ/148/13</identifier><altIdentifier>doi:10.26093/cds/vizier.51480013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rodney S.A.</name></creator><creator><name>Riess A.G.</name></creator><creator><name>Strolger L.-G.</name></creator><creator><name>Dahlen T.</name></creator><creator><name>Graur O.</name></creator><creator><name>Casertano S.,Dickinson M.E.</name></creator><creator><name>Ferguson H.C.</name></creator><creator><name>Garnavich P.</name></creator><creator><name>Hayden B.</name></creator><creator><name>Jha S.W.,Jones D.O.</name></creator><creator><name>Kirshner R.P.</name></creator><creator><name>Koekemoer A.M.</name></creator><creator><name>McCully C.</name></creator><creator><name>Mobasher B.,Patel B.</name></creator><creator><name>Weiner B.J.</name></creator><creator><name>Cenko S.B.</name></creator><creator><name>Clubb K.I.</name></creator><creator><name>Cooper M.</name></creator><creator><name>Filippenko A.V.,Frederiksen T.F.</name></creator><creator><name>Hjorth J.</name></creator><creator><name>Leibundgut B.</name></creator><creator><name>Matheson T.</name></creator><creator><name>Nayyeri H.,Penner K.</name></creator><creator><name>Trump J.</name></creator><creator><name>Silverman J.M.</name></creator><creator><name>U V.</name></creator><creator><name>Azalee Bostroem K.</name></creator><creator><name>Challis P.,Rajan A.</name></creator><creator><name>Wolff S.</name></creator><creator><name>Faber S.M.</name></creator><creator><name>Grogin N.A.</name></creator><creator><name>Kocevski D.</name></creator><date role="Updated">2020-08-07T07:23:39Z</date><date role="Created">2015-02-10T13:36:40Z</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>redshifted</subject><subject>galaxy-classification-systems</subject><description>The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) was a multi-cycle treasury program on the Hubble Space Telescope (HST) that surveyed a total area of ~0.25deg^2^ with ~900 HST orbits spread across five fields over three years. Within these survey images we discovered 65 supernovae (SNe) of all types, out to z~2.5. We classify ~24 of these as Type Ia SNe (SNe Ia) based on host galaxy redshifts and SN photometry (supplemented by grism spectroscopy of six SNe). Here we present a measurement of the volumetric SN Ia rate as a function of redshift, reaching for the first time beyond z=2 and putting new constraints on SN Ia progenitor models. Our highest redshift bin includes detections of SNe that exploded when the universe was only ~3Gyr old and near the peak of the cosmic star formation history. This gives the CANDELS high redshift sample unique leverage for evaluating the fraction of SNe Ia that explode promptly after formation (&lt;500Myr). Combining the CANDELS rates with all available SN Ia rate measurements in the literature we find that this prompt SN Ia fraction is f_p_=0.53_stat0.10sys0.26_^+/-0.09 +/-0.10^, consistent with a delay time distribution that follows a simple t^-1^ power law for all times t&gt;40Myr. However, mild tension is apparent between ground-based low-z surveys and space-based high-z surveys. In both CANDELS and the sister HST program CLASH (Cluster Lensing And Supernova Survey with Hubble), we find a low rate of SNe Ia at z&gt;1. This could be a hint that prompt progenitors are in fact relatively rare, accounting for only 20% of all SN Ia explosions--though further analysis and larger samples will be needed to examine that suggestion.</description><source format="bibcode">2014AJ....148...13R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/148/13</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/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/25">J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/31">J/ApJ/745/31 : HST Cluster Supernova Survey. 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Host galaxy hour of Right Ascension (J2000)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEG</name><description>? Host galaxy degree of Declination (J2000)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>ASep</name><description>? Angular separation (d)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PSep</name><description>? Physical separation (d) (5)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MType</name><description>Visual classification for host galaxy morphology: s=spheroid, d=disk, i=irregular</description><ucd>meta.code;src.morph</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>SED</name><description>Template-matching classification of host galaxy SED: P=passive, A=active, SB=starburst</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>zhost</name><description>? Redshift of host galaxy</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_zhost</name><description>? Uncertainty in zhost</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zhost</name><description>Reference for zhost; in refs.dat file</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>f_zhost</name><description>Indicates an host galaxy photometric redshift (6)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Inst1</name><description>Instrument used for unpublished spectroscopic observation</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>PI1</name><description>Name of PI for unpublished spectroscopic observation</description><ucd>obs.observer</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column></table></schema></tableset></ri:Resource>