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<ri:Resource created="2023-08-28T10:29:24Z" 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>Energies of X-ray plateaus and flares in GRBs</title><shortName>J/ApJ/924/69</shortName><identifier>ivo://CDS.VizieR/J/ApJ/924/69</identifier><altIdentifier>doi:10.26093/cds/vizier.19240069</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yi S.-X.</name></creator><creator><name>Du M.</name></creator><creator><name>Liu T.</name></creator><date role="Updated">2023-11-03T13:25:45Z</date><date role="Created">2023-08-28T10:29:24Z</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>x-ray-sources</subject><subject>spectral-energy-distribution</subject><description>Distinct X-ray plateau and flare phases have been observed in the afterglows of gamma-ray bursts (GRBs), and most of them should be related to central engine activities. In this paper, we collect 174 GRBs with X-ray plateau phases and 106 GRBs with X-ray flares. There are 51 GRBs that overlap in the two selected samples. We analyze the distributions of the proportions of the plateau energy Eplateau and the flare energy E_flare_ relative to the isotropic prompt emission energy E_{gamma},iso_. The results indicate that they well meet the Gaussian distributions and the medians of the logarithmic ratios are ~-0.96 and -1.39 in the two cases. Moreover, strong positive correlations between E_plateau_ (or E_flare_) and E_{gamma},iso_ with slopes of ~0.95 (or ~0.80) are presented. For the overlapping sample, the slope is ~0.80. We argue that most of X-ray plateaus and flares might have the same physical origin but appear with different features because of the different circumstances and radiation mechanisms. We also test the applicabilities of two models, i.e., black holes surrounded by fractured hyperaccretion disks and millisecond magnetars, on the origins of X-ray plateaus and flares.</description><source format="bibcode">2022ApJ...924...69Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/924/69</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/MNRAS/418/2202">J/MNRAS/418/2202 : Analysis of {gamma}-ray bursts (Dainotti+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/157">J/ApJ/774/157 : Swift GRBs with X-ray afterglows and z&lt;9.5 (Dainotti+, 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/227/7">J/ApJS/227/7 : Long &amp; short GRBs with host galaxies data (Li+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/20">J/ApJS/224/20 : 10yr of Swift/XRT obs. of GRBs (Yi+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/852/53">J/ApJ/852/53 : Early X-ray flares in GRBs (Ruffini+, 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 ivo-id="ivo://CDS.VizieR/J/MNRAS/492/1919">J/MNRAS/492/1919 : Type I GRBs &amp; the new classification method (Minaev+, 2020)</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/924/69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/924/69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/924/69</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/924/69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/924/69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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