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<ri:Resource created="2024-04-05T10:52:52Z" 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>Temporal analysis of GRB precursors in Swift-BAT cat.</title><shortName>J/ApJ/928/152</shortName><identifier>ivo://CDS.VizieR/J/ApJ/928/152</identifier><altIdentifier>doi:10.26093/cds/vizier.19280152</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li L.</name></creator><creator><name>Mao J.</name></creator><date role="Updated">2024-11-06T20:24:20Z</date><date role="Created">2024-04-05T10:52:52Z</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><subject>redshifted</subject><subject>photometry</subject><description>We select 52 long gamma-ray bursts (GRBs) that have precursor activity in the third Swift-BAT catalog. Each episode shown in both the precursors and the main bursts is fitted by the Norris function. We systematically analyze the temporal properties for both the precursors and the main bursts. We do not find any significant difference between the temporal profile of the precursor and that of the main burst. The photon count of the precursor is related to that of the main burst. It is indicated that the precursor and the main burst might have the same physical origin, as the precursor and the main burst follow the same {tau}p-{omega} relation. However, we do not find the explicit relation between the energy release of the precursor and the quiescent time. Some theoretical models, such as the fallback collapsar scenario and the jet-cocoon scenario, may be helpful to explain the GRB-precursor phenomena.</description><source format="bibcode">2022ApJ...928..152L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/928/152</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/J/ApJS/175/179">J/ApJS/175/179 : The BAT1 gamma-ray burst catalog (Sakamoto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/448/2624">J/MNRAS/448/2624 : List of isolated emission episodes in GRB (Charisi+, 2015)</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/ApJ/866/97">J/ApJ/866/97 : Swift X-ray flash &amp; rich GRBs in BAT3 (Bi+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/862/155">J/ApJ/862/155 : Two-episode prompt emission of GRB with Fermi (Lan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/59">J/ApJ/884/59 : GRB X-ray flare temporal &amp; spectral properties (Liu+, 2019)</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/928/152</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/928/152</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/928/152</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/928/152</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/928/152</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/928/152</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/928/152/table3 (The quiescent time and the peak time)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/928/152/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/928/152/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/928/152/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>306.475417</ra><dec>-42.600608</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/140 207 314 500 646 2336 4449 4485 5726 5840 6521 7589 9321 9643 9897 10704 12006 13312 13694 15530 16991 17561 18494 18945 18978 20710 22129 25131 25946 26011 27284 27566 28032 29731 31494 31607 33004 33735 34435 34440 36374 36468 37383 38926 39076 40433 42901 43920 44436 45008 47148 47459</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/928/152?format=ascii</footprint><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/928/152/table3</name><description>The quiescent time and the peak time</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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