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<ri:Resource created="2021-12-02T14:37:35Z" 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>Swift BAT gamma-ray burst durations</title><shortName>J/ApJ/896/L20</shortName><identifier>ivo://CDS.VizieR/J/ApJ/896/L20</identifier><altIdentifier>doi:10.26093/cds/vizier.18969020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jespersen C.K.</name></creator><creator><name>Severin J.B.</name></creator><creator><name>Steinhardt C.L.</name></creator><creator><name>Vinther J.</name></creator><creator><name>Fynbo J.P.U.,Selsing J.</name></creator><creator><name>Watson D.</name></creator><date role="Updated">2022-03-21T07:00:25Z</date><date role="Created">2021-12-02T14:37:35Z</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>gamma-ray-astronomy</subject><subject>gamma-ray-bursts</subject><description>The duration of a gamma-ray burst (GRB) is a key indicator of its physical origin, with long bursts perhaps associated with the collapse of massive stars and short bursts with mergers of neutron stars. However, there is substantial overlap in the properties of both short and long GRBs and neither duration nor any other parameter so far considered completely separates the two groups. Here we unambiguously classify every GRB using a machine-learning dimensionality reduction algorithm, t-distributed stochastic neighborhood embedding, providing a catalog separating all Swift GRBs into two groups. Although the classification takes place only using prompt emission light curves, every burst with an associated supernova is found in the longer group and bursts with kilonovae in the short, suggesting along with the duration distributions that these two groups are truly long and short GRBs. Two bursts with a clear absence of a supernova belong to the longer class, indicating that these might have been direct-collapse black holes, a proposed phenomenon that may occur in the deaths of more massive stars.</description><source format="bibcode">2020ApJ...896L..20J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/896/L20</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/swift">B/swift : Swift Master Catalog (HEASARC, 2004-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/20">IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/495">J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/103">J/ApJ/731/103 : Redshift catalog for Swift long GRBs (Xiao+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A19">J/A+A/568/A19 : Photometry of 3 {gamma}-ray burst supernovae (Cano+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/110">J/ApJ/818/110 : Short GRBs with Fermi GBM and Swift BAT (Burns+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/828/36">J/ApJ/828/36 : GRB light-curve decay indices with Swift (Del Vecchio+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/829/7">J/ApJ/829/7 : 3rd Swift/BAT GRB catalog (past ~11yrs) (BAT3) (Lien+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/609/A112">J/A+A/609/A112 : Bulk Lorentz factors of gamma-ray bursts (Ghirlanda+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/248/21">J/ApJS/248/21 : Swift long gamma-ray bursts (Hao+, 2020)</relatedResource><relatedResource>http://swift.gsfc.nasa.gov/results/batgrbcat/ : Online Swift BAT GRB catalog</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/896/L20</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/896/L20</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/896/L20</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/896/L20</accessURL><mirrorURL title="VizieR at 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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>GRB</name><description>Gamma-ray burst given name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>m_GRB</name><description>[1/2]? Multiplicity number for GRB140716A</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>T90</name><description>[0.01/811]? 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