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<ri:Resource created="2018-01-15T14:21:02Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Short GRBs with Fermi GBM and Swift BAT</title><shortName>J/ApJ/818/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/110</identifier><altIdentifier>doi:10.26093/cds/vizier.18180110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Burns E.</name></creator><creator><name>Connaughton V.</name></creator><creator><name>Zhang B.-B.</name></creator><creator><name>Lien A.</name></creator><creator><name>Briggs M.S.</name></creator><creator><name>Goldstein A.,Pelassa V.</name></creator><creator><name>Troja E.</name></creator><date role="Updated">2018-03-12T09:26:21Z</date><date role="Created">2018-01-15T14:21:02Z</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><description>Compact binary system mergers are expected to generate gravitational radiation detectable by ground-based interferometers. A subset of these, the merger of a neutron star with another neutron star or a black hole, are also the most popular model for the production of short gamma-ray bursts (GRBs). The Swift Burst Alert Telescope (BAT) and the Fermi Gamma-ray Burst Monitor (GBM) trigger on short GRBs (SGRBs) at rates that reflect their relative sky exposures, with the BAT detecting 10 per year compared to about 45 for GBM. We examine the SGRB populations detected by Swift BAT and Fermi GBM.</description><source format="bibcode">2016ApJ...818..110B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/110</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/18">J/ApJS/199/18 : The Fermi GBM catalog (Paciesas+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/15">J/ApJ/763/15 : Fermi GRB analysis. III. T_90_ distributions (Qin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/66">J/ApJ/787/66 : Burst duration measurements for a GRB sample (Zhang+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/216/32">J/ApJS/216/32 : Localizations of GRBs with Fermi GBM (Connaughton+, 2015)</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/818/110</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/818/110</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/818/110</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/818/110</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/818/110</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/818/110</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/818/110/table1</name><description>GBM SGRBs as viewed by BAT</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">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>Trig</name><description>? 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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>SGRB name (&lt;GRB YYMMDDA&gt; in SIMBAD) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Trig</name><description>? 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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>? 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